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math/9903196
Kannan Soundararajan
Andrew Granville (University of Georgia), K. Soundararajan (AIM and Princeton University)
Large character sums
Abstract added in migration.
null
null
AIM 1999-5
math.NT
null
Assuming the Generalized Riemann Hypothesis, the authors study when a character sum over all n <= x is o(x); they show that this holds if log x / log log q -> infinity and q -> infinity (q is the size of the finite field).
[{'version': 'v1', 'created': 'Tue, 23 Mar 1999 00:00:00 GMT'}]
2016-09-07
[array(['Granville', 'Andrew', '', 'University of Georgia'], dtype=object) array(['Soundararajan', 'K.', '', 'AIM and\n Princeton University'], dtype=object) ]
1,001
1906.07339
Shubhendra Singhal Mr.
Shubhendra Pal Singhal
Reputation Systems -- Fair allocation of points to the editors in the collaborative community
6 pages, 2 figures
International Research Journal of Engineering and Technology (IRJET) (2019), e-ISSN: 2395-0056, p-ISSN: 2395-0072, June 2019, "https://www.irjet.net/archives/V6/i6/IRJET-V6I6482.pdf"
null
Volume: 06 Issue: 06, June 2019, Page number(2259-2263)
cs.SE cs.SI
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper we are trying to determine a scheme for the fair allocation of points to the contributors of the collaborative community. The major problem of fair allocation of points among the contributors is that we have to analyze the improvement in the versions of an article. Lets say there is a contribution of major change in content which is relevant vs the contribution of adding a single comma. Every contributor cannot be given the same points in such a case. There are many ways which can be used like number of changes in a new version. That might seem relevant but it becomes irrelevant in terms of correct content contribution and other significant changes. There is no AI system too which can detect such a change and award the points accordingly. So this problem of allocation of points to the contributors is presented by an algorithm with a theoretical proof. It relies on the interactive interaction of the users in the system which is trivial in case of big system design economies.
[{'version': 'v1', 'created': 'Tue, 18 Jun 2019 02:01:46 GMT'} {'version': 'v2', 'created': 'Fri, 28 Jun 2019 21:55:24 GMT'}]
2019-07-02
[array(['Singhal', 'Shubhendra Pal', ''], dtype=object)]
1,002
1812.10885
Longlong Jing
Longlong Jing, Yucheng Chen, Yingli Tian
Coarse-to-fine Semantic Segmentation from Image-level Labels
null
null
null
null
cs.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Deep neural network-based semantic segmentation generally requires large-scale cost extensive annotations for training to obtain better performance. To avoid pixel-wise segmentation annotations which are needed for most methods, recently some researchers attempted to use object-level labels (e.g. bounding boxes) or image-level labels (e.g. image categories). In this paper, we propose a novel recursive coarse-to-fine semantic segmentation framework based on only image-level category labels. For each image, an initial coarse mask is first generated by a convolutional neural network-based unsupervised foreground segmentation model and then is enhanced by a graph model. The enhanced coarse mask is fed to a fully convolutional neural network to be recursively refined. Unlike existing image-level label-based semantic segmentation methods which require to label all categories for images contain multiple types of objects, our framework only needs one label for each image and can handle images contains multi-category objects. With only trained on ImageNet, our framework achieves comparable performance on PASCAL VOC dataset as other image-level label-based state-of-the-arts of semantic segmentation. Furthermore, our framework can be easily extended to foreground object segmentation task and achieves comparable performance with the state-of-the-art supervised methods on the Internet Object dataset.
[{'version': 'v1', 'created': 'Fri, 28 Dec 2018 04:04:06 GMT'}]
2018-12-31
[array(['Jing', 'Longlong', ''], dtype=object) array(['Chen', 'Yucheng', ''], dtype=object) array(['Tian', 'Yingli', ''], dtype=object)]
1,003
1409.0102
Olav Kristian Nygaard
Olav Nygaard
Uniform boundedness deciding sets, and a problem of M. Valdivia
The paper is withdrawn because there is a serious gap that I haven't been able to fill
null
null
null
math.FA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We prove that if a set $B$ in a Banach space $X$ can be written as an increasing, countable union $B=\cup_n B_n$ of sets $B_n$ such that no $B_n$ is uniform boundedness deciding, then also $B$ is not uniform boundedness deciding. From this we can give a positive answer to a question of M. Valdivia.
[{'version': 'v1', 'created': 'Sat, 30 Aug 2014 11:09:15 GMT'} {'version': 'v2', 'created': 'Sun, 19 Jul 2015 15:20:43 GMT'}]
2015-07-21
[array(['Nygaard', 'Olav', ''], dtype=object)]
1,004
0911.5516
Hume A. Feldman
Hume A. Feldman (Kansas), Richard Watkins (Willamette) and Michael J. Hudson (Waterloo)
Cosmic Flows on 100 Mpc/h Scales: Standardized Minimum Variance Bulk Flow, Shear and Octupole Moments
13 Pages, 7 figures, 4 tables. Some changes to reflect the published version
Mon.Not.Roy.Astron.Soc.407:2328-2338,2010
10.1111/j.1365-2966.2010.17052.x
null
astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The low order moments, such as the bulk flow and shear, of the large scale peculiar velocity field are sensitive probes of the matter density fluctuations on very large scales. In practice, however, peculiar velocity surveys are usually sparse and noisy, which can lead to the aliasing of small scale power into what is meant to be a probe of the largest scales. Previously, we developed an optimal ``minimum variance'' (MV) weighting scheme, designed to overcome this problem by minimizing the difference between the measured bulk flow (BF) and that which would be measured by an ideal survey. Here we extend this MV analysis to include the shear and octupole moments, which are designed to have almost no correlations between them so that they are virtually orthogonal. We apply this MV analysis to a compilation of all major peculiar velocity surveys, consisting of 4536 measurements. Our estimate of the BF on scales of ~ 100 Mpc/h has a magnitude of |v|= 416 +/- 78 km/s towards Galactic l = 282 degree +/- 11 degree and b = 6 degree +/- 6 degree. This result is in disagreement with LCDM with WMAP5 cosmological parameters at a high confidence level, but is in good agreement with our previous MV result without an orthogonality constraint, showing that the shear and octupole moments did not contaminate the previous BF measurement. The shear and octupole moments are consistent with WMAP5 power spectrum, although the measurement noise is larger for these moments than for the BF. The relatively low shear moments suggest that the sources responsible for the BF are at large distances.
