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3,900
2207.00915
Zoe Xi
Zoe Xi and William Kuszmaul
Approximating Dynamic Time Warping Distance Between Run-Length Encoded Strings
A shorter version of this paper will be published in ESA 2022
null
null
null
cs.DS
http://creativecommons.org/licenses/by/4.0/
Dynamic Time Warping (DTW) is a widely used similarity measure for comparing strings that encode time series data, with applications to areas including bioinformatics, signature verification, and speech recognition. The standard dynamic-programming algorithm for DTW takes $O(n^2)$ time, and there are conditional lower bounds showing that no algorithm can do substantially better. In many applications, however, the strings $x$ and $y$ may contain long runs of repeated letters, meaning that they can be compressed using run-length encoding. A natural question is whether the DTW-distance between these compressed strings can be computed efficiently in terms of the lengths $k$ and $\ell$ of the compressed strings. Recent work has shown how to achieve $O(k\ell^2 + \ell k^2)$ time, leaving open the question of whether a near-quadratic $\tilde{O}(k\ell)$-time algorithm might exist. We show that, if a small approximation loss is permitted, then a near-quadratic time algorithm is indeed possible: our algorithm computes a $(1 + \epsilon)$-approximation for $DTW(x, y)$ in $\tilde{O}(k\ell / \epsilon^3)$ time, where $k$ and $\ell$ are the number of runs in $x$ and $y$. Our algorithm allows for $DTW$ to be computed over any metric space $(\Sigma, \delta)$ in which distances are $O(log(n))$-bit integers. Surprisingly, the algorithm also works even if $\delta$ does not induce a metric space on $\Sigma$ (e.g., $\delta$ need not satisfy the triangle inequality).
[{'version': 'v1', 'created': 'Sat, 2 Jul 2022 22:59:34 GMT'}]
2022-07-05
[array(['Xi', 'Zoe', ''], dtype=object) array(['Kuszmaul', 'William', ''], dtype=object)]
3,901
1010.2249
Richard J. Mathar
Richard J. Mathar
Clebsch--Gordan Coefficients of the Quaternion Group
13 pages. 28 tables with characters, Cayley tables and CG coefficients, 4 figures with Cayley graphs
null
null
null
math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The Clebsch--Gordan coefficients of the Kronecker products of the irreducible representations of the Quaternion Group Q8, of the Generalized Quaternion Groups Q16 and Q32, and of the factor group (Q32 X Q32)/{(1,1),(-1,-1)} are computed as eigenvectors of a well-known matrix of triple-products of the irreducible representations.
[{'version': 'v1', 'created': 'Mon, 11 Oct 2010 21:43:21 GMT'}]
2010-10-13
[array(['Mathar', 'Richard J.', ''], dtype=object)]
3,902
1409.1441
Vladimir Markov
Vladimir Markov, Slava Mazur, and David Saltz
Design and Implementation of Schedule-Based Trading Strategies Based on Uncertainty Bands
null
The Journal of Trading, Fall 2011, Vol. 6, No. 4, pp. 45-52
null
null
q-fin.TR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We propose a design for schedule-based execution trading strategies based on uncertainty bands. This formulation: 1) simplifies strategy specification and implementation; 2) provides for flexible allocation among passive, opportunistic, aggressive, and dark pool crossing execution tactics; 3) allows for rapid enhancements as new optimization methods, scheduling techniques, alpha models, and execution tactics are developed; and 4) yields information at macroscopic (strategic) and microscopic (tactical) levels that is easily published to trading databases and front-end applications.
[{'version': 'v1', 'created': 'Thu, 4 Sep 2014 13:44:15 GMT'}]
2014-09-05
[array(['Markov', 'Vladimir', ''], dtype=object) array(['Mazur', 'Slava', ''], dtype=object) array(['Saltz', 'David', ''], dtype=object)]
3,903
1506.02271
Taro Fujisawa
Taro Fujisawa
Limits of Hodge structures in several variables, II
Since Lemma 2.5 in the previous version was false, several corrections have been made. The main results are the same as in the previous version. Moreover, the presentation are improved
null
null
null
math.AG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The aim of this article is to study degeneration of the variations of Hodge structure associated to a proper K\"ahler semistable morphism. We prove that the weight filtrations constructed in the author's previous paper coincide with the monodromy weight filtrations on the relative log de Rham cohomology groups of a proper K\"ahler semistable morphism. Moreover, we show that the limiting mixed Hodge structures form admissible variations of mixed Hodge structure.
[{'version': 'v1', 'created': 'Sun, 7 Jun 2015 14:36:34 GMT'} {'version': 'v2', 'created': 'Mon, 12 Jun 2017 05:45:07 GMT'}]
2017-06-13
[array(['Fujisawa', 'Taro', ''], dtype=object)]
3,904
1908.11218
Adam Anderson
Adam Anderson and Steven R. Young and F. Kyle Reed and Jason M. Vann
Deep Modulation (Deepmod): A Self-Taught PHY Layer for Resilient Digital Communications
8 pages
null
null
null
eess.SP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Traditional physical (PHY) layer protocols contain chains of signal processing blocks that have been mathematically optimized to transmit information bits efficiently over noisy channels. Unfortunately, this same optimality encourages ubiquity in wireless communication technology and enhances the potential for catastrophic cyber or physical attacks due to prolific knowledge of underlying physical layers. Additionally, optimal signal processing for one channel medium may not work for another without significant changes in the software protocol. Any truly resilient communications protocol must be capable of immediate redeployment to meet quality of service (QoS) demands in a wide variety of possible channel media. Contrary to many traditional approaches which use immutable man-made signal processing blocks, this work proposes generating real-time blocks {\it ad hoc} through a machine learning framework, so-called deepmod, that is only relevant to the particular channel medium being used. With this approach, traditional signal processing blocks are replaced with machine learning graphs which are trained, used, and discarded as needed. Our experiments show that deepmod, using the same machine intelligence, converges to viable communication links over vastly different channels including: radio frequency (RF), powerline communications (PLC), and acoustic channels.
[{'version': 'v1', 'created': 'Thu, 29 Aug 2019 13:38:07 GMT'}]
2019-08-30
[array(['Anderson', 'Adam', ''], dtype=object) array(['Young', 'Steven R.', ''], dtype=object) array(['Reed', 'F. Kyle', ''], dtype=object) array(['Vann', 'Jason M.', ''], dtype=object)]
3,905
astro-ph/0109121
Daniel Harbeck
D. Harbeck, E. K. Grebel, J. Holtzman, P. Guhathakurta, W. Brandner, D. Geisler, A. Sarajedini, A. Dolphin, D. Hurley-Keller, M. Mateo
Population Gradients in Local Group Dwarf Spheroidals
accepted for publication in AJ; 25 pages; 11 images in jpeg and png format
Astron.J.122:3092,2001
10.1086/324232
null
astro-ph
null
We present a systematic and homogeneous analysis of population gradients for the Local Group dwarf spheroidals (dSphs) Carina, Sculptor, Sextans, Tucana, Andromeda I-III, V, and VI. For all of the Milky Way companions studied here we find significant population gradients. The same is true for the remote dSph Tucana located at the outskirts of the LG. Among the M 31 dSph companions only Andromeda I and VI show obvious gradients. In all cases where a HB morphology gradient is visible, the red HB stars are more centrally concentrated. The occurence of a HB morphological gradient shows a correlation with a morphology gradient in the red giant branch. It seems likely that metallicity is the driver of the gradients in Sextans, Sculptor, Tucana, and Andromeda VI, while age is an important factor in Carina. We find no evidence that the vicinity of a nearby massive spiral galaxy influences the formation of the population gradients.
[{'version': 'v1', 'created': 'Fri, 7 Sep 2001 16:29:46 GMT'}]
2011-05-05
[array(['Harbeck', 'D.', ''], dtype=object) array(['Grebel', 'E. K.', ''], dtype=object) array(['Holtzman', 'J.', ''], dtype=object) array(['Guhathakurta', 'P.', ''], dtype=object) array(['Brandner', 'W.', ''], dtype=object) array(['Geisler', 'D.', ''], dtype=object) array(['Sarajedini', 'A.', ''], dtype=object) array(['Dolphin', 'A.', ''], dtype=object) array(['Hurley-Keller', 'D.', ''], dtype=object) array(['Mateo', 'M.', ''], dtype=object)]
3,906
1209.4022
Christopher Griffin
Ryan Tatko and Christopher Griffin
Game Theoretic Formation of a Centrality Based Network
Submitted to 2012 ASE Social Informatics Conference
null
null
null
cs.GT cs.SI physics.soc-ph
http://creativecommons.org/licenses/publicdomain/
We model the formation of networks as a game where players aspire to maximize their own centrality by increasing the number of other players to which they are path-wise connected, while simultaneously incurring a cost for each added adjacent edge. We simulate the interactions between players using an algorithm that factors in rational strategic behavior based on a common objective function. The resulting networks exhibit pairwise stability, from which we derive necessary stable conditions for specific graph topologies. We then expand the model to simulate non-trivial games with large numbers of players. We show that using conditions necessary for the stability of star topologies we can induce the formation of hub players that positively impact the total welfare of the network.
[{'version': 'v1', 'created': 'Tue, 18 Sep 2012 16:38:06 GMT'}]
2012-09-19
[array(['Tatko', 'Ryan', ''], dtype=object) array(['Griffin', 'Christopher', ''], dtype=object)]
3,907
1607.07224
Sylvain Ribault
Marco Picco, Sylvain Ribault and Raoul Santachiara
A conformal bootstrap approach to critical percolation in two dimensions
16 pages, Python code available at https://github.com/ribault/bootstrap-2d-Python, v2: some clarifications and minor improvements
SciPost Phys. 1, 009 (2016)
10.21468/SciPostPhys.1.1.009
null
hep-th cond-mat.stat-mech math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study four-point functions of critical percolation in two dimensions, and more generally of the Potts model. We propose an exact ansatz for the spectrum: an infinite, discrete and non-diagonal combination of representations of the Virasoro algebra. Based on this ansatz, we compute four-point functions using a numerical conformal bootstrap approach. The results agree with Monte-Carlo computations of connectivities of random clusters.
[{'version': 'v1', 'created': 'Mon, 25 Jul 2016 12:00:02 GMT'} {'version': 'v2', 'created': 'Mon, 17 Oct 2016 20:57:35 GMT'}]
2018-04-20
[array(['Picco', 'Marco', ''], dtype=object) array(['Ribault', 'Sylvain', ''], dtype=object) array(['Santachiara', 'Raoul', ''], dtype=object)]
3,908
2002.01662
Kyohei Kawaguchi
Kyohei Kawaguchi, Masaru Shibata, Masaomi Tanaka
Constraint on the ejecta mass for a black hole-neutron star merger event candidate S190814bv
16 pages, 15 figures
The Astrophysical Journal, Volume 893, Issue 2, id.153 (2020)
10.3847/1538-4357/ab8309
null
astro-ph.HE gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We derive the upper limit to the ejecta mass of S190814bv, a black hole-neutron star merger candidate, through the radiative transfer simulations for kilonovae with the realistic ejecta density profile as well as the detailed opacity and heating rate models. The limits to the ejecta mass strongly depend on the viewing angle. For the face-on observations ($\le45^\circ$), the total ejecta mass should be smaller than $0.1\,M_\odot$ for the average distance of S190814bv ($D=267$ Mpc), while larger mass is allowed for the edge-on observations. We also derive the conservative upper limits of the dynamical ejecta mass to be $0.02\,M_\odot$, $0.03\,M_\odot$, and $0.05\,M_\odot$ for the viewing angle $\le 20^\circ$, $\le 50^\circ$, and for $\le 90^\circ$, respectively. We show that the {\it iz}-band observation deeper than $22$ mag within 2 d after the GW trigger is crucial to detect the kilonova with the total ejecta mass of $0.06\,M_\odot$ at the distance of $D=300$ Mpc. We also show that a strong constraint on the NS mass-radius relation can be obtained if the future observations put the upper limit of $0.03\,M_\odot$ to the dynamical ejecta mass for a BH-NS event with the chirp mass smaller than $\lesssim 3\,M_\odot$ and effective spin larger than $\gtrsim 0.5$.
[{'version': 'v1', 'created': 'Wed, 5 Feb 2020 06:55:52 GMT'} {'version': 'v2', 'created': 'Sat, 6 Jun 2020 05:12:49 GMT'}]
2020-06-09
[array(['Kawaguchi', 'Kyohei', ''], dtype=object) array(['Shibata', 'Masaru', ''], dtype=object) array(['Tanaka', 'Masaomi', ''], dtype=object)]
3,909
hep-ph/0507006
Piotr Niezurawski
P. Niezurawski, A. F. Zarnecki, M. Krawczyk
Extended analysis of the MSSM Higgs boson production at the Photon Collider
Presented at the International Linear Collider Workshop LCWS05, Stanford, USA
null
null
null
hep-ph
null
New analysis of the heavy, neutral MSSM Higgs bosons H and A production at the Photon Collider is presented for M_A = 200, 250, 300 and 350 GeV in the parameter range corresponding to the so called "LHC wedge" and beyond. The expected precision of the cross section measurement for the process gamma+gamma->A,H->b+bbar and the "discovery reach" of the Photon Collider are compared for different MSSM scenarios. The analysis takes into account all relevant theoretical and experimental issues which could affect the measurement. For MSSM Higgs bosons A and H, for M_A = 200-350 GeV and tan(beta)=7, the statistical precision of the cross-section determination is estimated to be 8-34%, after one year of Photon Collider running, for four considered MSSM parameters sets. As heavy neutral Higgs bosons in this scenario may not be discovered at LHC or at the first stage of the e+e- collider, an opportunity of being a discovery machine is also studied for the Photon Collider.
[{'version': 'v1', 'created': 'Fri, 1 Jul 2005 01:34:11 GMT'}]
2007-05-23
[array(['Niezurawski', 'P.', ''], dtype=object) array(['Zarnecki', 'A. F.', ''], dtype=object) array(['Krawczyk', 'M.', ''], dtype=object)]
3,910
1807.03360
Dmitry Lande
D.V. Lande and C.V. Prishchepa
The automatic detection of the information operations event basis
7 pages, 6 figures
null
null
null
cs.CY cs.SI
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The methodology of automatic detection of the event basis of information operations, reflected in thematic information flows, is described. The presented methodology is based on the technologies for identifying information operations, the formation of the terminological basis of the subject area, the application of cluster analysis with cluster centroids, determined by analyzing the terminology of the information flow. The clusters formed in this way reflect the main events occurring during the information operations and reveal the technique for their implementation.
[{'version': 'v1', 'created': 'Fri, 22 Jun 2018 16:52:06 GMT'}]
2018-07-11
[array(['Lande', 'D. V.', ''], dtype=object) array(['Prishchepa', 'C. V.', ''], dtype=object)]
3,911
2201.01016
Hao Zhu
Yunze Xiao, Hao Zhu, Haotian Yang, Zhengyu Diao, Xiangju Lu, Xun Cao
Detailed Facial Geometry Recovery from Multi-View Images by Learning an Implicit Function
AAAI 2022 Oral, updated to camera ready version
null
null
null
cs.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Recovering detailed facial geometry from a set of calibrated multi-view images is valuable for its wide range of applications. Traditional multi-view stereo (MVS) methods adopt an optimization-based scheme to regularize the matching cost. Recently, learning-based methods integrate all these into an end-to-end neural network and show superiority of efficiency. In this paper, we propose a novel architecture to recover extremely detailed 3D faces within dozens of seconds. Unlike previous learning-based methods that regularize the cost volume via 3D CNN, we propose to learn an implicit function for regressing the matching cost. By fitting a 3D morphable model from multi-view images, the features of multiple images are extracted and aggregated in the mesh-attached UV space, which makes the implicit function more effective in recovering detailed facial shape. Our method outperforms SOTA learning-based MVS in accuracy by a large margin on the FaceScape dataset. The code and data are released in https://github.com/zhuhao-nju/mvfr.
[{'version': 'v1', 'created': 'Tue, 4 Jan 2022 07:24:58 GMT'} {'version': 'v2', 'created': 'Thu, 5 May 2022 05:34:55 GMT'}]
2022-05-06
[array(['Xiao', 'Yunze', ''], dtype=object) array(['Zhu', 'Hao', ''], dtype=object) array(['Yang', 'Haotian', ''], dtype=object) array(['Diao', 'Zhengyu', ''], dtype=object) array(['Lu', 'Xiangju', ''], dtype=object) array(['Cao', 'Xun', ''], dtype=object)]
3,912
1101.4751
Tan Lei
Lei Tan, Yu Qing Zhang, Wu Ming Liu
Quantum phase transitions for two coupled sites with dipole-coupled effective Jaynes-Cummings model
7 pages, 11 figures
null
null
null
quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The nature of the ground states for a system composed of two coupled cavities with each containing a pair of dipole-coupled two-level atoms are studied over a wide range of detunings and dipole coupling strengths. The cases for three limits of exact resonance, large positive and negative detunings are discussed, and four types of the ground states are revealed. Then the phase diagrams of the ground state are plotted by choosing three different "order parameters". We find that the phase space, determined by the combinative action of detuning and the dipole coupling strength, is divided into four regions. This is different from the general Bose-Hubbard model and more richer physics are presented in the two-site coupled cavities system. That is, the insulator region may be polaritonic or atomic and the superfluid region may be polaritonic or photonic in nature.
[{'version': 'v1', 'created': 'Tue, 25 Jan 2011 09:18:07 GMT'} {'version': 'v2', 'created': 'Mon, 9 May 2011 07:47:27 GMT'}]
2015-03-18
[array(['Tan', 'Lei', ''], dtype=object) array(['Zhang', 'Yu Qing', ''], dtype=object) array(['Liu', 'Wu Ming', ''], dtype=object)]
3,913
0805.3656
Astrid Wachter
A. Wachter, J. M. Winters, K.-P. Schr\"oder, E. Sedlmayr
Dust-driven Winds and Mass Loss of C-rich AGB Stars with subsolar Metallicities
8 pages, 4 figures. Accepted for publication in A&A
null
10.1051/0004-6361:200809893
null
astro-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the mass loss of highly evolved, low- and intermediate mass stars and stellar samples with subsolar metallicity. We give a qualitative as well as quantitative description which can be applied to LMC/SMC-type stellar populations. For that purpose we apply the same approach as we did for solar metallicity stars and calculate hydrodynamical wind models including dust formation with LMC and SMC abundances under consideration of an adapted model assumption. In particular, we improved the treatment of the radiative transfer problem in order to accommodate larger non-local contributions occurring with smaller opacities. For each wind model we determine an averaged mass-loss rate. The resulting, approximate mass-loss formulae are then applied to well-tested and calibrated stellar evolution calculations in order to quantify the stellar mass loss. The dynamical models for LMC and SMC metallicity result in mass-loss rates of the same order of magnitude as the solar metallicity models which is in this basic approach in agreement with observations. The hydrodynamical properties like e.g. the outflow velocity differ (for fixed C/O abundance ratio) noticeably, though. While critical luminosities of LMC and solar metallicity models fairly coincide, the SMC models need higher luminosities to develop dust-driven winds.
[{'version': 'v1', 'created': 'Fri, 23 May 2008 15:23:41 GMT'}]
2009-11-13
[array(['Wachter', 'A.', ''], dtype=object) array(['Winters', 'J. M.', ''], dtype=object) array(['Schröder', 'K. -P.', ''], dtype=object) array(['Sedlmayr', 'E.', ''], dtype=object)]
3,914
2207.13298
Peihao Wang
Mukund Varma T, Peihao Wang, Xuxi Chen, Tianlong Chen, Subhashini Venugopalan, Zhangyang Wang
Is Attention All That NeRF Needs?
International Conference on Learning Representations (ICLR), 2023
null
null
null
cs.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We present Generalizable NeRF Transformer (GNT), a transformer-based architecture that reconstructs Neural Radiance Fields (NeRFs) and learns to renders novel views on the fly from source views. While prior works on NeRFs optimize a scene representation by inverting a handcrafted rendering equation, GNT achieves neural representation and rendering that generalizes across scenes using transformers at two stages. (1) The view transformer leverages multi-view geometry as an inductive bias for attention-based scene representation, and predicts coordinate-aligned features by aggregating information from epipolar lines on the neighboring views. (2) The ray transformer renders novel views using attention to decode the features from the view transformer along the sampled points during ray marching. Our experiments demonstrate that when optimized on a single scene, GNT can successfully reconstruct NeRF without an explicit rendering formula due to the learned ray renderer. When trained on multiple scenes, GNT consistently achieves state-of-the-art performance when transferring to unseen scenes and outperform all other methods by ~10% on average. Our analysis of the learned attention maps to infer depth and occlusion indicate that attention enables learning a physically-grounded rendering. Our results show the promise of transformers as a universal modeling tool for graphics. Please refer to our project page for video results: https://vita-group.github.io/GNT/.
[{'version': 'v1', 'created': 'Wed, 27 Jul 2022 05:09:54 GMT'} {'version': 'v2', 'created': 'Tue, 18 Oct 2022 01:14:37 GMT'} {'version': 'v3', 'created': 'Thu, 2 Mar 2023 04:54:00 GMT'}]
2023-03-03
[array(['T', 'Mukund Varma', ''], dtype=object) array(['Wang', 'Peihao', ''], dtype=object) array(['Chen', 'Xuxi', ''], dtype=object) array(['Chen', 'Tianlong', ''], dtype=object) array(['Venugopalan', 'Subhashini', ''], dtype=object) array(['Wang', 'Zhangyang', ''], dtype=object)]
3,915
1810.11869
Martin Mourigal
X. Bai, J. A. M. Paddison, E. Kapit, S. M. Koohpayeh, J.-J. Wen, S. E. Dutton, A. T. Savici, A. I. Kolesnikov, G. E. Granroth, C. L. Broholm, J. T. Chalker, and M. Mourigal
Magnetic excitations of the classical spin liquid MgCr2O4
6 pages, 3 figures; supplementary material: 12 pages with figures
Phys. Rev. Lett. 122, 097201 (2019)
10.1103/PhysRevLett.122.097201
null
cond-mat.str-el
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We report a comprehensive inelastic neutron-scattering study of the frustrated pyrochlore antiferromagnet MgCr2O4 in its cooperative paramagnetic regime. Theoretical modeling yields a microscopic Heisenberg model with exchange interactions up to third-nearest neighbors, which quantitatively explains all the details of the dynamic magnetic response. Our work demonstrates that the magnetic excitations in paramagnetic MgCr2O4 are faithfully represented in the entire Brillouin zone by a theory of magnons propagating in a highly-correlated paramagnetic background. Our results also suggest that MgCr2O4 is proximate to a spiral spin-liquid phase distinct from the Coulomb phase, which has implications for the magneto-structural phase transition in MgCr2O4 .
[{'version': 'v1', 'created': 'Sun, 28 Oct 2018 19:42:42 GMT'}]
2019-03-11
[array(['Bai', 'X.', ''], dtype=object) array(['Paddison', 'J. A. M.', ''], dtype=object) array(['Kapit', 'E.', ''], dtype=object) array(['Koohpayeh', 'S. M.', ''], dtype=object) array(['Wen', 'J. -J.', ''], dtype=object) array(['Dutton', 'S. E.', ''], dtype=object) array(['Savici', 'A. T.', ''], dtype=object) array(['Kolesnikov', 'A. I.', ''], dtype=object) array(['Granroth', 'G. E.', ''], dtype=object) array(['Broholm', 'C. L.', ''], dtype=object) array(['Chalker', 'J. T.', ''], dtype=object) array(['Mourigal', 'M.', ''], dtype=object)]
3,916
1901.01058
Moshe Schwartz
Han Cai, Johan Chrisnata, Tuvi Etzion, Moshe Schwartz, Antonia Wachter-Zeh
Network-Coding Solutions for Minimal Combination Networks and Their Sub-networks
null
null
null
null
cs.IT math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Minimal multicast networks are fascinating and efficient combinatorial objects, where the removal of a single link makes it impossible for all receivers to obtain all messages. We study the structure of such networks, and prove some constraints on their possible solutions. We then focus on the combination network, which is one of the simplest and most insightful network in network-coding theory. Of particular interest are minimal combination networks. We study the gap in alphabet size between vector-linear and scalar-linear network-coding solutions for such minimal combination networks and some of their sub-networks. For minimal multicast networks with two source messages we find the maximum possible gap. We define and study sub-networks of the combination network, which we call Kneser networks, and prove that they attain the upper bound on the gap with equality. We also prove that the study of this gap may be limited to the study of sub-networks of minimal combination networks, by using graph homomorphisms connected with the $q$-analog of Kneser graphs. Additionally, we prove a gap for minimal multicast networks with three or more source messages by studying Kneser networks. Finally, an upper bound on the gap for full minimal combination networks shows nearly no gap, or none in some cases. This is obtained using an MDS-like bound for subspaces over a finite field.
[{'version': 'v1', 'created': 'Fri, 4 Jan 2019 11:14:48 GMT'} {'version': 'v2', 'created': 'Fri, 13 Sep 2019 05:30:43 GMT'}]
2019-09-16
[array(['Cai', 'Han', ''], dtype=object) array(['Chrisnata', 'Johan', ''], dtype=object) array(['Etzion', 'Tuvi', ''], dtype=object) array(['Schwartz', 'Moshe', ''], dtype=object) array(['Wachter-Zeh', 'Antonia', ''], dtype=object)]
3,917
1205.4199
Eugene Frumker
E. Frumker, C. T. Hebeisen, N. Kajumba, J. B. Bertrand, H. J. Worner, M. Spanner, D. M. Villeneuve, A. Naumov, and P.B. Corkum
Oriented rotational wave-packet dynamics studies via high harmonic generation
null
null
10.1103/PhysRevLett.109.113901
null
physics.atom-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We produce oriented rotational wave packets in CO and measure their characteristics via high harmonic generation. The wavepacket is created using an intense, femtosecond laser pulse and its second harmonic. A delayed 800 nm pulse probes the wave packet, generating even-order high harmonics that arise from the broken symmetry induced by the orientation dynamics. The even-order harmonic radiation that we measure appears on a zero background, enabling us to accurately follow the temporal evolution of the wave packet. Our measurements reveal that, for the conditions optimum for harmonic generation, the orientation is produced by preferential ionization which depletes the sample of molecules of one orientation.
[{'version': 'v1', 'created': 'Fri, 18 May 2012 17:02:16 GMT'}]
2015-06-05
[array(['Frumker', 'E.', ''], dtype=object) array(['Hebeisen', 'C. T.', ''], dtype=object) array(['Kajumba', 'N.', ''], dtype=object) array(['Bertrand', 'J. B.', ''], dtype=object) array(['Worner', 'H. J.', ''], dtype=object) array(['Spanner', 'M.', ''], dtype=object) array(['Villeneuve', 'D. M.', ''], dtype=object) array(['Naumov', 'A.', ''], dtype=object) array(['Corkum', 'P. B.', ''], dtype=object)]
3,918
1702.06718
Marcos Tadeu Oliveira Pimenta
C. O. Alves, M. T. O. Pimenta
On existence and concentration of solutions to a class of quasilinear problems involving the $1-$Laplace operator
null
null
null
null
math.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this work we use variational methods to prove results on existence and concentration of solutions to a problem in $\mathbb{R}^N$ involving the $1-$Laplacian operator. A thorough analysis on the energy functional defined in the space of functions of bounded variation $BV(\mathbb{R}^N)$ is necessary, where the lack of compactness is overcome by using the Concentration of Compactness Principle of Lions.
[{'version': 'v1', 'created': 'Wed, 22 Feb 2017 09:23:46 GMT'}]
2017-02-23
[array(['Alves', 'C. O.', ''], dtype=object) array(['Pimenta', 'M. T. O.', ''], dtype=object)]
3,919
1106.5211
Takeshi Araki
Takeshi Araki
Getting at large theta_13 with almost maximal theta_23 from tri-bimaximal mixing
v1:7 pages, 1 figure; v2:added references and short comments; v3:typos corrected, final version
Phys.Rev.D84:037301,2011
10.1103/PhysRevD.84.037301
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We introduce a small correction term, \delta M_\nu, in the neutrino sector and examine whether a large \theta_13 and an almost maximal \theta_23 can simultaneously be obtained starting from the tri-bimaximal neutrino mixing. It is found that one can easily gain \theta_13 \simeq 10^\circ, which is favored by the recent T2K experiment, by taking account of the enhancement due to the degeneracy among three neutrino masses. We also find that (\delta M_\nu)_22=(\delta M_\nu)_33 is a key condition for \theta_23 \simeq 45^\circ.
[{'version': 'v1', 'created': 'Sun, 26 Jun 2011 11:40:54 GMT'} {'version': 'v2', 'created': 'Sat, 16 Jul 2011 08:42:01 GMT'} {'version': 'v3', 'created': 'Tue, 2 Aug 2011 08:19:45 GMT'}]
2011-08-12
[array(['Araki', 'Takeshi', ''], dtype=object)]
3,920
2204.13892
Ziming Chen
Chang Shu, Ziming Chen, Lei Chen, Kuan Ma, Minghui Wang and Haibing Ren
SideRT: A Real-time Pure Transformer Architecture for Single Image Depth Estimation
7 pages, 5 figures
null
null
null
cs.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Since context modeling is critical for estimating depth from a single image, researchers put tremendous effort into obtaining global context. Many global manipulations are designed for traditional CNN-based architectures to overcome the locality of convolutions. Attention mechanisms or transformers originally designed for capturing long-range dependencies might be a better choice, but usually complicates architectures and could lead to a decrease in inference speed. In this work, we propose a pure transformer architecture called SideRT that can attain excellent predictions in real-time. In order to capture better global context, Cross-Scale Attention (CSA) and Multi-Scale Refinement (MSR) modules are designed to work collaboratively to fuse features of different scales efficiently. CSA modules focus on fusing features of high semantic similarities, while MSR modules aim to fuse features at corresponding positions. These two modules contain a few learnable parameters without convolutions, based on which a lightweight yet effective model is built. This architecture achieves state-of-the-art performances in real-time (51.3 FPS) and becomes much faster with a reasonable performance drop on a smaller backbone Swin-T (83.1 FPS). Furthermore, its performance surpasses the previous state-of-the-art by a large margin, improving AbsRel metric 6.9% on KITTI and 9.7% on NYU. To the best of our knowledge, this is the first work to show that transformer-based networks can attain state-of-the-art performance in real-time in the single image depth estimation field. Code will be made available soon.
[{'version': 'v1', 'created': 'Fri, 29 Apr 2022 05:46:20 GMT'}]
2022-05-02
[array(['Shu', 'Chang', ''], dtype=object) array(['Chen', 'Ziming', ''], dtype=object) array(['Chen', 'Lei', ''], dtype=object) array(['Ma', 'Kuan', ''], dtype=object) array(['Wang', 'Minghui', ''], dtype=object) array(['Ren', 'Haibing', ''], dtype=object)]
3,921
1408.5614
Fulvia De Fazio
Pietro Biancofiore, Pietro Colangelo, Fulvia De Fazio, Egidio Scrimieri
Exclusive $b \to s \nu \bar \nu$ induced transitions in RS$_c$ model
RevTex, 13 pages, 12 figures
null
null
BARI-TH/2014-690
hep-ph hep-ex hep-lat
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study a set of exclusive $B$ and $B_s$ decay modes induced by the rare $b \to s \nu \bar \nu$ transition in the RS$_c$ model, an extra-dimensional extension of the standard model with warped 5D metric and extended gauge group. We emphasize the role of correlations among the observables, and their importance for detecting the predicted small deviations from the standard model expectations.
[{'version': 'v1', 'created': 'Sun, 24 Aug 2014 15:53:46 GMT'}]
2014-08-26
[array(['Biancofiore', 'Pietro', ''], dtype=object) array(['Colangelo', 'Pietro', ''], dtype=object) array(['De Fazio', 'Fulvia', ''], dtype=object) array(['Scrimieri', 'Egidio', ''], dtype=object)]
3,922
1502.06081
Radu Arsinte
Radu Arsinte
Study of a Robust Algorithm Applied in the Optimal Position Tuning for the Camera Lens in Automated Visual Inspection Systems
5 pages, 2 figures
Proceedings of Fifth International Conference on Pattern Recognition and Information Processing - PRIP'99 - May 18-20, 1999 Minsk, Belarus - pag.237-242 - ISBN 83-87362-16-6
null
null
cs.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper present the mathematical fundaments and experimental study of an algorithm used to find the optimal position for the camera lens to obtain a maximum of details. This information can be further applied to a appropriate system to automatically correct this position. The algorithm is based on the evaluation of a so called resolution function who calculates the maximum of gradient in a certain zone of the image. The paper also presents alternative forms of the function, results of measurements and set up a set of practical rules for the right application of the algorithm.
[{'version': 'v1', 'created': 'Sat, 21 Feb 2015 07:40:18 GMT'}]
2015-02-24
[array(['Arsinte', 'Radu', ''], dtype=object)]
3,923
cond-mat/0111163
Shinobu Ohya
Shinobu Ohya, Hiromasa Shimizu, Yutaka Higo, Jiaming Sun, and Masaaki Tanaka
Growth and Properties of Quaternary Alloy Magnetic Semiconductor (InGaMn)As
4 pages, 4 figures
null
null
null
cond-mat.mtrl-sci
null
We have studied growth and properties of quaternary alloy magnetic semiconductor (InGaMn)As grown both on GaAs substrates and on InP substrates by low-temperature molecular-beam epitaxy (LT-MBE). (InGaMn)As thin films were ferromagnetic below ~30 K, exhibiting strong magneto-optical effect. The lattice constant of [(InyGa1-y)1-xMnx]As, whose Mn concentration x is below 4%, is slightly smaller than that of InyGa1-yAs with the same In/Ga content ratio. We have also obtained very smooth surface morphology of nearly lattice matched (InGaMn)As thin films grown on InP substrates, which is important for application to thin-film type magneto-optical devices integrated with III-V opto-electronics.
[{'version': 'v1', 'created': 'Fri, 9 Nov 2001 12:10:26 GMT'}]
2007-05-23
[array(['Ohya', 'Shinobu', ''], dtype=object) array(['Shimizu', 'Hiromasa', ''], dtype=object) array(['Higo', 'Yutaka', ''], dtype=object) array(['Sun', 'Jiaming', ''], dtype=object) array(['Tanaka', 'Masaaki', ''], dtype=object)]
3,924
1404.5911
Fernando C. Lombardo
C. D. Fosco, F. C. Lombardo, and F. D. Mazzitelli
The derivative expansion approach to the interaction between close surfaces
Minor changes, version to appear in Phys. Rev. A
null
10.1103/PhysRevA.89.062120
null
quant-ph hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The derivative expansion approach to the calculation of the interaction between two surfaces, is a generalization of the proximity force approximation, a technique of widespread use in different areas of physics. The derivative expansion has so far been applied to seemingly unrelated problems in different areas; it is our principal aim here to present the approach in its full generality. To that end, we introduce an unified setting, which is independent of any particular application, provide a formal derivation of the derivative expansion in that general setting, and study some its properties. With a view on the possible application of the derivative expansion to other areas, like nuclear and colloidal physics, we also discuss the relation between the derivative expansion and some time-honoured uncontrolled approximations used in those contexts. By putting them under similar terms as the derivative expansion, we believe that the path is open to the calculation of next to leading order corrections also for those contexts. We also review some results obtained within the derivative expansion, by applying it to different concrete examples and highlighting some important points.
[{'version': 'v1', 'created': 'Wed, 23 Apr 2014 17:51:13 GMT'} {'version': 'v2', 'created': 'Wed, 18 Jun 2014 14:46:31 GMT'}]
2015-06-19
[array(['Fosco', 'C. D.', ''], dtype=object) array(['Lombardo', 'F. C.', ''], dtype=object) array(['Mazzitelli', 'F. D.', ''], dtype=object)]
3,925
2205.02235
Alexis Plascencia
Pavel Fileviez Perez, Elliot Golias, Alexis D. Plascencia
Two-Higgs-Doublet Model and Quark-Lepton Unification
16 pages, 10 figures
JHEP 08 (2022) 293
10.1007/JHEP08(2022)293
null
hep-ph hep-ex
http://creativecommons.org/licenses/by/4.0/
We study the Two-Higgs-Doublet Model predicted in the minimal theory for quark-lepton unification that can describe physics at the low scale. We discuss the relations among the different decay widths of the new Higgs bosons and study their phenomenology at the Large Hadron Collider. As a result of matter unification, this theory predicts a correlation between the decay widths of the heavy Higgs bosons into tau leptons and bottom quarks. We point out how to probe this theory using these relations and discuss the relevant flavor constraints.
[{'version': 'v1', 'created': 'Wed, 4 May 2022 18:00:00 GMT'}]
2022-09-01
[array(['Perez', 'Pavel Fileviez', ''], dtype=object) array(['Golias', 'Elliot', ''], dtype=object) array(['Plascencia', 'Alexis D.', ''], dtype=object)]
3,926
physics/0212049
Hanns L. Harney
A.Y. Abul-Magd, H.L. Harney, M.H. Simbel, and H.A. Weidenmueller
Statistical Analysis of Composite Spectra
26 pages, 3 figures; v3: changed conclusions, appendix added
Annals Phys. 321 (2006) 560-580
10.1016/j.aop.2005.04.005
null
physics.data-an nucl-th
null
We consider nearest neighbor spacing distributions of composite ensembles of levels. These are obtained by combining independently unfolded sequences of levels containing only few levels each. Two problems arise in the spectral analysis of such data. One problem lies in fitting the nearest neighbor spacing distribution to the histogram of level spacings obtained from the data. We show that the method of Bayesian inference is superior to this procedure. The second problem occurs when one unfolds such short sequences. We show that the unfolding procedure generically leads to an overestimate of the chaoticity parameter. This trend is absent in the presence of long-range level correlations. Thus, composite ensembles of levels from a system with long-range spectral stiffness yield reliable information about the chaotic behavior of the system.
[{'version': 'v1', 'created': 'Thu, 12 Dec 2002 09:08:52 GMT'} {'version': 'v2', 'created': 'Thu, 12 Feb 2004 08:41:06 GMT'} {'version': 'v3', 'created': 'Wed, 24 Nov 2004 21:14:32 GMT'}]
2009-11-07
[array(['Abul-Magd', 'A. Y.', ''], dtype=object) array(['Harney', 'H. L.', ''], dtype=object) array(['Simbel', 'M. H.', ''], dtype=object) array(['Weidenmueller', 'H. A.', ''], dtype=object)]
3,927
1810.13111
Peng Kang
Peng Kang, Yixuan Xie, Lei Yang, Chen Zheng, Jinhong Yuan, and Yuejun Wei
Enhanced Quasi-Maximum Likelihood Decoding of Short LDPC Codes based on Saturation
null
null
null
null
cs.IT math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we propose an enhanced quasi-maximum likelihood (EQML) decoder for LDPC codes with short block lengths. After the failure of the conventional belief propagation (BP) decoding, the proposed EQML decoder selects unreliable variable nodes (VNs) and saturates their associated channel output values to generate a list of decoder input sequences. Each decoder input sequence in the list is then decoded by the conventional BP decoder to obtain the most likely codeword. To improve the accuracy of selecting unreliable VNs, we propose an edge-wise selection method based on the sign fluctuation of VNs' extrinsic messages. A partial pruning stopping (PPS) rule is also presented to reduce the decoding latency. Simulation results show that the proposed EQML decoder outperforms the conventional BP decoder and the augmented BP decoder for short LDPC codes. It even approaches the performance of ML decoding within 0.3 dB in terms of frame error rate. In addition, the proposed PPS rule achieves a lower decoding latency compared to the list decoding stopping rule.