[{'version': 'v1', 'created': 'Sun, 29 Nov 2009 21:13:58 GMT'} {'version': 'v2', 'created': 'Fri, 25 Jun 2010 21:00:34 GMT'}]
2011-02-15
[array(['Feldman', 'Hume A.', '', 'Kansas'], dtype=object) array(['Watkins', 'Richard', '', 'Willamette'], dtype=object) array(['Hudson', 'Michael J.', '', 'Waterloo'], dtype=object)]
1,005
1403.7684
Nikolaos Mavromatos
Nick E. Mavromatos
Pseudoscalar Fields in Torsionful Geometries of the Early Universe, the Baryon Asymmetry and Majorana Neutrino Mass Generation
14 pages bibtex, one eps figure incorporated, uses special macros; Invited plenary talk at XIV Mexican Workshop on Particles and Fields, November 25-29 2013, Oaxaca (Mexico)
null
null
LCTS/2014-03, KCL-PH-TH/2014-03
hep-ph gr-qc hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We discuss here a specific field-theory model, inspired from string theory, in which the generation of a matter-antimatter asymmetry in the Cosmos is due to the propagation of fermions in a non-trivial, spherically asymmetric (and hence Lorentz violating) gravitational background that may characterise the epochs of the early universe. The background induces different dispersion relations, hence populations, between fermions and antifermions, and thus CPT Violation (CPTV) already in thermal equilibrium. Species populations may freeze out leading to leptogenesis and baryogenesis. More specifically, after reviewing some generic models of background-induced CPTV in early epochs of the Universe, we consider a string-inspired scenario, in which the CPTV is associated with a cosmological background with torsion provided by the Kalb-Ramond (KR) antisymemtric tensor field of the string gravitational multiplet. In a four-dimensional space time this field is dual to a pseudoscalar ``axion-like'' field. The thermalising processes in this model are (right-handed) Majorana neutrino-antineutrino oscillations, which are induced in the presence of the KR axion background. These processes freeze out at a (high) temperature $T_c >> m$, where $m$ is the Majorana neutrino mass, at which the KR background goes to zero or is diminished significantly, through appropriate phase transitions of the (string) universe. An additional, but equally important, r\^ole, of the KR field is that its quantum fluctuations and mixing with an ordinary axion, which couples to the Majorana neutrinos via appropriate Yukawa couplings, can also lead to the generation of a Majorana neutrino mass through quantum anomalies. This provides a novel way for generating neutrino masses, independent of the traditional seesaw mechanism.
[{'version': 'v1', 'created': 'Sun, 30 Mar 2014 00:38:28 GMT'}]
2014-04-01
[array(['Mavromatos', 'Nick E.', ''], dtype=object)]
1,006
1210.2449
EPTCS
Chung-Hao Huang (National Taiwan University), Doron Peled (Bar Ilan University), Sven Schewe (University of Liverpool), Farn Wang (National Taiwan University)
Rapid Recovery for Systems with Scarce Faults
In Proceedings GandALF 2012, arXiv:1210.2028
EPTCS 96, 2012, pp. 15-28
10.4204/EPTCS.96.2
null
cs.SY
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Our goal is to achieve a high degree of fault tolerance through the control of a safety critical systems. This reduces to solving a game between a malicious environment that injects failures and a controller who tries to establish a correct behavior. We suggest a new control objective for such systems that offers a better balance between complexity and precision: we seek systems that are k-resilient. In order to be k-resilient, a system needs to be able to rapidly recover from a small number, up to k, of local faults infinitely many times, provided that blocks of up to k faults are separated by short recovery periods in which no fault occurs. k-resilience is a simple but powerful abstraction from the precise distribution of local faults, but much more refined than the traditional objective to maximize the number of local faults. We argue why we believe this to be the right level of abstraction for safety critical systems when local faults are few and far between. We show that the computational complexity of constructing optimal control with respect to resilience is low and demonstrate the feasibility through an implementation and experimental results.
[{'version': 'v1', 'created': 'Tue, 9 Oct 2012 00:53:01 GMT'}]
2012-10-10
[array(['Huang', 'Chung-Hao', '', 'National Taiwan University'], dtype=object) array(['Peled', 'Doron', '', 'Bar Ilan\n University'], dtype=object) array(['Schewe', 'Sven', '', 'University of Liverpool'], dtype=object) array(['Wang', 'Farn', '', 'National\n Taiwan University'], dtype=object)]
1,007
0911.2613
Anders Basboll
Anders Basboll
SUSY Flat Directions -- to get a VEV or not?
Comments: 10 pages. To appear in the Proceedings from Invisible Universe International Conference (Paris 2009). AIP Conference Proceedings
AIP Conf.Proc.1241:477-486,2010
10.1063/1.3462674
null
hep-ph astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the potential of SUSY flat directions (FDs). Large FD vacuum expectation values (VEVs) can delay thermalisation and solve the gravitino problem - if FDs decay perturbatively. This depends on how many and which directions get the VEVs. Recently the decay of the FDs have been studied with the VEVs as input. Here we look at how the VEVs come about -- statistically and analytically.
[{'version': 'v1', 'created': 'Fri, 13 Nov 2009 13:54:32 GMT'}]
2014-11-20
[array(['Basboll', 'Anders', ''], dtype=object)]
1,008
1303.4348
Benjamin Recht
Gongguo Tang and Badri Narayan Bhaskar and Benjamin Recht
Near Minimax Line Spectral Estimation
25 pages, 12 figures. Added a numerical experiments section
null
null
null
cs.IT math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This paper establishes a nearly optimal algorithm for estimating the frequencies and amplitudes of a mixture of sinusoids from noisy equispaced samples. We derive our algorithm by viewing line spectral estimation as a sparse recovery problem with a continuous, infinite dictionary. We show how to compute the estimator via semidefinite programming and provide guarantees on its mean-square error rate. We derive a complementary minimax lower bound on this estimation rate, demonstrating that our approach nearly achieves the best possible estimation error. Furthermore, we establish bounds on how well our estimator localizes the frequencies in the signal, showing that the localization error tends to zero as the number of samples grows. We verify our theoretical results in an array of numerical experiments, demonstrating that the semidefinite programming approach outperforms two classical spectral estimation techniques.