[{'version': 'v1', 'created': 'Wed, 31 Oct 2018 05:17:51 GMT'} {'version': 'v2', 'created': 'Wed, 30 Jan 2019 11:32:02 GMT'}]
2019-01-31
[array(['Kang', 'Peng', ''], dtype=object) array(['Xie', 'Yixuan', ''], dtype=object) array(['Yang', 'Lei', ''], dtype=object) array(['Zheng', 'Chen', ''], dtype=object) array(['Yuan', 'Jinhong', ''], dtype=object) array(['Wei', 'Yuejun', ''], dtype=object)]
3,928
2203.07027
Jianzhang Zheng
Jianzhang Zheng, Fan Yang, Hao Shen, Xuan Tang, Mingsong Chen, Liang Song, Xian Wei
Learning from Attacks: Attacking Variational Autoencoder for Improving Image Classification
null
null
null
null
cs.LG cs.CV eess.IV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Adversarial attacks are often considered as threats to the robustness of Deep Neural Networks (DNNs). Various defending techniques have been developed to mitigate the potential negative impact of adversarial attacks against task predictions. This work analyzes adversarial attacks from a different perspective. Namely, adversarial examples contain implicit information that is useful to the predictions i.e., image classification, and treat the adversarial attacks against DNNs for data self-expression as extracted abstract representations that are capable of facilitating specific learning tasks. We propose an algorithmic framework that leverages the advantages of the DNNs for data self-expression and task-specific predictions, to improve image classification. The framework jointly learns a DNN for attacking Variational Autoencoder (VAE) networks and a DNN for classification, coined as Attacking VAE for Improve Classification (AVIC). The experiment results show that AVIC can achieve higher accuracy on standard datasets compared to the training with clean examples and the traditional adversarial training.
[{'version': 'v1', 'created': 'Fri, 11 Mar 2022 08:48:26 GMT'}]
2022-04-12
[array(['Zheng', 'Jianzhang', ''], dtype=object) array(['Yang', 'Fan', ''], dtype=object) array(['Shen', 'Hao', ''], dtype=object) array(['Tang', 'Xuan', ''], dtype=object) array(['Chen', 'Mingsong', ''], dtype=object) array(['Song', 'Liang', ''], dtype=object) array(['Wei', 'Xian', ''], dtype=object)]
3,929
1409.0998
Matthias W\"ahlisch
Keigo Kawahara, Yutaka Matsubara, Hiroaki Takada
A Simulation Environment and preliminary evaluation for Automotive CAN-Ethernet AVB Networks
Published in: A. F\"orster, C. Sommer, T. Steinbach, M. W\"ahlisch (Eds.), Proc. of 1st OMNeT++ Community Summit, Hamburg, Germany, September 2, 2014, arXiv:1409.0093, 2014
null
null
OMNET/2014/02
cs.NI
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Ethernet is being considered as the backbone network protocol for next-generation automotive control networks. In such networks, Controller Area Network (CAN) messages related to automotive control can be sent from a CAN network to other sub-networks via the backbone Ethernet bus and, if the CAN messages have real-time constraints, these have to be guaranteed. This paper presents a simulation environment for CAN--Ethernet Audio Video Bridging (AVB) mixed networks based on OMNeT++. We use Ethernet AVB, which can guarantee network bandwidth, to improve the real-time property of CAN messages through the backbone Ethernet bus. To simulate the networks, we also developed a CAN--Ethernet AVB gateway (GW) model. To verify the efficacy of our model, we measured the latency of CAN messages sent from a CAN bus to an Ethernet AVB node via the backbone Ethernet AVB bus in both bandwidth-guaranteed and best-effort queue scenarios. The results indicate that the latency of Ethernet AVB frames containing CAN messages is minimized and limited by the bandwidth-guaranteed mechanism of Ethernet AVB.
[{'version': 'v1', 'created': 'Wed, 3 Sep 2014 09:01:50 GMT'}]
2014-09-04
[array(['Kawahara', 'Keigo', ''], dtype=object) array(['Matsubara', 'Yutaka', ''], dtype=object) array(['Takada', 'Hiroaki', ''], dtype=object)]
3,930
1606.08094
Michael Margaliot
Yoram Zarai and Michael Margaliot and Tamir Tuller
Optimal Down Regulation of mRNA Translation
null
null
null
null
q-bio.GN
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Down regulation of mRNA translation is an important problem in various bio-medical domains ranging from developing effective medicines for tumors and for viral diseases to developing attenuated virus strains that can be used for vaccination. Here, we study the problem of down regulation of mRNA translation using a mathematical model called the ribosome flow model (RFM). In the RFM, the mRNA molecule is modeled as a chain of $n$ sites. The flow of ribosomes between consecutive sites is regulated by $n+1$ transition rates. Given a set of feasible transition rates, that models the outcome of all possible mutations, we consider the problem of maximally down regulating the translation rate by altering the rates within this set of feasible rates. Under certain conditions on the feasible set, we show that an optimal solution can be determined efficiently. We also rigorously analyze two special cases of the down regulation optimization problem. Our results suggest that one must focus on the position along the mRNA molecule where the transition rate has the strongest effect on the protein production rate. However, this rate is not necessarily the slowest transition rate along the mRNA molecule. We discuss some of the biological implications of these results.
[{'version': 'v1', 'created': 'Sun, 26 Jun 2016 22:23:08 GMT'} {'version': 'v2', 'created': 'Tue, 28 Jun 2016 06:26:10 GMT'}]
2016-06-29
[array(['Zarai', 'Yoram', ''], dtype=object) array(['Margaliot', 'Michael', ''], dtype=object) array(['Tuller', 'Tamir', ''], dtype=object)]
3,931
2211.13901
Yu Deng
Yu Deng, Baoyuan Wang, Heung-Yeung Shum
Learning Detailed Radiance Manifolds for High-Fidelity and 3D-Consistent Portrait Synthesis from Monocular Image
CVPR 2023 camera-ready version. Project page: https://yudeng.github.io/GRAMInverter/
null
null
null
cs.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A key challenge for novel view synthesis of monocular portrait images is 3D consistency under continuous pose variations. Most existing methods rely on 2D generative models which often leads to obvious 3D inconsistency artifacts. We present a 3D-consistent novel view synthesis approach for monocular portrait images based on a recent proposed 3D-aware GAN, namely Generative Radiance Manifolds (GRAM), which has shown strong 3D consistency at multiview image generation of virtual subjects via the radiance manifolds representation. However, simply learning an encoder to map a real image into the latent space of GRAM can only reconstruct coarse radiance manifolds without faithful fine details, while improving the reconstruction fidelity via instance-specific optimization is time-consuming. We introduce a novel detail manifolds reconstructor to learn 3D-consistent fine details on the radiance manifolds from monocular images, and combine them with the coarse radiance manifolds for high-fidelity reconstruction. The 3D priors derived from the coarse radiance manifolds are used to regulate the learned details to ensure reasonable synthesized results at novel views. Trained on in-the-wild 2D images, our method achieves high-fidelity and 3D-consistent portrait synthesis largely outperforming the prior art.
[{'version': 'v1', 'created': 'Fri, 25 Nov 2022 05:20:04 GMT'} {'version': 'v2', 'created': 'Mon, 20 Mar 2023 09:07:21 GMT'}]
2023-03-21
[array(['Deng', 'Yu', ''], dtype=object) array(['Wang', 'Baoyuan', ''], dtype=object) array(['Shum', 'Heung-Yeung', ''], dtype=object)]
3,932
2010.00369
Sergei Ivanov Olegovich
Sergei O. Ivanov, Fedor Pavutnitskiy, Vladislav Romanovskii, Anatolii Zaikovskii
On homology of Lie algebras over commutative rings
null
Journal of Algebra, Volume 586, 2021, Pages 99-139, ISSN 0021-8693
10.1016/j.jalgebra.2021.06.019
null
math.KT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study five different types of the homology of a Lie algebra over a commutative ring which are naturally isomorphic over fields. We show that they are not isomorphic over commutative rings, even over $\mathbb Z,$ and study connections between them. In particular, we show that they are naturally isomorphic in the case of a Lie algebra which is flat as a module. As an auxiliary result we prove that the Koszul complex of a module $M$ over a principal ideal domain that connects the exterior and the symmetric powers $0\to \Lambda^n M\to M \otimes \Lambda^{n-1} M \to \dots \to S^{n-1}M \otimes M \to S^nM\to 0 $ is purely acyclic.
[{'version': 'v1', 'created': 'Thu, 1 Oct 2020 13:01:43 GMT'} {'version': 'v2', 'created': 'Sun, 11 Oct 2020 07:42:05 GMT'} {'version': 'v3', 'created': 'Thu, 29 Oct 2020 12:33:27 GMT'} {'version': 'v4', 'created': 'Thu, 17 Dec 2020 12:11:43 GMT'} {'version': 'v5', 'created': 'Wed, 16 Jun 2021 15:18:52 GMT'} {'version': 'v6', 'created': 'Tue, 29 Jun 2021 11:08:42 GMT'}]
2022-01-19
[array(['Ivanov', 'Sergei O.', ''], dtype=object) array(['Pavutnitskiy', 'Fedor', ''], dtype=object) array(['Romanovskii', 'Vladislav', ''], dtype=object) array(['Zaikovskii', 'Anatolii', ''], dtype=object)]
3,933
astro-ph/0607338
Kristen Menou
James Y-K. Cho (QM Univ. London), Kristen Menou (Columbia), Brad Hansen (UCLA), Sara Seager (Carnegie/DTM)
Atmospheric Circulation of Close-In Extrasolar Giant Planets: I. Global, Barotropic, Adiabatic Simulations
Accepted for publication in ApJ. Section added on key assumptions. See previous version for the figures (postscript link)
null
null
null
astro-ph
null
We present results from a set of over 300 pseudospectral simulations of atmospheric circulation on extrasolar giant planets with circular orbits. The simulations are of high enough resolution (up to 341 total and sectoral modes) to resolve small-scale eddies and waves, required for reasonable physical accuracy. In this work, we focus on the global circulation pattern that emerges in a shallow, ``equivalent-barotropic'', turbulent atmosphere on both tidally synchronized and unsynchronized planets. A full exploration of the large physical and numerical parameter-space is performed to identify robust features of the circulation. For some validation, the model is first applied to Solar System giant planets. For extrasolar giant planets with physical parameters similar to HD209458b--a presumably synchronized extrasolar giant planet, representative in many dynamical respects--the circulation is characterized by the following features: 1) a coherent polar vortex that revolves around the pole in each hemisphere; 2) a low number--typically two or three--of slowly-varying, broad zonal (east-west) jets that form when the maximum jet speed is comparable to, or somewhat stronger than, those observed on the planets in the Solar System; and, 3) motion-associated temperature field, whose detectability and variability depend on the strength of the net heating rate and the global root mean square wind speed in the atmosphere. In many ways, the global circulation is Earth-like, rather than Jupiter-like. However, if extrasolar giant planets rotate faster and are not close-in (therefore not synchronized), their circulations become more Jupiter-like, for Jupiter-like rotation rates.
[{'version': 'v1', 'created': 'Fri, 14 Jul 2006 16:27:37 GMT'} {'version': 'v2', 'created': 'Sun, 21 Oct 2007 19:13:31 GMT'}]
2007-10-22
[array(['Cho', 'James Y-K.', '', 'QM Univ. London'], dtype=object) array(['Menou', 'Kristen', '', 'Columbia'], dtype=object) array(['Hansen', 'Brad', '', 'UCLA'], dtype=object) array(['Seager', 'Sara', '', 'Carnegie/DTM'], dtype=object)]
3,934
1609.03431
Mats G Larson
Erik Burman, Peter Hansbo, Mats G. Larson, Rolf Stenberg
Galerkin least squares finite element method for the obstacle problem
18 pages, 5 figures
null
10.1016/j.cma.2016.09.025
null
math.NA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We construct a consistent multiplier free method for the finite element solution of the obstacle problem. The method is based on an augmented Lagrangian formulation in which we eliminate the multiplier by use of its definition in a discrete setting. We prove existence and uniqueness of discrete solutions and optimal order a priori error estimates for smooth exact solutions. Using a saturation assumption we also prove an a posteriori error estimate. Numerical examples show the performance of the method and of an adaptive algorithm for the control of the discretization error.
[{'version': 'v1', 'created': 'Mon, 12 Sep 2016 14:58:53 GMT'}]
2016-11-23
[array(['Burman', 'Erik', ''], dtype=object) array(['Hansbo', 'Peter', ''], dtype=object) array(['Larson', 'Mats G.', ''], dtype=object) array(['Stenberg', 'Rolf', ''], dtype=object)]
3,935
2010.01914
Patrick Krauss
Patrick Krauss and Achim Schilling
Towards a Cognitive Computational Neuroscience of Auditory Phantom Perceptions
null
null
null
null
q-bio.NC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In order to gain a mechanistic understanding of how tinnitus emerges in the brain, we must build biologically plausible computational models that mimic both tinnitus development and perception, and test the tentative models with brain and behavioral experiments. With a special focus on tinnitus research, we review recent work at the intersection of artificial intelligence, psychology and neuroscience, indicating a new research agenda that follows the idea that experiments will yield theoretical insight only when employed to test brain-computational models. This view challenges the popular belief, that tinnitus research is primarily data limited, and that producing large, multi-modal, and complex datasets, analyzed with advanced data analysis algorithms, will finally lead to fundamental insights into how tinnitus emerges. However, there is converging evidence that although modern technologies allow assessing neural activity in unprecedentedly rich ways in both, animals and humans, empirical testing one verbally defined hypothesis about tinnitus after another, will never lead to a mechanistic understanding. Instead, hypothesis testing needs to be complemented with the construction of computational models that generate verifiable predictions. We argue, that even though, contemporary artificial intelligence and machine learning approaches largely lack biological plausibility, the models to be constructed will have to draw on concepts from these fields, since they have already proven to do well in modeling brain function. Nevertheless, biological fidelity will have to be increased successively, leading to ever better and fine-grained models, allowing at the end for even testing possible treatment strategies in silico, before application in animal or patient studies.
[{'version': 'v1', 'created': 'Mon, 5 Oct 2020 10:55:03 GMT'}]
2020-10-06
[array(['Krauss', 'Patrick', ''], dtype=object) array(['Schilling', 'Achim', ''], dtype=object)]
3,936
1910.08473
Sisi Zhou
Sisi Zhou, Liang Jiang
An exact correspondence between the quantum Fisher information and the Bures metric
5 pages
null
null
null
quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The quantum information and the Bures metric are equivalent to each other, except at points where the rank of the density matrix changes. Here we show that by slightly modifying the definition of the Bures metric, the quantum information will be fully equivalent to the Bures metric without exception.
[{'version': 'v1', 'created': 'Fri, 18 Oct 2019 15:32:11 GMT'}]
2019-10-21
[array(['Zhou', 'Sisi', ''], dtype=object) array(['Jiang', 'Liang', ''], dtype=object)]
3,937
2102.01673
Benjamin Linowitz
Sara Lapan, Benjamin Linowitz, Jeffrey S. Meyer
Universal systole bounds for arithmetic locally symmetric spaces
null
null
null
null
math.DG math.GT math.NT
http://creativecommons.org/licenses/by/4.0/
The systole of a closed Riemannian manifold is the minimal length of a non-contractible closed loop. We give a uniform lower bound for the systole for large classes of simple arithmetic locally symmetric orbifolds. We establish new bounds for the translation length of a semisimple element x in SL_n(R) in terms of its associated Mahler measure. We use these geometric methods to prove the existence of extensions of number fields in which fixed sets of primes have certain prescribed splitting behavior.
[{'version': 'v1', 'created': 'Tue, 2 Feb 2021 18:43:59 GMT'}]
2021-02-03
[array(['Lapan', 'Sara', ''], dtype=object) array(['Linowitz', 'Benjamin', ''], dtype=object) array(['Meyer', 'Jeffrey S.', ''], dtype=object)]
3,938
1511.07731
Cemsinan Deliduman
Cemsinan Deliduman, Oguzhan Kasikci, and Baris Yapiskan
Flat Galactic Rotation Curves from Geometry in Weyl Gravity
8 pages, latex; v2: typos corrected, v3: discussion shortened, v4: new section added, v5: discussion extended, v6: published version
Astrophys.Space Sci. 365 (2020) 3, 51
10.1007/s10509-020-03764-y
null
gr-qc astro-ph.GA hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We searched for a resolution of the flat galactic rotation curve problem from geometry instead of assuming the existence of dark matter. We observed that the scale independence of the rotational velocity in the outer region of galaxies could point out to a possible existence of local scale symmetry and therefore the gravitational phenomena inside such regions should be described by the unique local scale symmetric theory, namely Weyl's theory of gravity. We solved field equations of Weyl gravity and determined the special geometry in the outer region of galaxies. In order to understand the effective description of gravitational phenomena, we compared individual terms of so called Einstein-Weyl theory and concluded that while the outer region of galaxies are described by the Weyl term, the inner region of galaxies are described by the Einstein-Hilbert term.
[{'version': 'v1', 'created': 'Tue, 24 Nov 2015 14:36:47 GMT'} {'version': 'v2', 'created': 'Sun, 6 Dec 2015 10:55:22 GMT'} {'version': 'v3', 'created': 'Wed, 30 Aug 2017 18:52:37 GMT'} {'version': 'v4', 'created': 'Sun, 30 Sep 2018 14:38:35 GMT'} {'version': 'v5', 'created': 'Thu, 17 Oct 2019 15:20:22 GMT'} {'version': 'v6', 'created': 'Sun, 5 Apr 2020 12:05:59 GMT'}]
2020-04-15
[array(['Deliduman', 'Cemsinan', ''], dtype=object) array(['Kasikci', 'Oguzhan', ''], dtype=object) array(['Yapiskan', 'Baris', ''], dtype=object)]
3,939
2212.14356
Chiara Toldo
Alejandra Castro, Francesca Mariani, Chiara Toldo
Near-Extremal Limits of de Sitter Black Holes
32 pages, 2 figures; v3: typos fixed, clarifications on branches of 2D solutions added, comments on metric backreaction in sec. 4.2 removed. Section with outlook and conclusions added
null
null
null
hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We analyze the thermodynamic response near extremality of charged black holes in four-dimensional Einstein-Maxwell theory with a positive cosmological constant. The latter exhibit three different extremal limits, dubbed cold, Nariai and ultracold configurations, with near-horizon geometries AdS$_2 \times S^2$, dS$_2 \times S^2$, Mink$_2 \times S^2$, respectively. For each of these three cases we analyze small deformations away from extremality, and contrast their response. We also construct the effective two-dimensional theory, obtained by dimensional reduction, that captures these features and we provide a more detailed analysis of the perturbations around the near-horizon geometry for each case. Our results for the ultracold case in particular show an interesting interplay between the entropy variation and charge variation, realizing a different symmetry breaking with respect to the other two near-extremal limits.
[{'version': 'v1', 'created': 'Thu, 29 Dec 2022 16:09:16 GMT'} {'version': 'v2', 'created': 'Mon, 6 Feb 2023 19:01:48 GMT'} {'version': 'v3', 'created': 'Mon, 29 May 2023 21:52:27 GMT'}]
2023-05-31
[array(['Castro', 'Alejandra', ''], dtype=object) array(['Mariani', 'Francesca', ''], dtype=object) array(['Toldo', 'Chiara', ''], dtype=object)]
3,940
1911.03764
Ruoxuan Xiong
Ruoxuan Xiong, Susan Athey, Mohsen Bayati, Guido Imbens
Optimal Experimental Design for Staggered Rollouts
null
null
null
null
econ.EM stat.ME stat.ML
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we study the design and analysis of experiments conducted on a set of units over multiple time periods where the starting time of the treatment may vary by unit. The design problem involves selecting an initial treatment time for each unit in order to most precisely estimate both the instantaneous and cumulative effects of the treatment. We first consider non-adaptive experiments, where all treatment assignment decisions are made prior to the start of the experiment. For this case, we show that the optimization problem is generally NP-hard, and we propose a near-optimal solution. Under this solution, the fraction entering treatment each period is initially low, then high, and finally low again. Next, we study an adaptive experimental design problem, where both the decision to continue the experiment and treatment assignment decisions are updated after each period's data is collected. For the adaptive case, we propose a new algorithm, the Precision-Guided Adaptive Experiment (PGAE) algorithm, that addresses the challenges at both the design stage and at the stage of estimating treatment effects, ensuring valid post-experiment inference accounting for the adaptive nature of the design. Using realistic settings, we demonstrate that our proposed solutions can reduce the opportunity cost of the experiments by over 50%, compared to static design benchmarks.
[{'version': 'v1', 'created': 'Sat, 9 Nov 2019 19:46:29 GMT'} {'version': 'v2', 'created': 'Mon, 17 Aug 2020 02:19:05 GMT'} {'version': 'v3', 'created': 'Mon, 10 Jan 2022 06:32:31 GMT'} {'version': 'v4', 'created': 'Sun, 1 Jan 2023 06:36:51 GMT'} {'version': 'v5', 'created': 'Thu, 30 Mar 2023 17:17:42 GMT'}]
2023-03-31
[array(['Xiong', 'Ruoxuan', ''], dtype=object) array(['Athey', 'Susan', ''], dtype=object) array(['Bayati', 'Mohsen', ''], dtype=object) array(['Imbens', 'Guido', ''], dtype=object)]
3,941
1709.07766
Delfim F. M. Torres
Ravi P. Agarwal, Dumitru Baleanu, Juan J. Nieto, Delfim F. M. Torres, Yong Zhou
A survey on fuzzy fractional differential and optimal control nonlocal evolution equations
This is a preprint of a paper whose final and definite form is with 'Journal of Computational and Applied Mathematics', ISSN: 0377-0427. Submitted 17-July-2017; Revised 18-Sept-2017; Accepted for publication 20-Sept-2017. arXiv admin note: text overlap with arXiv:1504.05153
J. Comput. Appl. Math. 339 (2018), 3--29
10.1016/j.cam.2017.09.039
null
math.OC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We survey some representative results on fuzzy fractional differential equations, controllability, approximate controllability, optimal control, and optimal feedback control for several different kinds of fractional evolution equations. Optimality and relaxation of multiple control problems, described by nonlinear fractional differential equations with nonlocal control conditions in Banach spaces, are considered.
[{'version': 'v1', 'created': 'Thu, 21 Sep 2017 13:39:32 GMT'}]
2018-04-20
[array(['Agarwal', 'Ravi P.', ''], dtype=object) array(['Baleanu', 'Dumitru', ''], dtype=object) array(['Nieto', 'Juan J.', ''], dtype=object) array(['Torres', 'Delfim F. M.', ''], dtype=object) array(['Zhou', 'Yong', ''], dtype=object)]
3,942
0909.4790
David F. Anderson
David F. Anderson, Arnab Ganguly, Thomas G. Kurtz
Error analysis of tau-leap simulation methods
Published in at http://dx.doi.org/10.1214/10-AAP756 the Annals of Applied Probability (http://www.imstat.org/aap/) by the Institute of Mathematical Statistics (http://www.imstat.org)
Annals of Applied Probability 2011, Vol. 21, No. 6, 2226-2262
10.1214/10-AAP756
IMS-AAP-AAP756
math.PR math.NA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We perform an error analysis for numerical approximation methods of continuous time Markov chain models commonly found in the chemistry and biochemistry literature. The motivation for the analysis is to be able to compare the accuracy of different approximation methods and, specifically, Euler tau-leaping and midpoint tau-leaping. We perform our analysis under a scaling in which the size of the time discretization is inversely proportional to some (bounded) power of the norm of the state of the system. We argue that this is a more appropriate scaling than that found in previous error analyses in which the size of the time discretization goes to zero independent of the rest of the model. Under the present scaling, we show that midpoint tau-leaping achieves a higher order of accuracy, in both a weak and a strong sense, than Euler tau-leaping; a result that is in contrast to previous analyses. We present examples that demonstrate our findings.
[{'version': 'v1', 'created': 'Fri, 25 Sep 2009 20:04:34 GMT'} {'version': 'v2', 'created': 'Thu, 8 Jul 2010 16:14:25 GMT'} {'version': 'v3', 'created': 'Tue, 14 Feb 2012 14:28:25 GMT'}]
2012-02-15
[array(['Anderson', 'David F.', ''], dtype=object) array(['Ganguly', 'Arnab', ''], dtype=object) array(['Kurtz', 'Thomas G.', ''], dtype=object)]
3,943
1912.07366
Piyush Pandita
Piyush Pandita, Nimish Awalgaonkar, Ilias Bilionis and Jitesh Panchal
Learning Arbitrary Quantities of Interest from Expensive Black-Box Functions through Bayesian Sequential Optimal Design
58 figures
null
null
null
stat.ML cs.LG stat.ME
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Estimating arbitrary quantities of interest (QoIs) that are non-linear operators of complex, expensive-to-evaluate, black-box functions is a challenging problem due to missing domain knowledge and finite budgets. Bayesian optimal design of experiments (BODE) is a family of methods that identify an optimal design of experiments (DOE) under different contexts, using only in a limited number of function evaluations. Under BODE methods, sequential design of experiments (SDOE) accomplishes this task by selecting an optimal sequence of experiments while using data-driven probabilistic surrogate models instead of the expensive black-box function. Probabilistic predictions from the surrogate model are used to define an information acquisition function (IAF) which quantifies the marginal value contributed or the expected information gained by a hypothetical experiment. The next experiment is selected by maximizing the IAF. A generally applicable IAF is the expected information gain (EIG) about a QoI as captured by the expectation of the Kullback-Leibler divergence between the predictive distribution of the QoI after doing a hypothetical experiment and the current predictive distribution about the same QoI. We model the underlying information source as a fully-Bayesian, non-stationary Gaussian process (FBNSGP), and derive an approximation of the information gain of a hypothetical experiment about an arbitrary QoI conditional on the hyper-parameters The EIG about the same QoI is estimated by sample averages to integrate over the posterior of the hyper-parameters and the potential experimental outcomes. We demonstrate the performance of our method in four numerical examples and a practical engineering problem of steel wire manufacturing. The method is compared to two classic SDOE methods: random sampling and uncertainty sampling.
[{'version': 'v1', 'created': 'Mon, 16 Dec 2019 13:55:07 GMT'}]
2019-12-17
[array(['Pandita', 'Piyush', ''], dtype=object) array(['Awalgaonkar', 'Nimish', ''], dtype=object) array(['Bilionis', 'Ilias', ''], dtype=object) array(['Panchal', 'Jitesh', ''], dtype=object)]
3,944
0804.0384
Jonas Kraus A.
Franz M. Weinert (1), Jonas A. Kraus (2), Thomas Franosch (2), Dieter Braun (1) ((1) Applied Physics and Center for NanoScience (CeNS), Department of Physics, Ludwig-Maximilians-Universit\"at M\"unchen, Germany, (2) Arnold Sommerfeld Center for Theoretical Physics (ASC) and Center for NanoScience (CeNS), Department of Physics, Ludwig-Maximilians-Universit\"at M\"unchen, Germany)
Microscale fluid flow induced by thermoviscous expansion along a traveling wave
5 pages, 3 figures, accepted by Physical Review Letters
null
10.1103/PhysRevLett.100.164501
null
cond-mat.soft
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The thermal expansion of a fluid combined with a temperature-dependent viscosity introduces nonlinearities in the Navier-Stokes equations unrelated to the convective momentum current. The couplings generate the possibility for net fluid flow at the microscale controlled by external heating. This novel thermo-mechanical effect is investigated for a thin fluid chamber by a numerical solution of the Navier-Stokes equations and analytically by a perturbation expansion. A demonstration experiment confirms the basic mechanism and quantitatively validates our theoretical analysis.
[{'version': 'v1', 'created': 'Wed, 2 Apr 2008 16:05:57 GMT'}]
2009-11-13
[array(['Weinert', 'Franz M.', ''], dtype=object) array(['Kraus', 'Jonas A.', ''], dtype=object) array(['Franosch', 'Thomas', ''], dtype=object) array(['Braun', 'Dieter', ''], dtype=object)]
3,945
2204.07504
Pedro De La Puente Sierra
Pedro Alfonso de la Puente, Juan Jos\'e Berdugo Cepeda, Mar\'ia Jos\'e P\'erez Pacheco
Systematic review of development literature from Latin America between 2010- 2021
Working paper, in Spanish language
null
null
null
cs.DL
http://creativecommons.org/licenses/by-nc-sa/4.0/
The purpose of this systematic review is to identify and describe the state of development literature published in Latin America, in Spanish and English, since 2010. For this, we carried out a topographic review of 44 articles available in the most important bibliographic indexes of Latin America, published in journals of diverse disciplines. Our analysis focused on analyzing the nature and composition of literature, finding a large proportion of articles coming from Mexico and Colombia, as well as specialized in the economic discipline. The most relevant articles reviewed show methodological and thematic diversity, with special attention to the problem of growth in Latin American development. An important limitation of this review is the exclusion of articles published in Portuguese, as well as non-indexed literature (such as theses and dissertations). This leads to various recommendations for future reviews of the development literature produced in Latin America.
[{'version': 'v1', 'created': 'Fri, 18 Mar 2022 02:01:56 GMT'}]
2022-04-18
[array(['de la Puente', 'Pedro Alfonso', ''], dtype=object) array(['Cepeda', 'Juan José Berdugo', ''], dtype=object) array(['Pacheco', 'María José Pérez', ''], dtype=object)]
3,946
2208.08509
Wei Zou
Goutham Rajendran, Wei Zou
Analyzing Robustness of End-to-End Neural Models for Automatic Speech Recognition
5 pages, 14 figures
null
null
null
cs.CL cs.LG cs.SD eess.AS
http://creativecommons.org/licenses/by/4.0/
We investigate robustness properties of pre-trained neural models for automatic speech recognition. Real life data in machine learning is usually very noisy and almost never clean, which can be attributed to various factors depending on the domain, e.g. outliers, random noise and adversarial noise. Therefore, the models we develop for various tasks should be robust to such kinds of noisy data, which led to the thriving field of robust machine learning. We consider this important issue in the setting of automatic speech recognition. With the increasing popularity of pre-trained models, it's an important question to analyze and understand the robustness of such models to noise. In this work, we perform a robustness analysis of the pre-trained neural models wav2vec2, HuBERT and DistilHuBERT on the LibriSpeech and TIMIT datasets. We use different kinds of noising mechanisms and measure the model performances as quantified by the inference time and the standard Word Error Rate metric. We also do an in-depth layer-wise analysis of the wav2vec2 model when injecting noise in between layers, enabling us to predict at a high level what each layer learns. Finally for this model, we visualize the propagation of errors across the layers and compare how it behaves on clean versus noisy data. Our experiments conform the predictions of Pasad et al. [2021] and also raise interesting directions for future work.
[{'version': 'v1', 'created': 'Wed, 17 Aug 2022 20:00:54 GMT'}]
2022-08-19
[array(['Rajendran', 'Goutham', ''], dtype=object) array(['Zou', 'Wei', ''], dtype=object)]
3,947
1609.02835
Alessandro Biason
Chiara Pielli, Alessandro Biason, Andrea Zanella and Michele Zorzi
Joint Optimization of Energy Efficiency and Data Compression in TDMA-Based Medium Access Control for the IoT - Extended Version
8 pages, 4 figures, revised and extended version of a paper that was accepted for presentation at IEEE Int. Workshop on Low-Layer Implementation and Protocol Design for IoT Applications (IoT-LINK), GLOBECOM 2016
null
null
null
cs.IT math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Energy efficiency is a key requirement for the Internet of Things, as many sensors are expected to be completely stand-alone and able to run for years without battery replacement. Data compression aims at saving some energy by reducing the volume of data sent over the network, but also affects the quality of the received information. In this work, we formulate an optimization problem to jointly design the source coding and transmission strategies for time-varying channels and sources, with the twofold goal of extending the network lifetime and granting low distortion levels. We propose a scalable offline optimal policy that allocates both energy and transmission parameters (i.e., times and powers) in a network with a dynamic Time Division Multiple Access (TDMA)-based access scheme.
[{'version': 'v1', 'created': 'Fri, 9 Sep 2016 15:32:13 GMT'} {'version': 'v2', 'created': 'Thu, 29 Sep 2016 06:41:59 GMT'}]
2016-09-30
[array(['Pielli', 'Chiara', ''], dtype=object) array(['Biason', 'Alessandro', ''], dtype=object) array(['Zanella', 'Andrea', ''], dtype=object) array(['Zorzi', 'Michele', ''], dtype=object)]
3,948
1611.02199
Alessio Sancetta
Alessio Sancetta
Inference for Additive Models in the Presence of Possibly Infinite Dimensional Nuisance Parameters
null
null
null
null
stat.ME
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A framework for estimation and hypothesis testing of functional restrictions against general alternatives is proposed. The parameter space is a reproducing kernel Hilbert space (RKHS). The null hypothesis does not necessarily define a parametric model. The test allows us to deal with infinite dimensional nuisance parameters. The methodology is based on a moment equation similar in spirit to the construction of the efficient score in semiparametric statistics. The feasible version of such moment equation requires to consistently estimate projections in the space of RKHS and it is shown that this is possible using the proposed approach. This allows us to derive some tractable asymptotic theory and critical values by fast simulation. Simulation results show that the finite sample performance of the test is consistent with the asymptotics and that ignoring the effect of nuisance parameters highly distorts the size of the tests.
[{'version': 'v1', 'created': 'Mon, 7 Nov 2016 18:14:52 GMT'} {'version': 'v2', 'created': 'Thu, 8 Jun 2017 09:30:48 GMT'} {'version': 'v3', 'created': 'Mon, 20 Aug 2018 10:25:21 GMT'}]
2018-08-21
[array(['Sancetta', 'Alessio', ''], dtype=object)]
3,949
0908.2338
Paul Hopkins
Paul Hopkins, Andrew J. Archer, and Robert Evans
Solvent mediated interactions between model colloids and interfaces: A microscopic approach
17 Pages, 13 Figures. Accepted for publication in Journal of Chemical Physics
J. Chem. Phys. 131, 124704 (2009)
10.1063/1.3212888
null
cond-mat.soft
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We determine the solvent mediated contribution to the effective potentials for model colloidal or nano- particles dispersed in a binary solvent that exhibits fluid-fluid phase separation. Using a simple density functional theory we calculate the density profiles of both solvent species in the presence of the `colloids', which are treated as external potentials, and determine the solvent mediated (SM) potentials. Specifically, we calculate SM potentials between (i) two colloids, (ii) a colloid and a planar fluid-fluid interface, and (iii) a colloid and a planar wall with an adsorbed wetting film. We consider three different types of colloidal particles: colloid A which prefers the bulk solvent phase rich in species 2, colloid C which prefers the solvent phase rich in species 1, and `neutral' colloid B which has no strong preference for either phase, i.e. the free energies to insert the colloid into either of the coexisting bulk phases are almost equal. When a colloid which has a preference for one of the two solvent phases is inserted into the disfavored phase at statepoints close to coexistence a thick adsorbed `wetting' film of the preferred phase may form around the colloids. The presence of the adsorbed film has a profound influence on the form of the SM potentials.
[{'version': 'v1', 'created': 'Mon, 17 Aug 2009 12:02:14 GMT'}]
2011-06-24
[array(['Hopkins', 'Paul', ''], dtype=object) array(['Archer', 'Andrew J.', ''], dtype=object) array(['Evans', 'Robert', ''], dtype=object)]
3,950
1910.05349
Tomohiro Oishi
Tomohiro Oishi, Goran Kruzic, and Nils Paar
Relativistic energy-density functional approach to magnetic-dipole excitation and its sum rule
6 pages, 2 figures, 1 table, contribution to the conference proceedings for INPC 2019 in Glasgow, UK (29th July - 2nd August, 2019)
null
null
null
nucl-th astro-ph.HE nucl-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Magnetic-dipole (M1) excitations of $^{18}$O and $^{42}$Ca nuclei are investigated within a relativistic nuclear energy density functional framework. In our last work \cite{2019OP}, these nuclei are found to have unique M1 excitation and its sum rule, because of their characteristic structure: the system consists of the shell-closure core plus two neutrons. For a more systematic investigation of the M1 mode, we have implemented a framework based on the relativistic nuclear energy density functional (RNEDF). For benchmark, we have performed the RNEDF calculations combined with the random-phase approximation (RPA). We evaluate the M1 excitation of $^{18}$O and $^{42}$Ca, whose sum-rule value (SRV) of the M1 transitions can be useful to test the computational implementation \cite{2019OP}. We also apply this RNEDF method to $^{208}$Pb, whose M1 property has been precisely measured \cite{1979Holt,1987Koehler,1988Laszewski,2016Birkhan}. Up to the level of the M1 sum rule, our result is in agreement with the experiments, except the discrepancy related with the quenching factors for $g$ coefficients.
[{'version': 'v1', 'created': 'Fri, 11 Oct 2019 18:00:04 GMT'}]
2019-10-15
[array(['Oishi', 'Tomohiro', ''], dtype=object) array(['Kruzic', 'Goran', ''], dtype=object) array(['Paar', 'Nils', ''], dtype=object)]
3,951
1811.07745
Ariel Keselman
Ariel Keselman, Sergey Ten, Adham Ghazali, Majed Jubeh
Reinforcement Learning with A* and a Deep Heuristic
6 pages 2 figures
null
null
null
cs.LG stat.ML
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A* is a popular path-finding algorithm, but it can only be applied to those domains where a good heuristic function is known. Inspired by recent methods combining Deep Neural Networks (DNNs) and trees, this study demonstrates how to train a heuristic represented by a DNN and combine it with A*. This new algorithm which we call aleph-star can be used efficiently in domains where the input to the heuristic could be processed by a neural network. We compare aleph-star to N-Step Deep Q-Learning (DQN Mnih et al. 2013) in a driving simulation with pixel-based input, and demonstrate significantly better performance in this scenario.
[{'version': 'v1', 'created': 'Mon, 19 Nov 2018 15:15:18 GMT'}]
2018-11-20
[array(['Keselman', 'Ariel', ''], dtype=object) array(['Ten', 'Sergey', ''], dtype=object) array(['Ghazali', 'Adham', ''], dtype=object) array(['Jubeh', 'Majed', ''], dtype=object)]
3,952
1705.01821
D Thirumulanathan
D. Thirumulanathan, Rajesh Sundaresan, and Y Narahari
On Optimal Mechanisms in the Two-Item Single-Buyer Unit-Demand Setting
null
Journal of Mathematical Economics (JME), vol. 82, pp.31--60, 2019
10.1016/j.jmateco.2019.01.005
null
cs.GT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We consider the problem of designing a revenue-optimal mechanism in the two-item, single-buyer, unit-demand setting when the buyer's valuations, $(z_1, z_2)$, are uniformly distributed in an arbitrary rectangle $[c,c+b_1]\times[c,c+b_2]$ in the positive quadrant. We provide a complete and explicit solution for arbitrary nonnegative values of $(c,b_1,b_2)$. We identify five simple structures, each with at most five (possibly stochastic) menu items, and prove that the optimal mechanism has one of the five structures. We also characterize the optimal mechanism as a function of $b_1, b_2$, and $c$. When $c$ is low, the optimal mechanism is a posted price mechanism with an exclusion region; when $c$ is high, it is a posted price mechanism without an exclusion region. Our results are the first to show the existence of optimal mechanisms with no exclusion region, to the best of our knowledge.