[{'version': 'v1', 'created': 'Mon, 18 Mar 2013 18:19:38 GMT'} {'version': 'v2', 'created': 'Mon, 1 Apr 2013 16:07:02 GMT'}]
2013-04-02
[array(['Tang', 'Gongguo', ''], dtype=object) array(['Bhaskar', 'Badri Narayan', ''], dtype=object) array(['Recht', 'Benjamin', ''], dtype=object)]
1,009
astro-ph/0103499
Christian Hettlage
Christian Hettlage and Karl Mannheim
High Energy Neutrino Fluxes from Cosmic Accelerators
4 pages, 2 figures, to appear in the Proceedings of the XXIst Moriond Workshop 'Very High Energy Phenomena in the Universe', Les Arcs, France, January 20-27 2001
null
null
null
astro-ph hep-ph
null
We constrain high-energy neutrino fluxes with the observed cosmic ray and gamma ray fluxes, include flavor oscillations and propagation through Earth, and show that blazars could possibly be detected by cubic-kilometer neutrino telescopes.
[{'version': 'v1', 'created': 'Thu, 29 Mar 2001 16:54:36 GMT'}]
2007-05-23
[array(['Hettlage', 'Christian', ''], dtype=object) array(['Mannheim', 'Karl', ''], dtype=object)]
1,010
1903.04554
Ali Rahmati
Ali Rahmati, Seyyedali Hosseinalipour, Huaiyu Dai
Optimal Time Allocation in VANETs Advertising: A Price-based Approach using Stackelberg Game
6 pages, 4 figures
null
null
null
cs.GT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Vehicular ad-hoc networks (VANETs) have recently attracted a lot of attention due to their immense potentials and applications. Wide range of coverage and accessibility to end users make VANETs a good target for commercial companies. In this paper, we consider a scenario in which advertising companies aim to disseminate their advertisements in different areas of a city by utilizing VANETs infrastructure. These companies compete for renting the VANETs infrastructure to spread their advertisements. We partition the city map into different blocks, and consider a manager for all the blocks who is in charge of splitting the time between interested advertising companies. Each advertising company (AdC) is charged proportional to the allocated time. In order to find the best time splitting between AdCs, we propose a Stackelberg game scheme in which the block manager assigns the companies to the blocks and imposes the renting prices to different companies in order to maximize its own profit. Based on this, AdCs request the amount of time they desire to rent the infrastructure in order to maximize their utilities. To obtain the Stackelberg equilibrium of the game, a mixed integer nonlinear optimization problem is solved using the proposed optimal and sub-optimal algorithms. The simulation results demonstrate that the sub-optimal algorithm approaches the optimal one in performance with lower complexity.
[{'version': 'v1', 'created': 'Mon, 11 Mar 2019 19:21:54 GMT'}]
2019-03-13
[array(['Rahmati', 'Ali', ''], dtype=object) array(['Hosseinalipour', 'Seyyedali', ''], dtype=object) array(['Dai', 'Huaiyu', ''], dtype=object)]
1,011
2301.03059
Alessandro Siciliano
Giusy Monzillo, Tim Penttila, Alessandro Siciliano
Eggs in finite projective spaces and unitals in translation planes
null
null
null
null
math.CO
http://creativecommons.org/licenses/by/4.0/
Inspired by the connection between ovoids and unitals arising from the Buekenhout construction in the Andr\'e/Bruck-Bose representation of translation planes of dimension at most two over their kernel, and since eggs of PG(4m-1,q), m>=1, are a generalization of ovoids, we explore the relation between eggs and unitals in translation planes of higher dimension over their kernel. By investigating such a relationship, we construct a unital in the Dickson semifield plane of order 3^{10}, which is represented in PG(20,3) by a cone whose base is a set of points constructed from the dual of the Penttila-Williams egg in PG(19,3). This unital is not polar; so, up to the knowledge of the authors, it seems to be a new unital in such a plane.
[{'version': 'v1', 'created': 'Sun, 8 Jan 2023 15:15:59 GMT'}]
2023-01-10
[array(['Monzillo', 'Giusy', ''], dtype=object) array(['Penttila', 'Tim', ''], dtype=object) array(['Siciliano', 'Alessandro', ''], dtype=object)]
1,012
2008.07756
Ying Sui
Ying Sui, Huimin Yu
Singularity formation for compressible Euler equations with time-dependent damping
19 pages
null
null
null
math.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we consider the compressible Euler equations with time-dependent damping \frac{\a}{(1+t)^\lambda}u in one space dimension. By constructing 'decoupled' Riccati type equations for smooth solutions, we provide some sufficient conditions under which the classical solutions must break down in finite time. As a byproduct, we show that the derivatives blow up, somewhat like the formation of shock wave, if the derivatives of initial data are appropriately large at a point even when the damping coefficient goes to infinity with a algebraic growth rate. We study the case \lambda\neq1 and \lambda=1 respectively, moreover, our results have no restrictions on the size of solutions and the positivity/monotonicity of the initial Riemann invariants. In addition, for 1<\gamma<3 we provide time-dependent lower bounds on density for arbitrary classical solutions, without any additional assumptions on the initial data.