[{'version': 'v1', 'created': 'Thu, 4 May 2017 12:47:39 GMT'} {'version': 'v2', 'created': 'Thu, 29 Jun 2017 10:17:20 GMT'} {'version': 'v3', 'created': 'Wed, 31 Jan 2018 19:59:35 GMT'} {'version': 'v4', 'created': 'Wed, 26 Sep 2018 07:26:28 GMT'} {'version': 'v5', 'created': 'Tue, 5 Mar 2019 09:23:56 GMT'}]
2019-03-06
[array(['Thirumulanathan', 'D.', ''], dtype=object) array(['Sundaresan', 'Rajesh', ''], dtype=object) array(['Narahari', 'Y', ''], dtype=object)]
3,953
1712.00910
Yuka Fujiki
Yuka Fujiki, Taro Takaguchi, and Kousuke Yakubo
A general formulation of long-range degree correlations in complex networks
9 pages, 4 figures
Phys. Rev. E 97, 062308 (2018)
10.1103/PhysRevE.97.062308
null
physics.soc-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We provide a general framework for analyzing degree correlations between nodes separated by more than one step (i.e., beyond nearest neighbors) in complex networks. One probability and four conditional probabilities are introduced to fully describe long-range degree correlations with respect to $k$ and $k'$ of two nodes and shortest path length $l$ between them. We present general relations among these probabilities and clarify the relevance to nearest-neighbor degree correlations. Unlike nearest-neighbor correlations, some of these probabilities are meaningful only in finite-size networks. Furthermore, as a baseline to determine the existence or nonexistence of long-range degree correlations in a network, the functional forms of these probabilities for networks without any long-range degree correlations are analytically evaluated within a mean-field approximation. The validity of our argument is demonstrated by applying it to real-world networks.
[{'version': 'v1', 'created': 'Mon, 4 Dec 2017 05:25:32 GMT'}]
2018-06-20
[array(['Fujiki', 'Yuka', ''], dtype=object) array(['Takaguchi', 'Taro', ''], dtype=object) array(['Yakubo', 'Kousuke', ''], dtype=object)]
3,954
2306.03149
Atrideb Chatterjee
Atrideb Chatterjee, Pratika Dayal, Valentin Mauerhofer
Predictions of the 21cm global signal in the JWST and ALMA era
null
null
null
null
astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We calculate the redshift evolution of the global 21cm signal in the first billion years using a semi-analytic galaxy formation model, DELPHI, that jointly tracks the assembly of dark matter halos and their constituent baryons including the impact of supernova feedback and dust enrichment. Employing only two redshift- and mass-independent free parameters, our model predicts galaxy populations in accord with data from both the James Webb Space Telescope (JWST) and the Atacama Large Millimetre Array (ALMA) at $z \sim 5-12$. In addition to this ``fiducial" model, which fully incorporates the impact of dust attenuation, we also explore an unphysical ``maximal" model wherein galaxies can convert a 100\% of their gas into stars instantaneously (and supernova feedback is ignored) required to explain JWST data at $z >=13$. We also explore a wide range of values for our {\it 21cm} parameters that include the impact of X-ray heating ($f_{\rm X,h} =0.02-2.0$) and the escape fraction of Lyman Alpha photons ($f_\alpha = 0.01-1.0$). Our key findings are: (i) the fiducial model predicts a global 21cm signal which reaches a minimum brightness temperature of $ T_{\rm b, min}\sim -215$ mK at a redshift $z_{\rm min} \sim 14$; (ii) since the impact of dust on galaxy properties (such as the star formation rate density) only becomes relevant at $z <= 8$, dust does not have a sensible impact on the global 21cm signal; (iii) the ``maximal" model predicts $T_{\rm b, min}= -210$ mK as early as $z_{\rm min} \sim 18$; (iv) galaxy formation and 21cm parameters have a degenerate impact on the global 21cm signal. A combination of the minimum temperature and its redshift will therefore be crucial in constraining galaxy formation parameters and their coupling to the 21cm signal at these early epochs.
[{'version': 'v1', 'created': 'Mon, 5 Jun 2023 18:04:22 GMT'}]
2023-06-07
[array(['Chatterjee', 'Atrideb', ''], dtype=object) array(['Dayal', 'Pratika', ''], dtype=object) array(['Mauerhofer', 'Valentin', ''], dtype=object)]
3,955
1910.00335
Riccardo Tione
Camillo De Lellis, Guido De Philippis, Bernd Kirchheim, Riccardo Tione
Geometric measure theory and differential inclusions
null
null
null
null
math.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper we consider Lipschitz graphs of functions which are stationary points of strictly polyconvex energies. Such graphs can be thought as integral currents, resp. varifolds, which are stationary for some elliptic integrands. The regularity theory for the latter is a widely open problem, in particular no counterpart of the classical Allard's theorem is known. We address the issue from the point of view of differential inclusions and we show that the relevant ones do not contain the class of laminates which are used in [22] and [25] to construct nonregular solutions. Our result is thus an indication that an Allard's type result might be valid for general elliptic integrands. We conclude the paper by listing a series of open questions concerning the regularity of stationary points for elliptic integrands.
[{'version': 'v1', 'created': 'Tue, 1 Oct 2019 12:20:49 GMT'} {'version': 'v2', 'created': 'Thu, 10 Oct 2019 19:16:18 GMT'}]
2019-10-14
[array(['De Lellis', 'Camillo', ''], dtype=object) array(['De Philippis', 'Guido', ''], dtype=object) array(['Kirchheim', 'Bernd', ''], dtype=object) array(['Tione', 'Riccardo', ''], dtype=object)]
3,956
hep-ph/0107172
Beata Ziaja
B. Ziaja
Low x double $ln^2(1/x)$ resummation effects at the sum rules for nucleon structure function $g_1$
19 pages, latex, 7 figures
Acta Phys.Polon.B32:2863,2001
null
null
hep-ph
null
We have estimated the contributions to the moments of polarized nucleon structure function $g_1(x,Q^2)$ coming from the region of the very low x ($10^{-5}<x$). Our approach uses the nucleon structure function extrapolated to the region of low x by the means of the double $ln^2(1/x)$ resummation. The $Q^2$ evolution of $g_1$ was described by the unified evolution equations incorporating both the leading order Altarelli-Parisi evolution at large and moderate x, and the double $ln^2(1/x)$ resummation at small x. The moments were obtained by integrating out the extrapolated nucleon structure function in the region $10^{-5}<x<1$.
[{'version': 'v1', 'created': 'Mon, 16 Jul 2001 11:59:45 GMT'}]
2014-11-17
[array(['Ziaja', 'B.', ''], dtype=object)]
3,957
2103.02791
Yi Jiang
Wei Zhang and Yi Jiang and Bin Zhou and Die Hu
Hybrid Interference Mitigation Using Analog Prewhitening
11 pages, 11 figures
null
null
null
eess.SP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper proposes a novel scheme for mitigating strong interferences, which is applicable to various wireless scenarios, including full-duplex wireless communications and uncoordinated heterogenous networks. As strong interferences can saturate the receiver's analog-to-digital converters (ADC), they need to be mitigated both before and after the ADCs, i.e., via hybrid processing. The key idea of the proposed scheme, namely the Hybrid Interference Mitigation using Analog Prewhitening (HIMAP), is to insert an M-input M-output analog phase shifter network (PSN) between the receive antennas and the ADCs to spatially prewhiten the interferences, which requires no signal information but only an estimate of the covariance matrix. After interference mitigation by the PSN prewhitener, the preamble can be synchronized, the signal channel response can be estimated, and thus a minimum mean squared error (MMSE) beamformer can be applied in the digital domain to further mitigate the residual interferences. The simulation results verify that the HIMAP scheme can suppress interferences 80dB stronger than the signal by using off-the-shelf phase shifters (PS) of 6-bit resolution.
[{'version': 'v1', 'created': 'Thu, 4 Mar 2021 02:26:08 GMT'}]
2021-03-05
[array(['Zhang', 'Wei', ''], dtype=object) array(['Jiang', 'Yi', ''], dtype=object) array(['Zhou', 'Bin', ''], dtype=object) array(['Hu', 'Die', ''], dtype=object)]
3,958
2005.02212
Daren Wei
Adam Kanigowski, Philipp Kunde, Kurt Vinhage, Daren Wei
Slow entropy of higher rank abelian unipotent actions
29 pages
null
null
null
math.DS
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study slow entropy invariants for abelian unipotent actions $U$ on any finite volume homogeneous space $G/\Gamma$. For every such action we show that the topological slow entropy can be computed directly from the dimension of a special decomposition of $\operatorname{Lie}(G)$ induced by $\operatorname{Lie}(U)$. Moreover, we are able to show that the metric slow entropy of the action coincides with its topological slow entropy. As a corollary, we obtain that the complexity of any abelian horocyclic action is only related to the dimension of $G$. This generalizes the rank one results from [A. Kanigowski, K. Vinhage, D. Wei, Commun. Math. Phys. 370 (2019), no. 2, 449-474.] to higher rank abelian actions.
[{'version': 'v1', 'created': 'Tue, 5 May 2020 14:19:12 GMT'}]
2020-05-06
[array(['Kanigowski', 'Adam', ''], dtype=object) array(['Kunde', 'Philipp', ''], dtype=object) array(['Vinhage', 'Kurt', ''], dtype=object) array(['Wei', 'Daren', ''], dtype=object)]
3,959
2101.07537
Partha Pratim Deka
P. P. Deka, G. C. Dewangan, K. P. Singh and J. Postma
A pair of UV nuclei or a compact star forming region near the active nucleus in Mrk~766?
null
null
10.1007/s12036-021-09695-6
null
astro-ph.GA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We report the discovery of a bright, compact ultraviolet source at a projected separation of 1.1~kpc from the known active galactic nucleus (AGN) in Mrk~766 based on Astrosat/UVIT observations. We perform radial profile analysis and derive the UV flux almost free from the nearby contaminating sources. The new source is about 2.5 and 5.6 times fainter than the AGN in the far and near UV bands. The two sources appear as a pair of nuclei in Mrk~766. We investigate the nature of the new source based on the UV flux ratio, X-ray and optical emission. The new source is highly unlikely to be another accreting supermassive black hole in Mrk~766 as it lacks X-ray emission. We find that the UV/Optical flux of the new source measured at four different bands closely follow the shape of the template spectrum of starburst galaxies. This strongly suggests that the new source is a compact star-forming region.
[{'version': 'v1', 'created': 'Tue, 19 Jan 2021 09:50:57 GMT'}]
2021-06-23
[array(['Deka', 'P. P.', ''], dtype=object) array(['Dewangan', 'G. C.', ''], dtype=object) array(['Singh', 'K. P.', ''], dtype=object) array(['Postma', 'J.', ''], dtype=object)]
3,960
cs/0602065
Paul Vitanyi
Rudi Cilibrasi (CWI) and Paul Vitanyi (CWI and University of Amsterdam)
Similarity of Objects and the Meaning of Words
LaTeX, 25 pages, 7 figures. Proc. 3rd Conf. Theory and Applications of Models of Computation (TAMC), 15-20 May, 2006, Beijing, China (Invited paper) This is an extended version of the 5-page abstract cs.IR/0504089
null
null
null
cs.CV cs.IR
null
We survey the emerging area of compression-based, parameter-free, similarity distance measures useful in data-mining, pattern recognition, learning and automatic semantics extraction. Given a family of distances on a set of objects, a distance is universal up to a certain precision for that family if it minorizes every distance in the family between every two objects in the set, up to the stated precision (we do not require the universal distance to be an element of the family). We consider similarity distances for two types of objects: literal objects that as such contain all of their meaning, like genomes or books, and names for objects. The latter may have literal embodyments like the first type, but may also be abstract like ``red'' or ``christianity.'' For the first type we consider a family of computable distance measures corresponding to parameters expressing similarity according to particular featuresdistances generated by web users corresponding to particular semantic relations between the (names for) the designated objects. For both families we give universal similarity distance measures, incorporating all particular distance measures in the family. In the first case the universal distance is based on compression and in the second case it is based on Google page counts related to search terms. In both cases experiments on a massive scale give evidence of the viability of the approaches. between pairs of literal objects. For the second type we consider similarity
[{'version': 'v1', 'created': 'Fri, 17 Feb 2006 16:15:07 GMT'}]
2007-05-23
[array(['Cilibrasi', 'Rudi', '', 'CWI'], dtype=object) array(['Vitanyi', 'Paul', '', 'CWI and University of\n Amsterdam'], dtype=object) ]
3,961
2010.08523
Alessandro Ravoni
Alessandro Ravoni
Long-term behaviours of Autocatalytic Sets
null
null
null
null
q-bio.MN nlin.AO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Autocatalytic Sets are reaction networks theorised as networks at the basis of life. Their main feature is the ability of spontaneously emerging and self-reproducing. The Reflexively and Food-generated theory provides a formal definition of Autocatalytic Sets in terms of graphs with peculiar topological properties. This formalisation has been proved to be a powerful tool for the study of the chemical networks underlying life, and it was able to identify autocatalytic structures in real metabolic networks. However, the dynamical behaviour of such networks has not been yet complitely clarified. In this work, we present a first attempt to connect the topology of an Autocatalytic Set with its dynamics. For this purpose, we represent Autocatalytic Sets in terms of Chemical Reaction Networks, and we use the Chemical Reaction Network theory to detect motifs in the networks'structure, that allow us to determine the long-term behaviour of the system.
[{'version': 'v1', 'created': 'Fri, 16 Oct 2020 17:29:18 GMT'}]
2020-10-19
[array(['Ravoni', 'Alessandro', ''], dtype=object)]
3,962
math/0509437
Pere Ara
Pere Ara, Martin Mathieu
A not so simple local multiplier algebra
18 pages
null
null
null
math.OA
null
We construct an AF-algebra $A$ such that its local multiplier algebra $M_{\text{loc}}(A)$ does not agree with $M_{\text{loc}}(M_{\text{loc}}(A))$, thus answering a question raised by G.K. Pedersen in 1978.
[{'version': 'v1', 'created': 'Mon, 19 Sep 2005 18:17:47 GMT'}]
2007-05-23
[array(['Ara', 'Pere', ''], dtype=object) array(['Mathieu', 'Martin', ''], dtype=object)]
3,963
1812.07605
Mustafa Kandemir
Mustafa Kandemir, Altan Cakir
Comparison of Plastic Antineutrino Detector Designs in the Context of Near Field Reactor Monitoring
null
Nucl. Instrum. Methods. Phys. Res. A. 927 (2019) 353-361
10.1016/j.nima.2019.02.055
NIMA-D-18-01340
physics.ins-det hep-ex nucl-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We compare existing segmented plastic antineutrino detectors with our new geometrically improved design for antineutrino detection and light collection efficiency. The purpose of this study is to determine the most suitable design style for remote reactor monitoring in the context of nuclear safeguards. Using Monte Carlo based GEANT4 simulation package, we perform detector simulation based on two prominent experiments: Plastic antineutrino detector array (Panda) and Core monitoring by reactor antineutrino detector (Cormorad). In addition to these two well-known designs, another concept, the Panda2, can be obtained by making a small variation of Panda detector, is also considered in the simulation. The results show that the light collection efficiency of the Cormorad is substantially less with respect to the other two detectors while the highest antineutrino detection efficiency is achieved with the Cormorad and Panda2. Furthermore, as an alternative to these design choices, which are composed of an array of identical rectangular-shaped modules, we propose to combine regular hexagonal-shaped modules which minimizes the surface area of the whole detector and consequently reduces the number of optical readout channels considerably. With this approach, it is possible to obtain a detector configuration with a slightly higher detection efficiency with respect to the Panda design and a better energy resolution detector compared to the Cormorad design.
[{'version': 'v1', 'created': 'Tue, 18 Dec 2018 19:17:31 GMT'} {'version': 'v2', 'created': 'Fri, 21 Dec 2018 12:21:04 GMT'} {'version': 'v3', 'created': 'Mon, 18 Feb 2019 12:57:26 GMT'} {'version': 'v4', 'created': 'Wed, 20 Feb 2019 08:20:44 GMT'}]
2019-03-07
[array(['Kandemir', 'Mustafa', ''], dtype=object) array(['Cakir', 'Altan', ''], dtype=object)]
3,964
1812.07944
James Duffy
James A. Duffy and Ioannis Kasparis
Estimation and Inference in the Presence of Fractional d=1/2 and Weakly Nonstationary Processes
Authors' accepted manuscript; to appear in the Annals of Statistics
null
null
null
math.ST stat.TH
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We provide new limit theory for functionals of a general class of processes lying at the boundary between stationarity and nonstationarity -- what we term weakly nonstationary processes (WNPs). This includes, as leading examples, fractional processes with d=1/2, and arrays of autoregressive processes with roots drifting slowly towards unity. We first apply the theory to study inference in parametric and nonparametric regression models involving WNPs as covariates. We then use these results to develop a new specification test for parametric regression models. By construction, our specification test statistic has a chi-squared limiting distribution regardless of the form and extent of persistence of the regressor, implying that a practitioner can validly perform the test using a fixed critical value, while remaining agnostic about the mechanism generating the regressor. Simulation exercises confirm that the test controls size across a wide range of data generating processes, and outperforms a comparable test due to Wang and Phillips (2012, Ann. Stat.) against many alternatives.
[{'version': 'v1', 'created': 'Wed, 19 Dec 2018 13:50:47 GMT'} {'version': 'v2', 'created': 'Thu, 20 Feb 2020 16:39:44 GMT'} {'version': 'v3', 'created': 'Thu, 13 Aug 2020 23:45:01 GMT'}]
2020-08-17
[array(['Duffy', 'James A.', ''], dtype=object) array(['Kasparis', 'Ioannis', ''], dtype=object)]
3,965
1107.2191
Snigdhayan Mahanta
Snigdhayan Mahanta
Assembly maps with coefficients in topological algebras and the integral K-theoretic Novikov conjecture
v2 Exposition improved; one lemma and grant acknowledgement added; v3 some terminology changed and details added, Theorems 4.5 and 4.7 in v3 need an extra hypothesis; v4 abridged version accepted for publication in JHRS
J. Homotopy Relat. Struct., 9 (2), 299-315, 2014
10.1007/s40062-013-0027-6
null
math.KT math.AT math.GT math.OA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We prove that any countable discrete and torsion free subgroup of a general linear group over an arbitrary field or a similar subgroup of an almost connected Lie group satisfies the integral algebraic K-theoretic (split) Novikov conjecture over \cpt and \S, where \cpt denotes the C^*-algebra of compact operators and \S denotes the algebra of Schatten class operators. We introduce assembly maps with finite coefficients and under an additional hypothesis, we prove that such a group also satisfies the algebraic K-theoretic Novikov conjecture over \bar{\mathbb{Q}} and \mathbb{C} with finite coefficients. For all torsion free Gromov hyperbolic groups G, we demonstrate that the canonical algebra homomorphism \cpt[G]\map C^*_r(G)\hat{\otimes}\cpt induces an isomorphism between their algebraic K-theory groups.