[{'version': 'v1', 'created': 'Tue, 18 Aug 2020 06:16:28 GMT'}]
2020-08-19
[array(['Sui', 'Ying', ''], dtype=object) array(['Yu', 'Huimin', ''], dtype=object)]
1,013
2208.12347
Eugenio Moggi
Amin Farjudian, Eugenio Moggi
Robustness, Scott Continuity, and Computability
26 pages
null
null
null
cs.LO
http://creativecommons.org/licenses/by-nc-nd/4.0/
Robustness is a property of system analyses, namely monotonic maps from the complete lattice of subsets of a (system's state) space to the two-point lattice. The definition of robustness requires the space to be a metric space. Robust analyses cannot discriminate between a subset of the metric space and its closure, therefore one can restrict to the complete lattice of closed subsets. When the metric space is compact, the complete lattice of closed subsets ordered by reverse inclusion is w-continuous and robust analyses are exactly the Scott continuous maps. Thus, one can also ask whether a robust analysis is computable (with respect to a countable base). The main result of this paper establishes a relation between robustness and Scott continuity, when the metric space is not compact. The key idea is to replace the metric space with a compact Hausdorff space, and relate robustness and Scott continuity by an adjunction between the complete lattice of closed subsets of the metric space and the w-continuous lattice of closed subsets of the compact Hausdorff space. We demonstrate the applicability of this result with several examples involving Banach spaces.
[{'version': 'v1', 'created': 'Thu, 25 Aug 2022 21:14:59 GMT'}]
2022-08-29
[array(['Farjudian', 'Amin', ''], dtype=object) array(['Moggi', 'Eugenio', ''], dtype=object)]
1,014
1003.0328
Roland Gillen Mr
Roland Gillen, Marcel Mohr, Janina Maultzsch
Symmetry properties of vibrational modes in graphene nanoribbons
10 pages, 5 figures
Phys. Rev. B 81, 205426 (2010)
10.1103/PhysRevB.81.205426
null
cond-mat.mes-hall
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We present symmetry properties of the lattice vibrations of graphene nanoribbons with pure armchair (AGNR) and zigzag edges (ZGNR). In non-symmorphic nanoribbons the phonon modes at the edge of the Brillouin zone are twofold degenerate, whereas the phonon modes in symmorphic nanoribbons are non-degenerate. We identified the Raman-active and infrared-active modes. We predict 3N and 3(N+1) Raman-active modes for N-ZGNRs and N-AGNRs, respectively (N is the number of dimers per unit cell). These modes can be used for the experimental characterization of graphene nanoribbons. Calculations based on density functional theory suggest that the frequency splitting of the LO and TO in AGNRs (corresponding to the E2g mode in graphene) exhibits characteristic width and family dependence. Further, all graphene nanoribbons have a Raman-active breathing-like mode, the frequency of which is inversely proportional to the nanoribbon width and thus might be used for experimental determination of the width of graphene nanoribbons.
[{'version': 'v1', 'created': 'Mon, 1 Mar 2010 16:18:31 GMT'}]
2015-05-18
[array(['Gillen', 'Roland', ''], dtype=object) array(['Mohr', 'Marcel', ''], dtype=object) array(['Maultzsch', 'Janina', ''], dtype=object)]
1,015
1905.04064
Ermin Sakic
Ermin Sakic, Nemanja Deric, Endri Goshi, Wolfgang Kellerer
P4BFT: Hardware-Accelerated Byzantine-Resilient Network Control Plane
Accepted for publication at IEEE Globecom 2019 CQRM
null
null
null
cs.NI cs.DC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Byzantine Fault Tolerance (BFT) enables correct operation of distributed, i.e., replicated applications in the face of malicious take-over and faulty/buggy individual instances. Recently, BFT designs have gained traction in the context of Software Defined Networking (SDN). In SDN, controller replicas are distributed and their state replicated for high availability purposes. Malicious controller replicas, however, may destabilize the control plane and manipulate the data plane, thus motivating the BFT requirement. Nonetheless, deploying BFT in practice comes at a disadvantage of increased traffic load stemming from replicated controllers, as well as a requirement for proprietary switch functionalities, thus putting strain on switches' control plane where particular BFT actions must be executed in software. P4BFT leverages an optimal strategy to decrease the total amount of messages transmitted to switches that are the configuration targets of SDN controllers. It does so by means of message comparison and deduction of correct messages in the determined optimal locations in the data plane. In terms of the incurred control plane load, our P4-based data plane extensions outperform the existing solutions by ~33.2% and ~40.2% on average, in random 128-switch and Fat-Tree/Internet2 topologies, respectively. To validate the correctness and performance gains of P4BFT, we deploy bmv2 and Netronome Agilio SmartNIC-based topologies. The advantages of P4BFT can thus be reproduced both with software switches and "commodity" P4-enabled hardware. A hardware-accelerated controller packet comparison procedure results in an average 96.4% decrease in processing delay per request compared to existing software approaches.
[{'version': 'v1', 'created': 'Fri, 10 May 2019 10:46:28 GMT'} {'version': 'v2', 'created': 'Wed, 14 Aug 2019 09:36:55 GMT'}]
2019-08-15
[array(['Sakic', 'Ermin', ''], dtype=object) array(['Deric', 'Nemanja', ''], dtype=object) array(['Goshi', 'Endri', ''], dtype=object) array(['Kellerer', 'Wolfgang', ''], dtype=object)]
1,016
1406.6650
Cristina Costantini
Cristina Costantini and Thomas G. Kurtz
Viscosity methods giving uniqueness for martingale problems
null
Electronic Journal of Probability (2015) Volume 20, Number 67, Pages 1-27
10.1214/EJP.v20-3624
null
math.PR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Let $E$ be a complete, separable metric space and $A$ be an operator on $C_b(E)$. We give an abstract definition of viscosity sub/supersolution of the resolvent equation $\lambda u-Au=h$ and show that, if the comparison principle holds, then the martingale problem for $A$ has a unique solution. Our proofs work also under two alternative definitions of viscosity sub/supersolution which might be useful, in particular, in infinite dimensional spaces, for instance to study measure-valued processes. We prove the analogous result for stochastic processes that must satisfy boundary conditions, modeled as solutions of constrained martingale problems. In the case of reflecting diffusions in $D\subset {\bf R}^d$, our assumptions allow $ D$ to be nonsmooth and the direction of reflection to be degenerate. Two examples are presented: A diffusion with degenerate oblique direction of reflection and a class of jump diffusion processes with infinite variation jump component and possibly degenerate diffusion matrix.
[{'version': 'v1', 'created': 'Wed, 25 Jun 2014 17:39:32 GMT'} {'version': 'v2', 'created': 'Wed, 18 Nov 2015 12:59:10 GMT'}]
2015-11-19
[array(['Costantini', 'Cristina', ''], dtype=object) array(['Kurtz', 'Thomas G.', ''], dtype=object)]
1,017
1910.05583
Marcel Ausloos
Olgica Nedic, Ivana Drvenica, Marcel Ausloos, and Aleksandar Dekanski
Efficiency in managing peer-review of scientific manuscripts -- editors' perspective
28 refs. ; 4 Tables; 5 figures; 21 pages
Journal of Serbian Chemical Society 83(12), 1391-1405 (2018)
10.2298/JSC180531066N
null
cs.DL cs.DS physics.soc-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The purpose of this paper is to introduce a model for measuring the efficiency in managing peer-review of scientific manuscripts by editors. The approach employed is based on the assumption that the editorial aim is to manage publication with high efficiency, employing the least amount of editorial resources. Efficiency is defined in this research as a measure based on 7 variables. An on-line survey was constructed and editors of journals originating from Serbia regularly publishing articles in the field of chemistry were invited to participate. An evaluation of the model is given based on responses from 24 journals and 50 editors. With this investigation we aimed to contribute to our understanding of the peer-review process and, possibly, offer a tool to improve the "efficiency" in journal editing. The proposed protocol may be adapted by other journals in order to assess the managing potential of editors.
[{'version': 'v1', 'created': 'Sat, 12 Oct 2019 15:54:46 GMT'}]
2019-10-15
[array(['Nedic', 'Olgica', ''], dtype=object) array(['Drvenica', 'Ivana', ''], dtype=object) array(['Ausloos', 'Marcel', ''], dtype=object) array(['Dekanski', 'Aleksandar', ''], dtype=object)]
1,018
1209.6586
Jan T. Sobczyk
Jorge G. Morfin, Juan Nieves, Jan T. Sobczyk
Recent Developments in Neutrino/Antineutrino - Nucleus Interactions
37 pages, 7 figures, to be published in Advances in High Energy Physics
null
null
FERMILAB-PUB-12-529-PPD
hep-ex hep-ph nucl-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Recent experimental results and developments in the theoretical treatment of neutrino-nucleus interactions in the energy range of 1-10 GeV are discussed. Difficulties in extracting neutrino-nucleon cross sections from neutrino-nucleus scattering data are explained and significance of understanding nuclear effects for neutrino oscillation experiments is stressed. Detailed discussions of the status of two-body current contribution in the kinematic region dominated by quasi-elastic scattering and specific features of partonic nuclear effects in weak DIS scattering are presented.
[{'version': 'v1', 'created': 'Fri, 28 Sep 2012 17:58:00 GMT'}]
2012-10-01
[array(['Morfin', 'Jorge G.', ''], dtype=object) array(['Nieves', 'Juan', ''], dtype=object) array(['Sobczyk', 'Jan T.', ''], dtype=object)]
1,019
1101.0055
Yves Grandati
Yves Grandati (FCN)
Solvable rational extensions of the isotonic oscillator
null
Annals Phys.326:2074-2090,2011
10.1016/j.aop.2011.03.001
null
math-ph math.MP quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Combining recent results on rational solutions of the Riccati-Schr\"odinger equations for shape invariant potentials to the finite difference B\"acklund algorithm and specific symmetries of the isotonic potential, we show that it is possible to generate the three infinite sets (L1, L2 and L3 families) of regular rational solvable extensions of this potential in a very direct and transparent way.
[{'version': 'v1', 'created': 'Thu, 30 Dec 2010 08:26:12 GMT'} {'version': 'v2', 'created': 'Thu, 13 Jan 2011 13:24:40 GMT'}]
2011-06-16
[array(['Grandati', 'Yves', '', 'FCN'], dtype=object)]
1,020
2207.04359
Carlos Ceja-Espinosa
Carlos Ceja-Espinosa, Mehrdad Pirnia, Claudio A. Ca\~nizares
A Privacy-Preserving Energy Management System for Cooperative Multi-Microgrid Networks
In proceedings of the 11th Bulk Power Systems Dynamics and Control Symposium (IREP 2022), July 25-30, 2022, Banff, Canada
null
null
IREP2022-17
eess.SY cs.SY
http://creativecommons.org/licenses/by/4.0/
This paper presents an Energy Management System (EMS) that considers power exchanges between a set of interconnected microgrids (MGs) and the main grid, in the context of Multi-MG (MMG) systems. The model is first formulated as a centralized optimization problem, which is then decomposed into subproblems corresponding to each MG, using Lagrangian relaxation, and solved through a distributed approach using a subgradient method. The proposed model determines the power exchanges minimizing the operation cost of each MG, considering grid constraints and preserving the privacy of each MG by not revealing their generation cost and demand information. The distributed approach is validated with respect to the centralized problem, and various case studies are presented to demonstrate the performance of the proposed approach, comparing the costs of the MGs operating individually and cooperatively. The results show that all MGs in the MMG system improve their cost as consequence of the power exchanges, thus demonstrating the advantages of interconnecting MGs.