[{'version': 'v1', 'created': 'Tue, 12 Jul 2011 05:53:38 GMT'} {'version': 'v2', 'created': 'Tue, 2 Aug 2011 07:40:13 GMT'} {'version': 'v3', 'created': 'Fri, 20 Jan 2012 04:14:12 GMT'} {'version': 'v4', 'created': 'Thu, 20 Jun 2013 15:59:55 GMT'}]
2015-08-05
[array(['Mahanta', 'Snigdhayan', ''], dtype=object)]
3,966
1509.03580
Steven Brunton
Steven L. Brunton, Joshua L. Proctor, J. Nathan Kutz
Discovering governing equations from data: Sparse identification of nonlinear dynamical systems
26 Pages, 13 Figures, 7 Tables
null
10.1073/pnas.1517384113
null
math.DS
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The ability to discover physical laws and governing equations from data is one of humankind's greatest intellectual achievements. A quantitative understanding of dynamic constraints and balances in nature has facilitated rapid development of knowledge and enabled advanced technological achievements, including aircraft, combustion engines, satellites, and electrical power. In this work, we combine sparsity-promoting techniques and machine learning with nonlinear dynamical systems to discover governing physical equations from measurement data. The only assumption about the structure of the model is that there are only a few important terms that govern the dynamics, so that the equations are sparse in the space of possible functions; this assumption holds for many physical systems. In particular, we use sparse regression to determine the fewest terms in the dynamic governing equations required to accurately represent the data. The resulting models are parsimonious, balancing model complexity with descriptive ability while avoiding overfitting. We demonstrate the algorithm on a wide range of problems, from simple canonical systems, including linear and nonlinear oscillators and the chaotic Lorenz system, to the fluid vortex shedding behind an obstacle. The fluid example illustrates the ability of this method to discover the underlying dynamics of a system that took experts in the community nearly 30 years to resolve. We also show that this method generalizes to parameterized, time-varying, or externally forced systems.
[{'version': 'v1', 'created': 'Fri, 11 Sep 2015 16:43:06 GMT'}]
2016-04-27
[array(['Brunton', 'Steven L.', ''], dtype=object) array(['Proctor', 'Joshua L.', ''], dtype=object) array(['Kutz', 'J. Nathan', ''], dtype=object)]
3,967
1107.2852
Ilya Y. Dodin
I. Y. Dodin
Ponderomotive forces and wave dispersion: two sides of the same coin
null
null
null
null
physics.plasm-ph math-ph math.MP quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Presented here is a general view on adiabatic and resonant wave-particle interactions leading to a uniform description of nonlinear ponderomotive effects in very different environments, from low-temperature plasmas to relativistic plasmas or even atoms in laser light. Treating the wave-particle interaction as a classical mode-coupling problem, this theory shows the inherent connection between the ponderomotive forces and the properties of waves causing those forces. The adiabatic Lagrangians are derived for single particles and nonlinear waves, possibly carrying trapped particles, and yield both the dynamic equations and the nonlinear dispersion relations in the general case.
[{'version': 'v1', 'created': 'Thu, 14 Jul 2011 15:35:53 GMT'}]
2011-07-15
[array(['Dodin', 'I. Y.', ''], dtype=object)]
3,968
0712.3691
Christian Sevenheck
Claus Hertling, Christian Sevenheck
Curvature of classifying spaces for Brieskorn lattices
25 pages
null
10.1016/j.geomphys.2008.07.008
null
math.AG math.DG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study tt*-geometry on the classifying space for regular singular TERP-structures, e.g., Fourier-Laplace transformations of Brieskorn lattices of isolated hypersurface singularities. We show that (a part of) this classifying space can be canonically equipped with a hermitian structure. We derive an estimate for the holomorphic sectional curvature of this hermitian metric, which is the analogue of a similar result for classifying spaces of pure polarized Hodge structures.
[{'version': 'v1', 'created': 'Fri, 21 Dec 2007 13:30:16 GMT'} {'version': 'v2', 'created': 'Mon, 14 Jul 2008 16:27:20 GMT'} {'version': 'v3', 'created': 'Tue, 5 Aug 2008 11:38:56 GMT'}]
2009-11-13
[array(['Hertling', 'Claus', ''], dtype=object) array(['Sevenheck', 'Christian', ''], dtype=object)]
3,969
2112.12825
Takuya Okugawa
T. Okugawa, A. Benyamini, A. J. Millis, and D. M. Kennes
Anti-Poiseuille Flow: Increased Vortex Velocity at Superconductor Edges
null
null
10.1103/PhysRevB.105.224512
null
cond-mat.supr-con
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Using the time-dependent Ginzburg Landau equations we study vortex motion driven by an applied current in two dimensional superconductors in the presence of a physical boundary. At smaller sourced currents the vortex lattice moves as a whole, with each vortex moving at the same velocity. At larger sourced current, vortex motion is organized into channels, with vortices in channels nearer to the sample edges moving faster than those farther away from sample edges, opposite to the Poiseuille flow of basic hydrodynamics where the velocity is lowest at the boundaries. At intermediate currents, a stick-slip motion of the vortex lattice occurs in which vortices in the channel at the boundary break free from the Abrikosov lattice, accelerate, move past their neighbors and then slow down and reattach to the vortex lattice at which point the stick-slip process starts over. These effects could be observed experimentally, e.g. using fast scanning microscopy techniques.
[{'version': 'v1', 'created': 'Thu, 23 Dec 2021 19:58:19 GMT'}]
2022-07-13
[array(['Okugawa', 'T.', ''], dtype=object) array(['Benyamini', 'A.', ''], dtype=object) array(['Millis', 'A. J.', ''], dtype=object) array(['Kennes', 'D. M.', ''], dtype=object)]
3,970
0908.4199
Muhammad Sharif
M. Sharif and Umber Sheikh
Wave Properties of Isothermal Magneto-Rotational Fluids
29 pages, 24 figures accepted for publication in Canadian J. Physics
Canadian J. Phys. 87(2009)879-894
10.1139/P09-025
null
gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, the isothermal plasma wave properties in the neighborhood of the pair production region for the Kerr black hole magnetosphere are discussed. We have considered the Fourier analyzed form of the perturbed general relativistic magnetohydrodynamical equations whose determinant leads to a dispersion relation. For the special scenario, the $x$-component of the complex wave vectors are numerically calculated. Respective components of the propagation vector, attenuation vector, phase and group velocities are shown in graphs. We have particularly investigated the existence of a Veselago medium and wave behavior (modes of waves dispersion
[{'version': 'v1', 'created': 'Fri, 28 Aug 2009 08:29:20 GMT'}]
2015-05-14
[array(['Sharif', 'M.', ''], dtype=object) array(['Sheikh', 'Umber', ''], dtype=object)]
3,971
1308.5289
Andreea Nicoara
Andreea C. Nicoara
Coherence and Other Properties of Sheaves in the Kohn Algorithm
12 pages
International Journal of Mathematics 25 (2014) no.8
10.1142/S0129167X14500773
null
math.AG math.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In the smooth case, we prove quasi-flasqueness for the sheaves of all subelliptic multipliers as well as at each of the steps of the Kohn algorithm on a pseudoconvex domain in $\C^n.$ We use techniques by Jean-Claude Tougeron to show that if the domain has a real-analytic defining function, the modified Kohn algorithm involving generating ideals and taking real radicals only in the ring of real-analytic germs yields quasi-coherent sheaves. This sharpens a result obtained by J. J. Kohn in 1979.
[{'version': 'v1', 'created': 'Sat, 24 Aug 2013 03:52:29 GMT'}]
2014-08-13
[array(['Nicoara', 'Andreea C.', ''], dtype=object)]
3,972
2010.15526
Kelly Payette
Kelly Payette, Priscille de Dumast, Hamza Kebiri, Ivan Ezhov, Johannes C. Paetzold, Suprosanna Shit, Asim Iqbal, Romesa Khan, Raimund Kottke, Patrice Grehten, Hui Ji, Levente Lanczi, Marianna Nagy, Monika Beresova, Thi Dao Nguyen, Giancarlo Natalucci, Theofanis Karayannis, Bjoern Menze, Meritxell Bach Cuadra, Andras Jakab
An automatic multi-tissue human fetal brain segmentation benchmark using the Fetal Tissue Annotation Dataset
This is a preprint of an article published in Nature Scientific Data. The final authenticated version is available online at: https://doi.org/10.1038/s41597-021-00946-3
Sci Data 8, 167 (2021)
10.1038/s41597-021-00946-3
null
eess.IV cs.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
It is critical to quantitatively analyse the developing human fetal brain in order to fully understand neurodevelopment in both normal fetuses and those with congenital disorders. To facilitate this analysis, automatic multi-tissue fetal brain segmentation algorithms are needed, which in turn requires open databases of segmented fetal brains. Here we introduce a publicly available database of 50 manually segmented pathological and non-pathological fetal magnetic resonance brain volume reconstructions across a range of gestational ages (20 to 33 weeks) into 7 different tissue categories (external cerebrospinal fluid, grey matter, white matter, ventricles, cerebellum, deep grey matter, brainstem/spinal cord). In addition, we quantitatively evaluate the accuracy of several automatic multi-tissue segmentation algorithms of the developing human fetal brain. Four research groups participated, submitting a total of 10 algorithms, demonstrating the benefits the database for the development of automatic algorithms.
[{'version': 'v1', 'created': 'Thu, 29 Oct 2020 12:46:05 GMT'} {'version': 'v2', 'created': 'Tue, 16 Feb 2021 15:39:55 GMT'} {'version': 'v3', 'created': 'Thu, 29 Apr 2021 14:53:33 GMT'} {'version': 'v4', 'created': 'Wed, 7 Jul 2021 12:17:26 GMT'}]
2021-07-08
[array(['Payette', 'Kelly', ''], dtype=object) array(['de Dumast', 'Priscille', ''], dtype=object) array(['Kebiri', 'Hamza', ''], dtype=object) array(['Ezhov', 'Ivan', ''], dtype=object) array(['Paetzold', 'Johannes C.', ''], dtype=object) array(['Shit', 'Suprosanna', ''], dtype=object) array(['Iqbal', 'Asim', ''], dtype=object) array(['Khan', 'Romesa', ''], dtype=object) array(['Kottke', 'Raimund', ''], dtype=object) array(['Grehten', 'Patrice', ''], dtype=object) array(['Ji', 'Hui', ''], dtype=object) array(['Lanczi', 'Levente', ''], dtype=object) array(['Nagy', 'Marianna', ''], dtype=object) array(['Beresova', 'Monika', ''], dtype=object) array(['Nguyen', 'Thi Dao', ''], dtype=object) array(['Natalucci', 'Giancarlo', ''], dtype=object) array(['Karayannis', 'Theofanis', ''], dtype=object) array(['Menze', 'Bjoern', ''], dtype=object) array(['Cuadra', 'Meritxell Bach', ''], dtype=object) array(['Jakab', 'Andras', ''], dtype=object)]
3,973
2202.07761
Alexandros Hollender
Mika G\"o\"os, Alexandros Hollender, Siddhartha Jain, Gilbert Maystre, William Pires, Robert Robere, Ran Tao
Further Collapses in TFNP
null
null
null
null
cs.CC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We show $\textsf{EOPL}=\textsf{PLS}\cap\textsf{PPAD}$. Here the class $\textsf{EOPL}$ consists of all total search problems that reduce to the End-of-Potential-Line problem, which was introduced in the works by Hubacek and Yogev (SICOMP 2020) and Fearnley et al. (JCSS 2020). In particular, our result yields a new simpler proof of the breakthrough collapse $\textsf{CLS}=\textsf{PLS}\cap\textsf{PPAD}$ by Fearnley et al. (STOC 2021). We also prove a companion result $\textsf{SOPL}=\textsf{PLS}\cap\textsf{PPADS}$, where $\textsf{SOPL}$ is the class associated with the Sink-of-Potential-Line problem.
[{'version': 'v1', 'created': 'Tue, 15 Feb 2022 22:24:36 GMT'} {'version': 'v2', 'created': 'Fri, 20 May 2022 17:36:32 GMT'}]
2022-05-23
[array(['Göös', 'Mika', ''], dtype=object) array(['Hollender', 'Alexandros', ''], dtype=object) array(['Jain', 'Siddhartha', ''], dtype=object) array(['Maystre', 'Gilbert', ''], dtype=object) array(['Pires', 'William', ''], dtype=object) array(['Robere', 'Robert', ''], dtype=object) array(['Tao', 'Ran', ''], dtype=object)]
3,974
0710.0278
Chao-Yang Lu
Chao-Yang Lu, Wei-Bo Gao, Otfried G\"uhne, Xiao-Qi Zhou, Zeng-Bing Chen, Jian-Wei Pan
Demonstrating anyonic fractional statistics with a six-qubit quantum simulator
revised version 3, revTex, 4.3 pages, 4 figures, notes and reference added
Phys.Rev.Lett.102:030502,2009
10.1103/PhysRevLett.102.030502
null
quant-ph cond-mat.stat-mech
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Anyons are exotic quasiparticles living in two dimensions that do not fit into the usual categories of fermions and bosons, but obey a new form of fractional statistics. Following a recent proposal [Phys. Rev. Lett. 98, 150404 (2007)], we present an experimental demonstration of the fractional statistics of anyons in the Kitaev spin lattice model using a photonic quantum simulator. We dynamically create the ground state and excited states (which are six-qubit graph states) of the Kitaev model Hamiltonian, and implement the anyonic braiding and fusion operations by single-qubit rotations. A phase shift of $\pi$ related to the anyon braiding is observed, confirming the prediction of the fractional statistics of Abelian 1/2-anyons.
[{'version': 'v1', 'created': 'Mon, 1 Oct 2007 12:46:41 GMT'} {'version': 'v2', 'created': 'Thu, 31 Jan 2008 12:19:33 GMT'} {'version': 'v3', 'created': 'Thu, 16 Oct 2008 03:52:28 GMT'}]
2010-04-22
[array(['Lu', 'Chao-Yang', ''], dtype=object) array(['Gao', 'Wei-Bo', ''], dtype=object) array(['Gühne', 'Otfried', ''], dtype=object) array(['Zhou', 'Xiao-Qi', ''], dtype=object) array(['Chen', 'Zeng-Bing', ''], dtype=object) array(['Pan', 'Jian-Wei', ''], dtype=object)]
3,975
2301.13814
Chunwei Hsu
Chunwei Hsu, Michael Rohde, Gabriela Borin Barin, Guido Gandus, Daniele Passerone, Mathieu Luisier, Pascal Ruffieux, Roman Fasel, Herre S. J. van der Zant, Maria El Abbassi
Platinum contacts for 9-atom-wide armchair graphene nanoribbons
6 pages, 5 figures
Appl. Phys. Lett. 122, 173104 (2023)
10.1063/5.0143663
null
cond-mat.mes-hall
http://creativecommons.org/licenses/by/4.0/
Creating a good contact between electrodes and graphene nanoribbons (GNRs) has been a longstanding challenge in searching for the next GNR-based nanoelectronics. This quest requires the controlled fabrication of sub-20 nm metallic gaps, a clean GNR transfer minimizing damage and organic contamination during the device fabrication, as well as work function matching to minimize the contact resistance. Here, we transfer 9-atom-wide armchair-edged GNRs (9-AGNRs) grown on Au(111)/mica substrates to pre-patterned platinum electrodes, yielding polymer-free 9-AGNR field-effect transistor devices. Our devices have a resistance in the range of $10^6$ to $10^8$ $\Omega$ in the low-bias regime, which is 2 to 4 orders of magnitude lower than previous reports. Density functional theory (DFT) calculations combined with the non-equilibrium Green's function method (NEGF) explain the observed p-type electrical characteristics and further demonstrate that platinum gives strong coupling and higher transmission in comparison to other materials such as graphene.
[{'version': 'v1', 'created': 'Tue, 31 Jan 2023 18:01:23 GMT'}]
2023-05-01
[array(['Hsu', 'Chunwei', ''], dtype=object) array(['Rohde', 'Michael', ''], dtype=object) array(['Barin', 'Gabriela Borin', ''], dtype=object) array(['Gandus', 'Guido', ''], dtype=object) array(['Passerone', 'Daniele', ''], dtype=object) array(['Luisier', 'Mathieu', ''], dtype=object) array(['Ruffieux', 'Pascal', ''], dtype=object) array(['Fasel', 'Roman', ''], dtype=object) array(['van der Zant', 'Herre S. J.', ''], dtype=object) array(['Abbassi', 'Maria El', ''], dtype=object)]
3,976
1705.02985
Charles Jeon
Ramina Ghods, Charles Jeon, Gulnar Mirza, Arian Maleki, and Christoph Studer
Optimally-Tuned Nonparametric Linear Equalization for Massive MU-MIMO Systems
Will be presented at the 2017 IEEE International Symposium on Information Theory
null
null
null
cs.IT eess.SP math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper deals with linear equalization in massive multi-user multiple-input multiple-output (MU-MIMO) wireless systems. We first provide simple conditions on the antenna configuration for which the well-known linear minimum mean-square error (L-MMSE) equalizer provides near-optimal spectral efficiency, and we analyze its performance in the presence of parameter mismatches in the signal and/or noise powers. We then propose a novel, optimally-tuned NOnParametric Equalizer (NOPE) for massive MU-MIMO systems, which avoids knowledge of the transmit signal and noise powers altogether. We show that NOPE achieves the same performance as that of the L-MMSE equalizer in the large-antenna limit, and we demonstrate its efficacy in realistic, finite-dimensional systems. From a practical perspective, NOPE is computationally efficient and avoids dedicated training that is typically required for parameter estimation
[{'version': 'v1', 'created': 'Mon, 8 May 2017 17:34:30 GMT'}]
2018-11-12
[array(['Ghods', 'Ramina', ''], dtype=object) array(['Jeon', 'Charles', ''], dtype=object) array(['Mirza', 'Gulnar', ''], dtype=object) array(['Maleki', 'Arian', ''], dtype=object) array(['Studer', 'Christoph', ''], dtype=object)]
3,977
1405.2131
Jiangtao Su
J.T. Su, J. Jing, S. Wang, T. Wiegelmann and H.M. Wang
Statistical study of free magnetic energy and flare productivity of solar active regions
The paper was submitted to ApJ and it is accepted now
null
10.1088/0004-637X/788/2/150
null
astro-ph.SR
http://creativecommons.org/licenses/by-nc-sa/3.0/
Photospheric vector magnetograms from Helioseismic and Magnetic Imager on board the Solar Dynamic Observatory are utilized as the boundary conditions to extrapolate both non-linear force-free and potential magnetic fields in solar corona. Based on the extrapolations, we are able to determine the free magnetic energy (FME) stored in active regions (ARs). Over 3000 vector magnetograms in 61 ARs were analyzed. We compare FME with ARs' flare index (FI) and find that there is a weak correlation ($<60\%$) between FME and FI. FME shows slightly improved flare predictability relative to total unsigned magnetic flux of ARs in the following two aspects: (1) the flare productivity predicted by FME is higher than that predicted by magnetic flux and (2) the correlation between FI and FME is higher than that between FI and magnetic flux. However, this improvement is not significant enough to make a substantial difference in time-accumulated FI, rather than individual flare, predictions.
[{'version': 'v1', 'created': 'Fri, 9 May 2014 02:15:03 GMT'}]
2015-06-19
[array(['Su', 'J. T.', ''], dtype=object) array(['Jing', 'J.', ''], dtype=object) array(['Wang', 'S.', ''], dtype=object) array(['Wiegelmann', 'T.', ''], dtype=object) array(['Wang', 'H. M.', ''], dtype=object)]
3,978
1606.08144
Giampiero Esposito Dr.