[{'version': 'v1', 'created': 'Sun, 10 Jul 2022 01:30:21 GMT'}]
2022-07-12
[array(['Ceja-Espinosa', 'Carlos', ''], dtype=object) array(['Pirnia', 'Mehrdad', ''], dtype=object) array(['Cañizares', 'Claudio A.', ''], dtype=object)]
1,021
0807.2468
Christopher Search
Ivana Djuric, Marko Zivkovic, Chris P. Search, and Greg Recine
Quantum bistability and spin current shot noise of a single quantum dot coupled to an optical microcavity
null
null
10.1103/PhysRevB.78.195316
null
cond-mat.mes-hall
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Here we explore spin dependent quantum transport through a single quantum dot coupled to an optical microcavity. The spin current is generated by electron tunneling between a single doped reservoir and the dot combined with intradot spin flip transitions induced by a quantized cavity mode. In the limit of strong Coulomb blockade, this model is analogous to the Jaynes-Cummings model in quantum optics and generates a pure spin current in the absence of any charge current. Earlier research has shown that in the classical limit where a large number of such dots interact with the cavity field, the spin current exhibits bistability as a function of the laser amplitude that drives the cavity. We show that in the limit of a single quantum dot this bistability continues to be present in the intracavity photon statistics. Signatures of the bistable photon statistics manifest themselves in the frequency dependent shot noise of the spin current despite the fact that the quantum mechanical average spin current no longer exhibits bistability. Besides having significance for future quantum dot based optoelectronic devices, our results shed light on the relation between bistability, which is traditionally viewed as a classical effect, and quantum mechanics.
[{'version': 'v1', 'created': 'Tue, 15 Jul 2008 21:42:50 GMT'}]
2009-11-13
[array(['Djuric', 'Ivana', ''], dtype=object) array(['Zivkovic', 'Marko', ''], dtype=object) array(['Search', 'Chris P.', ''], dtype=object) array(['Recine', 'Greg', ''], dtype=object)]
1,022
cond-mat/9507106
Ryusuke Ikeda
Ryusuke Ikeda (Dept. of Phys., Kyoto Univ., Japan)
Hydrodynamics and Nonlocal Conductivities in Vortex States of Type II Superconductors
12 pages, no figures, to appear in J. Phys. Soc. Jpn. in October, 1995
null
10.1143/JPSJ.64.3925
null
cond-mat
null
A hydrodynamical description for vortex states in type II superconductors is presented based on the time-dependent Ginzburg-Landau equation (TDGL). In contrast to the familiar extension of a single vortex dynamics based on the force balance, our description is consistent with the known hydrodynamics of a rotating neutral superfluid and correctly includes informations on the Goldstone mode. Further it enables one to examine nonlocal conductivities perpendicular to the magnetic field in terms of Kubo formula. The nonlocal conductivities deviate from the usual vortex flow expressions typically when the nonlocality parallel to the field becomes weaker than the perpendicular one measuring a degree of positional correlations, and, for instance, the superconducting contribution of dc Hall conductivity nonlocal only in directions perpendicular to the field becomes vanishingly small in the situations with large shear viscosity, leading to an experimentally measurable relation $\rho_{xy} \sim {\rho_{xx}^2}$ among the total resistivity components. Other situations are also discussed on the basis of the resulting expressions.
[{'version': 'v1', 'created': 'Tue, 25 Jul 1995 05:50:31 GMT'}]
2009-10-28
[array(['Ikeda', 'Ryusuke', '', 'Dept. of Phys., Kyoto Univ., Japan'], dtype=object) ]
1,023
cond-mat/0103501
John Singleton
Charles Mielke, John Singleton, Moon-Sun Nam, Neil Harrison, C.C. Agosta, B. Fravel and L. K. Montgomery
Superconducting properties and Fermi-surface topology of the quasi-two-dimensional organic superconductor $\lambda$-(BETS)$_{2}$GaCl$_{4}$
24 pages 10 figures
null
10.1088/0953-8984/13/36/308
null
cond-mat.supr-con cond-mat.dis-nn cond-mat.str-el
null
The Fermi surface topology of the organic superconductor \lbets has been determined using the Shubnikov-de Haas and magnetic breakdown effects and angle-dependent magnetoresistance oscillations. The former experiments were carried out in pulsed fields of up to 60 T, whereas the latter employed quasistatic fields of up to 30 T. All of these data show that the Fermi-surface topology of \lbets is very similar to that of the most heavily-studied organic superconductor, \cuscn, except in one important respect; the interplane transfer integral in \lbets is a factor $\sim 10$ larger than that in \cuscn . The increased three-dimensionality of \lbets is manifested in radiofrequency penetration-depth measurements, which show a clear dimensional crossover in the behaviour of $H_{c2}(T)$. The radiofrequency measurements have also been used to extract the Labusch parameter determining the fluxoid interactions as a function of temperature, and to map the flux-lattice melting curve.
[{'version': 'v1', 'created': 'Fri, 23 Mar 2001 22:13:40 GMT'} {'version': 'v2', 'created': 'Tue, 31 Jul 2001 23:04:45 GMT'}]
2009-11-07
[array(['Mielke', 'Charles', ''], dtype=object) array(['Singleton', 'John', ''], dtype=object) array(['Nam', 'Moon-Sun', ''], dtype=object) array(['Harrison', 'Neil', ''], dtype=object) array(['Agosta', 'C. C.', ''], dtype=object) array(['Fravel', 'B.', ''], dtype=object) array(['Montgomery', 'L. K.', ''], dtype=object)]
1,024
1507.03492
Mario Collura
Mario Collura, Pasquale Calabrese and Fabian H. L. Essler
Quantum quench within the gapless phase of the spin-1/2 Heisenberg XXZ spin-chain
27 pages, 13 figures
Phys. Rev. B 92, 125131 (2015)
10.1103/PhysRevB.92.125131
null
cond-mat.stat-mech cond-mat.str-el quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We consider an interaction quench in the critical spin-1/2 Heisenberg XXZ chain. We numerically compute the time evolution of the two-point correlation functions of spin operators in the thermodynamic limit and compare the results to predictions obtained in the framework of the Luttinger liquid approximation. We find that the transverse correlation function $\langle S^x_jS^x_{j+\ell}\rangle$ agrees with the Luttinger model prediction to a surprising level of accuracy. The agreement for the longitudinal two-point function $\langle S^z_jS^z_{j+\ell}\rangle$ is found to be much poorer. We speculate that this difference between transverse and longitudinal correlations has its origin in the locality properties of the respective spin operator with respect to the underlying fermionic modes.
[{'version': 'v1', 'created': 'Mon, 13 Jul 2015 15:24:30 GMT'}]
2015-09-23
[array(['Collura', 'Mario', ''], dtype=object) array(['Calabrese', 'Pasquale', ''], dtype=object) array(['Essler', 'Fabian H. L.', ''], dtype=object)]
1,025
2006.05495
Lucio Santi
Lucio Santi, Joaqu\'in Fern\'andez, Ernesto Kofman, Rodrigo Castro
retQSS: A Novel Methodology for Efficient Modeling and Simulation of Particle Systems in Reticulated Geometries
Accepted for publication in Computer Physics Communications
Comput. Phys. Commun. 270 (2022) 108157
10.1016/j.cpc.2021.108157
null
physics.comp-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This work presents retQSS, a novel methodology for efficient modeling and simulation of particle systems in reticulated meshed geometries. On the simulation side, retQSS profits from the discrete-event nature of Quantized State System (QSS) methods, which enable efficient particle tracking algorithms that are agnostic of the application domain. On the modeling side, retQSS relies on the standardized Modelica modeling language, yielding compact and elegant specifications of hybrid (continuous/discrete) dynamic systems. Combined together, these features offer a sound, general-purpose framework for modeling and simulation of particle systems. We show how the state-events that arise when particles interact with a reticulated mesh are seamlessly translated into easily tractable time-events. The latter can substantially improve simulation performance in scenarios where discontinuities dominate the computational demand. We showcase the flexibility of our approach by addressing four case studies arising from different application domains. Performance studies revealed that retQSS can perform similarly to, and even outperform, well-known domain-specific particle simulation toolkits while offering a clear and sound accuracy control interface.
[{'version': 'v1', 'created': 'Tue, 9 Jun 2020 20:31:34 GMT'} {'version': 'v2', 'created': 'Wed, 15 Sep 2021 01:47:37 GMT'} {'version': 'v3', 'created': 'Thu, 16 Sep 2021 03:39:16 GMT'}]
2021-09-17
[array(['Santi', 'Lucio', ''], dtype=object) array(['Fernández', 'Joaquín', ''], dtype=object) array(['Kofman', 'Ernesto', ''], dtype=object) array(['Castro', 'Rodrigo', ''], dtype=object)]
1,026
2303.06411
Qiong Wu
Hongbiao Zhu, Qiong Wu, Qiang Fan, Pingyi Fan, Jiangzhou Wang, and Zhengquan Li
Deep Reinforcement Learning Based Power Allocation for Minimizing AoI and Energy Consumption in MIMO-NOMA IoT Systems
null
null
null
null
cs.IT cs.AI math.IT
http://creativecommons.org/licenses/by/4.0/
Multi-input multi-out and non-orthogonal multiple access (MIMO-NOMA) internet-of-things (IoT) systems can improve channel capacity and spectrum efficiency distinctly to support the real-time applications. Age of information (AoI) is an important metric for real-time application, but there is no literature have minimized AoI of the MIMO-NOMA IoT system, which motivates us to conduct this work. In MIMO-NOMA IoT system, the base station (BS) determines the sample collection requirements and allocates the transmission power for each IoT device. Each device determines whether to sample data according to the sample collection requirements and adopts the allocated power to transmit the sampled data to the BS over MIMO-NOMA channel. Afterwards, the BS employs successive interference cancelation (SIC) technique to decode the signal of the data transmitted by each device. The sample collection requirements and power allocation would affect AoI and energy consumption of the system. It is critical to determine the optimal policy including sample collection requirements and power allocation to minimize the AoI and energy consumption of MIMO-NOMA IoT system, where the transmission rate is not a constant in the SIC process and the noise is stochastic in the MIMO-NOMA channel. In this paper, we propose the optimal power allocation to minimize the AoI and energy consumption of MIMO- NOMA IoT system based on deep reinforcement learning (DRL). Extensive simulations are carried out to demonstrate the superiority of the optimal power allocation.
[{'version': 'v1', 'created': 'Sat, 11 Mar 2023 14:09:46 GMT'}]
2023-03-14
[array(['Zhu', 'Hongbiao', ''], dtype=object) array(['Wu', 'Qiong', ''], dtype=object) array(['Fan', 'Qiang', ''], dtype=object) array(['Fan', 'Pingyi', ''], dtype=object) array(['Wang', 'Jiangzhou', ''], dtype=object) array(['Li', 'Zhengquan', ''], dtype=object)]
1,027
1202.3000
Sudarshan Tiwari
Sudarshan Tiwari, Axel Klar, Steffen Hardt
Simulation of a moving liquid droplet inside a rarefied gas region
null
null
null
null
math.NA physics.flu-dyn
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the dynamics of a liquid droplet inside a gas over a large range of the Knudsen numbers. The moving liquid droplet is modeled by the incompressible Navier-Stokes equations, the surrounding rarefied gas by the Boltzmann equation. The interface boundary conditions between the gas and liquid phases are derived. The incompressible Navier-Stokes equations are solved by a meshfree Lagrangian particle method called Finite Pointset Method (FPM), and the Boltzmann equation by a DSMC type of particle method. To validiate the coupled solutions of the Boltzmann and the incompressible Navier-Stokes equations we have further solved the compressible and the incompressible Navier-Stokes equations in the gas and liquid phases, respectively. In the latter case both the compressible and the incompressible Navier-Stokes equations are also solved by the FPM. In the continuum regime the coupled solutions obtained from the Boltzmann and the incompressible Navier-Stokes equations match with the solutions obtained from the compressible and the incompressible Navier-Stokes equations. In this paper, we presented solutions in one-dimensional physical space.