Giampiero Esposito, Raju Roychowdhury
From pseudo-holomorphic functions to the associated real manifold
25 pages
null
null
null
math.CV math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper studies first the differential inequalities that make it possible to build a global theory of pseudo-holomorphic functions in the case of one or several complex variables. In the case of one complex dimension, we prove that the differential inequalities describing pseudo-holomorphic functions can be used to define a one-real-dimensional manifold (by the vanishing of a function with nonzero gradient), which is here a 1-parameter family of plane curves. On studying the associated envelopes, such a parameter can be eliminated by solving two nonlinear partial differential equations. The classical differential geometry of curves can be therefore exploited to get a novel perspective on the equations describing the global theory of pseudo-holomorphic functions.
[{'version': 'v1', 'created': 'Mon, 27 Jun 2016 07:23:17 GMT'}]
2016-06-28
[array(['Esposito', 'Giampiero', ''], dtype=object) array(['Roychowdhury', 'Raju', ''], dtype=object)]
3,979
1711.00403
Eduardo Rozo
DES Collaboration: T. M. C. Abbott, F. B. Abdalla, J. Annis, K. Bechtol, B. A. Benson, R. A. Bernstein, G. M. Bernstein, E. Bertin, D. Brooks, D. L. Burke, A. Carnero Rosell, M. Carrasco Kind, J. Carretero, F. J. Castander, C. L. Chang, T. M. Crawford, C. E. Cunha, C. B. D'Andrea, L. N. da Costa, C. Davis, S. Desai, H. T. Diehl, J. P. Dietrich, P. Doel, A. Drlica-Wagner, A. E. Evrard, E. Fernandez, B. Flaugher, J. Frieman, J. Garcia-Bellido, E. Gaztanaga, D. W. Gerdes, T. Giannantonio, D. Gruen, R. A. Gruendl, J. Gschwend, G. Gutierrez, W. G. Hartley, J. W. Henning, K. Honscheid, B. Hoyle, B. Jain, D. J. James, M. Jarvis, T. Jeltema, M. D. Johnson, M. W. G. Johnson, E. Krause, K. Kuehn, S. Kuhlmann, N. Kuropatkin, O. Lahav, A. R. Liddle, M. Lima, H. Lin, M. A. G. Maia, A. Manzotti, M. March, J. L. Marshall, R. Miquel, J. J. Mohr, T. Natoli, P. Nugent, R. L. C. Ogando, Y. Park, A. A. Plazas, C. L. Reichardt, K. Reil, A. Roodman, A. J. Ross, E. Rozo, E. S. Rykoff, E. Sanchez, V. Scarpine, M. Schubnell, I. Sevilla-Noarbe, M. Smith, R. C. Smith, M. Soares-Santos, F. Sobreira, E. Suchyta, G. Tarle, D. Thomas, M. A. Troxel, A. R. Walker, R. H. Wechsler, J. Weller, W. Wester, W. L. K. Wu, J. Zuntz
Dark Energy Survey Year 1 Results: A Precise H0 Measurement from DES Y1, BAO, and D/H Data
11 pages, 2 figures
null
10.1093/mnras/sty1939
null
astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We combine Dark Energy Survey Year 1 clustering and weak lensing data with Baryon Acoustic Oscillations (BAO) and Big Bang Nucleosynthesis (BBN) experiments to constrain the Hubble constant. Assuming a flat $\Lambda$CDM model with minimal neutrino mass ($\sum m_\nu = 0.06$ eV) we find $H_0=67.2^{+1.2}_{-1.0}$ km/s/Mpc (68% CL). This result is completely independent of Hubble constant measurements based on the distance ladder, Cosmic Microwave Background (CMB) anisotropies (both temperature and polarization), and strong lensing constraints. There are now five data sets that: a) have no shared observational systematics; and b) each constrain the Hubble constant with a few percent level precision. We compare these five independent measurements, and find that, as a set, the differences between them are significant at the $2.1\sigma$ level ($\chi^2/dof=20.1/11$, probability to exceed=4%). This difference is low enough that we consider the data sets statistically consistent with each other. The best fit Hubble constant obtained by combining all five data sets is $H_0 = 69.1^{+0.4}_{-0.6}$ km/s/Mpc.
[{'version': 'v1', 'created': 'Wed, 1 Nov 2017 15:42:57 GMT'}]
2018-08-29
[array(['DES Collaboration', '', ''], dtype=object) array(['Abbott', 'T. M. C.', ''], dtype=object) array(['Abdalla', 'F. B.', ''], dtype=object) array(['Annis', 'J.', ''], dtype=object) array(['Bechtol', 'K.', ''], dtype=object) array(['Benson', 'B. A.', ''], dtype=object) array(['Bernstein', 'R. A.', ''], dtype=object) array(['Bernstein', 'G. M.', ''], dtype=object) array(['Bertin', 'E.', ''], dtype=object) array(['Brooks', 'D.', ''], dtype=object) array(['Burke', 'D. L.', ''], dtype=object) array(['Rosell', 'A. Carnero', ''], dtype=object) array(['Kind', 'M. Carrasco', ''], dtype=object) array(['Carretero', 'J.', ''], dtype=object) array(['Castander', 'F. J.', ''], dtype=object) array(['Chang', 'C. L.', ''], dtype=object) array(['Crawford', 'T. M.', ''], dtype=object) array(['Cunha', 'C. E.', ''], dtype=object) array(["D'Andrea", 'C. B.', ''], dtype=object) array(['da Costa', 'L. N.', ''], dtype=object) array(['Davis', 'C.', ''], dtype=object) array(['Desai', 'S.', ''], dtype=object) array(['Diehl', 'H. T.', ''], dtype=object) array(['Dietrich', 'J. P.', ''], dtype=object) array(['Doel', 'P.', ''], dtype=object) array(['Drlica-Wagner', 'A.', ''], dtype=object) array(['Evrard', 'A. E.', ''], dtype=object) array(['Fernandez', 'E.', ''], dtype=object) array(['Flaugher', 'B.', ''], dtype=object) array(['Frieman', 'J.', ''], dtype=object) array(['Garcia-Bellido', 'J.', ''], dtype=object) array(['Gaztanaga', 'E.', ''], dtype=object) array(['Gerdes', 'D. W.', ''], dtype=object) array(['Giannantonio', 'T.', ''], dtype=object) array(['Gruen', 'D.', ''], dtype=object) array(['Gruendl', 'R. A.', ''], dtype=object) array(['Gschwend', 'J.', ''], dtype=object) array(['Gutierrez', 'G.', ''], dtype=object) array(['Hartley', 'W. G.', ''], dtype=object) array(['Henning', 'J. W.', ''], dtype=object) array(['Honscheid', 'K.', ''], dtype=object) array(['Hoyle', 'B.', ''], dtype=object) array(['Jain', 'B.', ''], dtype=object) array(['James', 'D. J.', ''], dtype=object) array(['Jarvis', 'M.', ''], dtype=object) array(['Jeltema', 'T.', ''], dtype=object) array(['Johnson', 'M. D.', ''], dtype=object) array(['Johnson', 'M. W. G.', ''], dtype=object) array(['Krause', 'E.', ''], dtype=object) array(['Kuehn', 'K.', ''], dtype=object) array(['Kuhlmann', 'S.', ''], dtype=object) array(['Kuropatkin', 'N.', ''], dtype=object) array(['Lahav', 'O.', ''], dtype=object) array(['Liddle', 'A. R.', ''], dtype=object) array(['Lima', 'M.', ''], dtype=object) array(['Lin', 'H.', ''], dtype=object) array(['Maia', 'M. A. G.', ''], dtype=object) array(['Manzotti', 'A.', ''], dtype=object) array(['March', 'M.', ''], dtype=object) array(['Marshall', 'J. L.', ''], dtype=object) array(['Miquel', 'R.', ''], dtype=object) array(['Mohr', 'J. J.', ''], dtype=object) array(['Natoli', 'T.', ''], dtype=object) array(['Nugent', 'P.', ''], dtype=object) array(['Ogando', 'R. L. C.', ''], dtype=object) array(['Park', 'Y.', ''], dtype=object) array(['Plazas', 'A. A.', ''], dtype=object) array(['Reichardt', 'C. L.', ''], dtype=object) array(['Reil', 'K.', ''], dtype=object) array(['Roodman', 'A.', ''], dtype=object) array(['Ross', 'A. J.', ''], dtype=object) array(['Rozo', 'E.', ''], dtype=object) array(['Rykoff', 'E. S.', ''], dtype=object) array(['Sanchez', 'E.', ''], dtype=object) array(['Scarpine', 'V.', ''], dtype=object) array(['Schubnell', 'M.', ''], dtype=object) array(['Sevilla-Noarbe', 'I.', ''], dtype=object) array(['Smith', 'M.', ''], dtype=object) array(['Smith', 'R. C.', ''], dtype=object) array(['Soares-Santos', 'M.', ''], dtype=object) array(['Sobreira', 'F.', ''], dtype=object) array(['Suchyta', 'E.', ''], dtype=object) array(['Tarle', 'G.', ''], dtype=object) array(['Thomas', 'D.', ''], dtype=object) array(['Troxel', 'M. A.', ''], dtype=object) array(['Walker', 'A. R.', ''], dtype=object) array(['Wechsler', 'R. H.', ''], dtype=object) array(['Weller', 'J.', ''], dtype=object) array(['Wester', 'W.', ''], dtype=object) array(['Wu', 'W. L. K.', ''], dtype=object) array(['Zuntz', 'J.', ''], dtype=object)]
3,980
2012.10413
Mikhail Nesterenko
Kendric Hood, Joseph Oglio, Mikhail Nesterenko, and Gokarna Sharma
Partitionable Asynchronous Cryptocurrency Blockchain
null
null
null
null
cs.DC
http://creativecommons.org/licenses/by/4.0/
We consider operation of blockchain-based cryptocurrency in case of partitioning. We define the Partitionable Blockchain Consensus Problem. The problem may have an interesting solution if the partitions proceed independently by splitting accounts. We prove that this problem is not solvable in the asynchronous system. The peers in the two partitions may not agree on the last jointly mined block or, alternatively, on the starting point of independent concurrent computation. We introduce a family of detectors that enable a solution. We establish the relationship between detectors. We present the algorithm that solves the Partitionable Blockchain Consensus Problem using our detectors. We extend our solution to multiple splits, message loss and to partition merging. We simulate and evaluate the performance of detectors, discuss the implementation of the detectors and future work.
[{'version': 'v1', 'created': 'Fri, 18 Dec 2020 18:07:02 GMT'}]
2020-12-21
[array(['Hood', 'Kendric', ''], dtype=object) array(['Oglio', 'Joseph', ''], dtype=object) array(['Nesterenko', 'Mikhail', ''], dtype=object) array(['Sharma', 'Gokarna', ''], dtype=object)]
3,981
1710.06470
Gelasio Salazar
Carolina Medina, Jorge Ram\'irez-Alfons\'in, Gelasio Salazar
On the number of unknot diagrams
null
null
null
null
math.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Let $D$ be a knot diagram, and let ${\mathcal D}$ denote the set of diagrams that can be obtained from $D$ by crossing exchanges. If $D$ has $n$ crossings, then ${\mathcal D}$ consists of $2^n$ diagrams. A folklore argument shows that at least one of these $2^n$ diagrams is unknot, from which it follows that every diagram has finite unknotting number. It is easy to see that this argument can be used to show that actually ${\mathcal D}$ has more than one unknot diagram, but it cannot yield more than $4n$ unknot diagrams. We improve this linear bound to a superpolynomial bound, by showing that at least $2^{\sqrt[3]{n}}$ of the diagrams in ${\mathcal D}$ are unknot. We also show that either all the diagrams in ${\mathcal D}$ are unknot, or there is a diagram in ${\mathcal D}$ that is a diagram of the trefoil knot.
[{'version': 'v1', 'created': 'Tue, 17 Oct 2017 18:56:21 GMT'}]
2017-10-19
[array(['Medina', 'Carolina', ''], dtype=object) array(['Ramírez-Alfonsín', 'Jorge', ''], dtype=object) array(['Salazar', 'Gelasio', ''], dtype=object)]
3,982
2012.13973
Hoang Son Le Mr
Hoang Son Le, Rini Akmeliawati, Gustavo Carneiro
Domain Generalisation with Domain Augmented Supervised Contrastive Learning (Student Abstract)
null
null
null
null
cs.LG cs.CV
http://creativecommons.org/licenses/by/4.0/
Domain generalisation (DG) methods address the problem of domain shift, when there is a mismatch between the distributions of training and target domains. Data augmentation approaches have emerged as a promising alternative for DG. However, data augmentation alone is not sufficient to achieve lower generalisation errors. This project proposes a new method that combines data augmentation and domain distance minimisation to address the problems associated with data augmentation and provide a guarantee on the learning performance, under an existing framework. Empirically, our method outperforms baseline results on DG benchmarks.
[{'version': 'v1', 'created': 'Sun, 27 Dec 2020 16:50:40 GMT'}]
2020-12-29
[array(['Le', 'Hoang Son', ''], dtype=object) array(['Akmeliawati', 'Rini', ''], dtype=object) array(['Carneiro', 'Gustavo', ''], dtype=object)]
3,983
0802.1242
Harsha Sanjeev Kumar
Harsha Sanjeev Kumar, Samar Safi-Harb
Variability of the High-Magnetic Field X-ray Pulsar PSR J1846-0258 Associated with the Supernova Remnant Kes 75 as Revealed by the Chandra X-ray Observatory
Accepted by the Astrophysical Journal (Letters)
null
null
null
astro-ph
null
We present results from the archival Chandra observations of the 0.3 s X-ray pulsar PSR J1846-0258 associated with the supernova remnant (SNR) Kes 75. The pulsar has the highest spin-down luminosity (Edot = 8.3e36 erg/s) among all the high magnetic field pulsars (HBPs) and has been classified as a Crab-like pulsar despite its magnetic field (5e13 G) being above the quantum critical field. It is the only HBP described by a non-thermal Crab-like spectrum, powering a bright pulsar wind nebula (PWN). Our spectroscopic study shows evidence of spectral softening (photon index = 1.32 to 1.97) and temporal brightening (unabsorbed flux = 4.3e-12 to 2.7e-11 erg/cm^2/s) of the pulsar by ~6 times from 2000 to 2006. The 0.5-10 keV luminosity of the pulsar at the revised distance of 6 kpc has also increased from 1.85e34 to 1.16e35 erg/s, and the X-ray efficiency increased from 0.2% to 1.4%. The observed X-ray brightening and softening of the pulsar suggests for the first time that this HBP is revealing itself as a magnetar.
[{'version': 'v1', 'created': 'Sun, 10 Feb 2008 21:21:55 GMT'} {'version': 'v2', 'created': 'Wed, 20 Feb 2008 16:26:09 GMT'} {'version': 'v3', 'created': 'Mon, 17 Mar 2008 19:14:20 GMT'}]
2008-03-17
[array(['Kumar', 'Harsha Sanjeev', ''], dtype=object) array(['Safi-Harb', 'Samar', ''], dtype=object)]
3,984
1408.0656
Seungwoo Lee
Seungwoo Lee and Juyoung Kim
Efficient Confinement of Ultraviolet Light into the Self-Assembled, Dielectric Colloidal Monolayer on a Flat Aluminum Film
null
null
10.7567/APEX.7.112002
null
physics.optics
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Here we propose the efficient confinement of ultraviolet (UV) light into the plasmonic-photonic crystal hybrid, which can be practically developed by the self-assembly of dielectric colloidal nanosphere monolayer onto a flat aluminum (Al) film. Using a numerical approach, we analyzed modal characteristics of each different resonant mode at the UV wavelengths including surface plasmon polariton (SPP) mode and waveguided (WG) mode and tuned these resonant modes from deep to far UV simply by adjusting the size of dielectric colloidal nanosphere. The calculated quality-factor (Q-factor) of such plasmonic-photonic crystal hybrid is at least one order of magnitude higher than that of the existing Al nanostructures (Al nanoparticles, nanodisks, nanovoids, or nanogratings) standing on the dielectric substrate. Also, we systematically studied how the amount of native oxide, which can be generated during the general process for the deposition of Al, can influence on both the SPP and WG modes of such plasmonic-photonic crystal hybrid in order to guide strategies for a realistic experimental fabrication and exploitation of relevant optical responses. We anticipate that the theoretical results in this paper enable a promising step in the enhancement of UV light interaction with the nanophotonic structure in a versatile, but highly efficient way.
[{'version': 'v1', 'created': 'Mon, 4 Aug 2014 12:24:36 GMT'}]
2015-06-22
[array(['Lee', 'Seungwoo', ''], dtype=object) array(['Kim', 'Juyoung', ''], dtype=object)]
3,985
gr-qc/0701062
Earnest Harrison
Earnest Harrison
Embedding the Schwarzschild Ideal Fluid Metric
5 pages, 9 figures, minor correction
null
null
null
gr-qc
null
Certain semi-Riemannian metrics can be decomposed into a Riemannian part and an isochronal part. The properties of such metrics are particularly easy to visualize in a coordinate-free way, using isometric embedding. We present such an isochronal, isometric embedding of the well known Schwarzschild ideal fluid metric in an attempt to see what is happening when the pressure becomes singular.
[{'version': 'v1', 'created': 'Thu, 11 Jan 2007 14:50:31 GMT'} {'version': 'v2', 'created': 'Sat, 13 Jan 2007 20:50:11 GMT'}]
2007-05-23
[array(['Harrison', 'Earnest', ''], dtype=object)]
3,986
1001.1512
Johannes Messchendorp J.G.
M. Eslami-Kalantari, H.R. Amir-Ahmadi, A. Biegun, I. Ga\v{s}paric, L. Joulaeizadeh, N. Kalantar-Nayestanaki, St. Kistryn, A. Kozela, H. Mardanpour, J.G. Messchendorp, H. Moeini, A. Ramazani-Moghaddam-Arani, S.V. Shende, E. Stephan, R. Sworst
Measurements of scattering observables for the $pd$ break-up reaction
Proceedings of 19th International IUPAP Conference on Few-Body Problems in Physics, Bonn University, 31.08 - 05.09.2009, Bonn, GERMANY
null
10.1051/epjconf/20100305010
null
nucl-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
High-precision measurements of the scattering observables such as cross sections and analyzing powers for the proton-deuteron elastic and break-up reactions have been performed at KVI in the last two decades and elsewhere to investigate various aspects of the three-nucleon force (3NF) effects simultaneously. In 2006 an experiment was performed to study these effects in $\vec{p}+d$ break-up reaction at 135 MeV with the detection system, Big Instrument for Nuclear polarization Analysis, BINA. BINA covers almost the entire kinematical phase space of the break-up reaction. The results are interpreted with the help of state-of-the-art Faddeev calculations and are partly presented in this contribution.
[{'version': 'v1', 'created': 'Sun, 10 Jan 2010 13:15:33 GMT'}]
2015-05-14
[array(['Eslami-Kalantari', 'M.', ''], dtype=object) array(['Amir-Ahmadi', 'H. R.', ''], dtype=object) array(['Biegun', 'A.', ''], dtype=object) array(['Gašparic', 'I.', ''], dtype=object) array(['Joulaeizadeh', 'L.', ''], dtype=object) array(['Kalantar-Nayestanaki', 'N.', ''], dtype=object) array(['Kistryn', 'St.', ''], dtype=object) array(['Kozela', 'A.', ''], dtype=object) array(['Mardanpour', 'H.', ''], dtype=object) array(['Messchendorp', 'J. G.', ''], dtype=object) array(['Moeini', 'H.', ''], dtype=object) array(['Ramazani-Moghaddam-Arani', 'A.', ''], dtype=object) array(['Shende', 'S. V.', ''], dtype=object) array(['Stephan', 'E.', ''], dtype=object) array(['Sworst', 'R.', ''], dtype=object)]
3,987
1603.01421
Gary Froyland
Davor Dragi\v{c}evi\'c and Gary Froyland
H\"older continuity of Oseledets splittings for semi-invertible operator cocycles
Minor revisions to match accepted version in ETDS
null
10.1017/etds.2016.55
null
math.DS
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
For H\"older continuous cocycles over an invertible, Lipschitz base, we establish the H\"older continuity of Oseledets subspaces on compact sets of arbitrarily large measure. This extends a result of Ara\'{u}jo, Bufetov, and Filip by considering possibly noninvertible cocycles, which in addition may take values in the space of compact operators on a Hilbert space. As a by-product of our work, we also show that a noninvertible cocycle with nonvanishing Lyapunov exponents exhibits nonuniformly hyperbolic behaviour (in the sense of Pesin) on a set of full measure.
[{'version': 'v1', 'created': 'Fri, 4 Mar 2016 10:57:34 GMT'} {'version': 'v2', 'created': 'Tue, 12 Jul 2016 15:55:53 GMT'}]
2016-09-14
[array(['Dragičević', 'Davor', ''], dtype=object) array(['Froyland', 'Gary', ''], dtype=object)]
3,988
1810.12143
Z Yan
Guoqiang Zhang and Zhenya Yan
A unified inverse scattering transform and soliton solutions of the nonlocal modified KdV equation with non-zero boundary conditions
21 pages, 4 figures
Physica D 402 (2020) 132170
null
null
nlin.SI math-ph math.AP math.MP nlin.PS physics.comp-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We present a rigorous theory of a unified and simple inverse scattering transform (IST) for both focusing and defocusing real nonlocal (reverse-space-time) modified Korteweg-de Vries (mKdV) equations with non-zero boundary conditions (NZBCs) at infinity. The IST problems for the nonlocal equations with NZBCs are more complicated then ones for the local equations with NZBCs. The suitable uniformization variable is introduced in order to make the direct and inverse problems be established on a complex plane instead of a two-sheeted Riemann surface. The direct scattering problem establishes the analyticity, symmetries, and asymptotic behaviors of Jost solutions and scattering matrix, and properties of discrete spectra. The inverse problem is formulated and solved by means of a matrix-valued Riemann-Hilbert problem. The reconstruction formula, trace formulae, and theta conditions are obtained. Finally, the dynamical behaviors of solitons for four different cases for the reflectionless potentials for both focusing and defocusing nonlocal mKdV equations with NZBCs are analyzed in detail.
[{'version': 'v1', 'created': 'Mon, 29 Oct 2018 14:25:07 GMT'} {'version': 'v2', 'created': 'Thu, 21 Mar 2019 07:13:59 GMT'}]
2020-12-08
[array(['Zhang', 'Guoqiang', ''], dtype=object) array(['Yan', 'Zhenya', ''], dtype=object)]
3,989
quant-ph/0311183
Luis L. Sanchez. Soto
A. B. Klimov, J. L. Romero, J. Delgado and L. L. Sanchez-Soto
Effective damping in the Raman cooling of trapped ions
15 pages, 5 figures. To appear in Optics Communications
Opt. Commun. 230, 393-400 (2004)
10.1016/j.optcom.2003.11.025
null
quant-ph
null
We present a method of treating the interaction of a single three-level ion with two laser beams. The idea is to apply a unitary transformation such that the exact transformed Hamiltonian has one of the three levels decoupled for all values of the detunings. When one takes into account damping, the evolution of the system is governed by a master equation usually obtained via adiabatic approximation under the assumption of far-detuned lasers. To go around the drawbacks of this technique, we use the same unitary transformation to get an effective master equation.
[{'version': 'v1', 'created': 'Wed, 26 Nov 2003 16:13:13 GMT'}]
2007-05-23
[array(['Klimov', 'A. B.', ''], dtype=object) array(['Romero', 'J. L.', ''], dtype=object) array(['Delgado', 'J.', ''], dtype=object) array(['Sanchez-Soto', 'L. L.', ''], dtype=object)]
3,990
1508.06544
Hassan Saadat
H. Saadat
A cosmological model of the early universe based on ECG with variable $\Lambda$-term in Lyra geometry
14 pages, 5 figures. arXiv admin note: text overlap with arXiv:1502.01189, arXiv:1410.5858 by other authors
null
10.1007/s10773-015-2874-x
null
gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we study interacting extended Chaplygin gas as dark matter and quintessence scalar field as dark energy with an effective $\Lambda$-term in Lyra manifold. As we know Chaplygin gas behaves as dark matter at the early universe while cosmological constant at the late time. Modified field equations are given and motivation of the phenomenological models discussed in details. Four different models based on the interaction term are investigated in this work. Then, we consider other models where Extended Chaplygin gas and quintessence field play role of dark matter and dark energy respectively with two different forms of interaction between the extended Chaplygin gas and quintessence scalar field for both constant and varying $\Lambda$. Concerning to the mathematical hardness of the problems we discuss results numerically and graphically. Obtained results give us hope that proposed models can work as good models for the early universe with later stage of evolution containing accelerated expansion.
[{'version': 'v1', 'created': 'Mon, 24 Aug 2015 12:38:32 GMT'}]
2016-01-20
[array(['Saadat', 'H.', ''], dtype=object)]
3,991
1210.5567
Yasuki Tachibana
Yasuki Tachibana, Tetsufumi Hirano
Emission of Low Momentum Particles at Large Angles from Jet
4 pages, 2figures, to appear in the proceedings of Quark Matter 2012, August 13-18, Washington D.C., USA
null
10.1016/j.nuclphysa.2013.02.189
null
nucl-th hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study dynamics of a QGP fluid induced by energetic partons propagating through it. We construct a (3+1)-dimensional QGP-fluid+Jet model. When a jet traverses a uniform fluid, it induces a Mach cone structure of energy density distribution and a vortex ring surrounding a path of the jet. When a pair of jets travels through a radially expanding fluid, low momentum particles are dominantly induced at large angles from the quenched jet. This result is qualitatively consistent with observation of the CMS Collaboration at LHC.
[{'version': 'v1', 'created': 'Sat, 20 Oct 2012 01:10:20 GMT'}]
2015-06-11
[array(['Tachibana', 'Yasuki', ''], dtype=object) array(['Hirano', 'Tetsufumi', ''], dtype=object)]
3,992
1801.03105
Diane Cormier
D. Cormier, F. Bigiel, M. J. Jim\'enez-Donaire, A. K. Leroy, M. Gallagher, A. Usero, K. Sandstrom, A. Bolatto, A. Hughes, C. Kramer, M. R. Krumholz, D. S. Meier, E. J. Murphy, J. Pety, E. Rosolowsky, E. Schinnerer, A. Schruba, K. Sliwa, and F. Walter
Full-disc $^{13}$CO(1-0) mapping across nearby galaxies of the EMPIRE survey and the CO-to-H$_2$ conversion factor
accepted for publication in MNRAS
null
10.1093/mnras/sty059
null
astro-ph.GA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Carbon monoxide (CO) provides crucial information about the molecular gas properties of galaxies. While $^{12}$CO has been targeted extensively, isotopologues such as $^{13}$CO have the advantage of being less optically thick and observations have recently become accessible across full galaxy discs. We present a comprehensive new dataset of $^{13}$CO(1-0) observations with the IRAM 30-m telescope of the full discs of 9 nearby spiral galaxies from the EMPIRE survey at a spatial resolution of $\sim$1.5kpc. $^{13}$CO(1-0) is mapped out to $0.7-1r_{25}$ and detected at high signal-to-noise throughout our maps. We analyse the $^{12}$CO(1-0)-to-$^{13}$CO(1-0) ratio ($\Re$) as a function of galactocentric radius and other parameters such as the $^{12}$CO(2-1)-to-$^{12}$CO(1-0) intensity ratio, the 70-to-160$\mu$m flux density ratio, the star-formation rate surface density, the star-formation efficiency, and the CO-to-H$_2$ conversion factor. We find that $\Re$ varies by a factor of 2 at most within and amongst galaxies, with a median value of 11 and larger variations in the galaxy centres than in the discs. We argue that optical depth effects, most likely due to changes in the mixture of diffuse/dense gas, are favored explanations for the observed $\Re$ variations, while abundance changes may also be at play. We calculate a spatially-resolved $^{13}$CO(1-0)-to-H$_2$ conversion factor and find an average value of $1.0\times10^{21}$ cm$^{-2}$ (K.km/s)$^{-1}$ over our sample with a standard deviation of a factor of 2. We find that $^{13}$CO(1-0) does not appear to be a good predictor of the bulk molecular gas mass in normal galaxy discs due to the presence of a large diffuse phase, but it may be a better tracer of the mass than $^{12}$CO(1-0) in the galaxy centres where the fraction of dense gas is larger.
[{'version': 'v1', 'created': 'Tue, 9 Jan 2018 19:01:01 GMT'}]
2018-01-24
[array(['Cormier', 'D.', ''], dtype=object) array(['Bigiel', 'F.', ''], dtype=object) array(['Jiménez-Donaire', 'M. J.', ''], dtype=object) array(['Leroy', 'A. K.', ''], dtype=object) array(['Gallagher', 'M.', ''], dtype=object) array(['Usero', 'A.', ''], dtype=object) array(['Sandstrom', 'K.', ''], dtype=object) array(['Bolatto', 'A.', ''], dtype=object) array(['Hughes', 'A.', ''], dtype=object) array(['Kramer', 'C.', ''], dtype=object) array(['Krumholz', 'M. R.', ''], dtype=object) array(['Meier', 'D. S.', ''], dtype=object) array(['Murphy', 'E. J.', ''], dtype=object) array(['Pety', 'J.', ''], dtype=object) array(['Rosolowsky', 'E.', ''], dtype=object) array(['Schinnerer', 'E.', ''], dtype=object) array(['Schruba', 'A.', ''], dtype=object) array(['Sliwa', 'K.', ''], dtype=object) array(['Walter', 'F.', ''], dtype=object)]
3,993
1612.07491
Irit Dinur
Amey Bhangale, Irit Dinur, Inbal Livni Navon
Cube vs. Cube Low Degree Test
null
null
null
null
cs.CC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We revisit the Raz-Safra plane-vs.-plane test and study the closely related cube vs. cube test. In this test the tester has access to a "cubes table" which assigns to every cube a low degree polynomial. The tester randomly selects two cubes (affine sub-spaces of dimension $3$) that intersect on a point $x\in \mathbf{F}^m$, and checks that the assignments to the cubes agree with each other on the point $x$. Our main result is a new combinatorial proof for a low degree test that comes closer to the soundness limit, as it works for all $\epsilon \ge poly(d)/{\mathbf{F}}^{1/2}$, where $d$ is the degree. This should be compared to the previously best soundness value of $\epsilon \ge poly(m, d)/\mathbf{F}^{1/8}$. Our soundness limit improves upon the dependence on the field size and does not depend on the dimension of the ambient space. Our proof is combinatorial and direct: unlike the Raz-Safra proof, it proceeds in one shot and does not require induction on the dimension of the ambient space. The ideas in our proof come from works on direct product testing which are even simpler in the current setting thanks to the low degree. Along the way we also prove a somewhat surprising fact about connection between different agreement tests: it does not matter if the tester chooses the cubes to intersect on points or on lines: for every given table, its success probability in either test is nearly the same.
[{'version': 'v1', 'created': 'Thu, 22 Dec 2016 08:54:49 GMT'}]
2016-12-23
[array(['Bhangale', 'Amey', ''], dtype=object) array(['Dinur', 'Irit', ''], dtype=object) array(['Navon', 'Inbal Livni', ''], dtype=object)]
3,994
hep-ph/0509138
Gregory Soyez
G. Soyez
Fluctuation effects in high-energy QCD
4 pages, 4 figures. Talk presented at the XIth International Conference on Elastic and Diffractive Scattering (EDS05), Blois, France, May 15-20 2005
null
null
null
hep-ph
null
The recent high-energy QCD equations including the effects of fluctuations are solved numerically. We discuss their asymptotic properties and compare them with the corresponding behaviour without fluctuations as well as with the statistical-physics model obtained in the saddle point approximation. The potential consequences on phenomenology, particularly on geometric scaling violations, are drawn.
[{'version': 'v1', 'created': 'Wed, 14 Sep 2005 00:33:46 GMT'}]
2007-05-23
[array(['Soyez', 'G.', ''], dtype=object)]
3,995
2005.10734
Mohammed Belkhatir
Noureddine Belkhatir, Jacky Estublier, Walcelio Melo
THE ADELE-TEMPO experience : an environment to support process modeling and enaction
null
null
null
null
cs.SE
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Process-Centered Software Engineering Environments (PSEE) have recently attracted a large number of researchers. In such environments the software processes are explicitly described and interpreted by the PSEE, allowing software activities to be automated, assisted, and enforced. Lehman and Belady (1985) & Osterweil (1987) claim that this capability is a central element in a software development environment for the improvement of software product quality and software developers productivity. We have addressed these problems in the framework of the Adele project. The Adele kernel, initially a configuration management system has been extended with respect to 1) modeling and support of complex product models: the Object Manager 2) modeling and support of software processes: the Activity Manager and 3) modeling and support of software product evolution: the Configuration Manager. For data and product modelling, an ER/OO model has been implemented including SEE specific features; On top of Adele kernel, which is a commercial product, we developed a Process Manager research prototype, Tempo, an enactable formalism based on two major concepts: objects may have a different description (role) depending on the process in which they are used, and processes are synchronized and coordinated by explicit connections. ADL-Tempo is organized around the concepts of software product, Work Environment and software process.
[{'version': 'v1', 'created': 'Thu, 21 May 2020 15:43:42 GMT'}]
2020-05-22
[array(['Belkhatir', 'Noureddine', ''], dtype=object) array(['Estublier', 'Jacky', ''], dtype=object) array(['Melo', 'Walcelio', ''], dtype=object)]
3,996
2102.07892
Arash Ghaani Farashahi
Arash Ghaani Farashahi
Covariant Functions of Characters of Compact Subgroups
null
null
null
null
math.FA
http://creativecommons.org/licenses/by/4.0/
This paper presents a systematic study for abstract harmonic analysis on classical Banach spaces of covariant functions of characters of compact subgroups. Let $G$ be a locally compact group and $H$ be a compact subgroup of $G$. Suppose that $\xi:H\to\mathbb{T}$ is a continuous character, $1\le p<\infty$ and $L_\xi^p(G,H)$ is the set of all covariant functions of $\xi$ in $L^p(G)$. It is shown that $L^p_\xi(G,H)$ is isometrically isomorphic to a quotient space of $L^p(G)$. It is also proven that $L^q_\xi(G,H)$ is isometrically isomorphic to the dual space $L^p_\xi(G,H)^*$, where $q$ is the conjugate exponent of $p$. The paper is concluded by some results for the case that $G$ is compact.
[{'version': 'v1', 'created': 'Mon, 15 Feb 2021 23:15:48 GMT'}]
2021-02-17
[array(['Farashahi', 'Arash Ghaani', ''], dtype=object)]
3,997
1405.2596
Mohammad Soltani
Mohammad Soltani, Pavol Bokes, Zachary Fox, Abhyudai Singh
Nonspecific transcription factor binding reduces variability in transcription factor and target protein expression
10 pages, 5 figures, Physical Biology
null
null
null
q-bio.SC q-bio.MN
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Transcription factors (TFs) interact with a multitude of binding sites on DNA and partner proteins inside cells. We investigate how nonspecific binding/unbinding to such decoy binding sites affects the magnitude and time-scale of random fluctuations in TF copy numbers arising from stochastic gene expression. A stochastic model of TF gene expression, together with decoy site interactions is formulated. Distributions for the total (bound and unbound) and free (unbound) TF levels are derived by analytically solving the chemical master equation under physiologically relevant assumptions. Our results show that increasing the number of decoy binding sides considerably reduces stochasticity in free TF copy numbers. The TF autocorrelation function reveals that decoy sites can either enhance or shorten the time-scale of TF fluctuations depending on model parameters. To understand how noise in TF abundances propagates downstream, a TF target gene is included in the model. Intriguingly, we find that noise in the expression of the target gene decreases with increasing decoy sites for linear TF-target protein dose-responses, even in regimes where decoy sites enhance TF autocorrelation times. Moreover, counterintuitive noise transmissions arise for nonlinear dose-responses. In summary, our study highlights the critical role of molecular sequestration by decoy binding sites in regulating the stochastic dynamics of TFs and target proteins at the single-cell level.
[{'version': 'v1', 'created': 'Sun, 11 May 2014 22:48:34 GMT'} {'version': 'v2', 'created': 'Tue, 14 Apr 2015 19:07:27 GMT'}]
2015-04-15
[array(['Soltani', 'Mohammad', ''], dtype=object) array(['Bokes', 'Pavol', ''], dtype=object) array(['Fox', 'Zachary', ''], dtype=object) array(['Singh', 'Abhyudai', ''], dtype=object)]
3,998
1403.5245
Alexander Kemper
A.F. Kemper, M.A. Sentef, B. Moritz, J.K. Freericks and T.P. Devereaux
Effect of dynamical spectral weight redistribution on effective interactions in time-resolved spectroscopy
5 pages, 4 figures. SI contained in sources
Phys. Rev. B 90, 075126 (2014)
10.1103/PhysRevB.90.075126
null
cond-mat.mes-hall cond-mat.mtrl-sci
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The redistribution of electrons in an ultrafast pump-probe experiment causes significant changes to the effective interaction between electrons and bosonic modes. We study the influence of these changes on pump-probe photoemission spectroscopy for a model electron-phonon coupled system using the nonequilibrium Keldysh formalism. We show that spectral rearrangement due to the driving field preserves an overall sum rule for the electronic self-energy, but modifies the effective electron-phonon scattering as a function of energy. Experimentally, this pump-modified scattering can be tracked by analyzing the fluence or excitation energy dependence of population decay rates and transient changes in dispersion kinks.
[{'version': 'v1', 'created': 'Thu, 20 Mar 2014 19:37:35 GMT'} {'version': 'v2', 'created': 'Fri, 21 Mar 2014 18:53:42 GMT'} {'version': 'v3', 'created': 'Thu, 21 Aug 2014 21:11:39 GMT'}]
2014-08-25
[array(['Kemper', 'A. F.', ''], dtype=object) array(['Sentef', 'M. A.', ''], dtype=object) array(['Moritz', 'B.', ''], dtype=object) array(['Freericks', 'J. K.', ''], dtype=object) array(['Devereaux', 'T. P.', ''], dtype=object)]
3,999
gr-qc/0508100
Daniel Sudarsky
Alejandro Perez, Hanno Sahlmann, and Daniel Sudarsky
On the quantum origin of the seeds of cosmic structure
replacement with final version to appear in Classical and Quantum Gravity
Class.Quant.Grav. 23 (2006) 2317-2354
10.1088/0264-9381/23/7/008
null
gr-qc astro-ph hep-th quant-ph
null
The current understanding of the quantum origin of cosmic structure is discussed critically. We point out that in the existing treatments a transition from a symmetric quantum state to an (essentially classical) non-symmetric state is implicitly assumed, but not specified or analyzed in any detail. In facing the issue we are led to conclude that new physics is required to explain the apparent predictive power of the usual schemes. Furthermore we show that the novel way of looking at the relevant issues opens new windows from where relevant information might be extracted regarding cosmological issues and perhaps even clues about aspects of quantum gravity.
[{'version': 'v1', 'created': 'Wed, 24 Aug 2005 13:54:34 GMT'} {'version': 'v2', 'created': 'Thu, 25 Aug 2005 00:15:43 GMT'} {'version': 'v3', 'created': 'Sat, 25 Feb 2006 19:55:57 GMT'}]
2015-06-25
[array(['Perez', 'Alejandro', ''], dtype=object) array(['Sahlmann', 'Hanno', ''], dtype=object) array(['Sudarsky', 'Daniel', ''], dtype=object)]