[{'version': 'v1', 'created': 'Tue, 14 Feb 2012 11:14:55 GMT'}]
2012-02-15
[array(['Tiwari', 'Sudarshan', ''], dtype=object) array(['Klar', 'Axel', ''], dtype=object) array(['Hardt', 'Steffen', ''], dtype=object)]
1,028
1612.00513
Kyle Stewart
Kyle R. Stewart (CBU)
Gas Accretion and Angular Momentum
22 pages, 3 figures. Invited review to appear in Gas Accretion onto Galaxies, Astrophysics and Space Science Library, eds. A. J. Fox & R. Dav\'e, to be published by Springer
ASSL, 430, 249S, 2017
10.1007/978-3-319-52512-9_11
null
astro-ph.GA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this chapter, we review the role of gas accretion to the acquisition of angular momentum, both in galaxies and in their gaseous halos. We begin by discussing angular momentum in dark matter halos, with a brief review of tidal torque theory and the importance of mergers, followed by a discussion of the canonical picture of galaxy formation within this framework, where halo gas is presumed to shock-heat to the virial temperature of the halo, following the same spin distribution as the dark matter halo before cooling to the center of the halo to form a galaxy there. In the context of recent observational evidence demonstrating the presence of high angular momentum gas in galaxy halos, we review recent cosmological hydrodynamic simulations that have begun to emphasize the role of "cold flow" accretion---anisotropic gas accretion along cosmic filaments that does not shock-heat before sinking to the central galaxy. We discuss the implications of these simulations, reviewing a number of recent developments in the literature, and suggest a revision to the canonical model as it relates to the expected angular momentum content of gaseous halos around galaxies.
[{'version': 'v1', 'created': 'Thu, 1 Dec 2016 23:19:31 GMT'}]
2017-08-25
[array(['Stewart', 'Kyle R.', '', 'CBU'], dtype=object)]
1,029
1906.01390
Thomas Giletti
Thomas Giletti (IECL), Hiroshi Matano (MIMS)
Existence and uniqueness of propagating terraces
Communications in Contemporary Mathematics, World Scientific Publishing, In press
null
null
null
math.AP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This work focuses on dynamics arising from reaction-diffusion equations , where the profile of propagation is no longer characterized by a single front, but by a layer of several fronts which we call a propagating terrace. This means, intuitively, that transition from one equilibrium to another may occur in several steps, that is, successive phases between some intermediate stationary states. We establish a number of properties on such propagating terraces in a one-dimensional periodic environment, under very wide and generic conditions. We are especially concerned with their existence, uniqueness, and their spatial structure. Our goal is to provide insight into the intricate dynamics arising from multistable non-linearities.
[{'version': 'v1', 'created': 'Tue, 4 Jun 2019 13:01:13 GMT'}]
2019-06-05
[array(['Giletti', 'Thomas', '', 'IECL'], dtype=object) array(['Matano', 'Hiroshi', '', 'MIMS'], dtype=object)]
1,030
math/9810134
Amnon Yekutieli
Amnon Yekutieli
Dualizing Complexes, Morita Equivalence and the Derived Picard Group of a Ring
22 pages, AMALaTeX, to appear in: J. London Math. Soc
null
null
null
math.RA math.RT
null
Two rings A and B are said to be derived Morita equivalent if their derived categories of modules are equivalent. By results of Rickard, if A and B are derived Morita equivalent algebras over a field k, then there is a complex of bimodules T s.t. the derived tensor product with T is an equivalence. The complex T is called a tilting complex. When B = A the isomorphism classes of tilting complexes T form the derived Picard group DPic(A). We prove that when the algebra A is either local or commutative, then any derived Morita equivalent algebra B is actually Morita equivalent. So we can compute DPic(A) in these cases. Assume A is noetherian. Dualizing complexes over A were defined by the author some years ago. These are complexes of bimodules which generalize the commutative definition of Grothendieck. We prove that the group DPic(A) classifies the set of isomorphism classes of dualizing complexes. Finally we consider finite k-algebras. For the algebra A of upper triangular 2 x 2 matrices over k, we prove that t^{3} = s, where t, s are the classes in DPic(A) of Hom_{k}(A, k) and A[1] respectively. In the Appendix by Elena Kreines this result is generalized to upper triangular n x n matrices, and it is shown that the relation t^{n + 1} = s^{n - 1} holds.
[{'version': 'v1', 'created': 'Thu, 22 Oct 1998 06:00:05 GMT'}]
2007-05-23
[array(['Yekutieli', 'Amnon', ''], dtype=object)]
1,031
2002.04394
Mario Mastriani
Mario Mastriani
Quantum Image Processing: the truth, the whole truth, and nothing but the truth about its problems on internal image representation and outcomes recovering
57 pages, 65 Figures, 3 Tables. Invited paper to 2020 Congress of Physics, Asociacion Fisica Argentina (AFA). July 2-6, Bahia Blanca, Buenos Aires, Argentina
null
null
null
quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, three techniques of internal image-representation in a quantum computer are compared: Flexible Representation of Quantum Images (FRQI), Novel Enhanced Quantum Representation of digital images (NEQR), and Quantum Boolean Image Processing (QBIP). All conspicuous technical items are considered in this comparison for complete analysis: i) performance as Classical-to-Quantum (Cl2Qu) interface, ii) characteristics of the employed qubits, iii) sparsity of the used internal registers, iv) number and size of the required registers, v) quality in the outcomes recovering, vi) number of required gates and its consequent accumulated noise, vi) decoherence, and vii) fidelity. These analyses and demonstrations are automatically extended to all variants of FRQI and NEQR. This study demonstrated the practical infeasibility in the implementation of FRQI and NEQR on a physical quantum computer (QPU), while QBIP has proven to be extremely successful on a) the four main quantum simulators on the cloud, b) two QPUs, and c) optical circuits from three labs. Moreover, QBIP also demonstrated its economy regarding the required resources needed for its proper function and its great robustness (immunity to noise), among other advantages, in fact, without any exceptions.
[{'version': 'v1', 'created': 'Thu, 6 Feb 2020 19:34:47 GMT'} {'version': 'v2', 'created': 'Fri, 21 Feb 2020 19:35:07 GMT'} {'version': 'v3', 'created': 'Wed, 24 Jun 2020 17:09:52 GMT'}]
2020-06-25
[array(['Mastriani', 'Mario', ''], dtype=object)]
1,032
cond-mat/0212024
Zhong Fang
Zhong Fang, Naoto Nagaosa, and Kiyoyuki Terakura
Anisotropic Optic Conductivities due to Spin and Orbital Orderings in LaVO3 and YVO3: First-Principles Studies
6 pages, 3 figures, accepted by PRB
Phys. Rev. B 67, 035101 (2003).
10.1103/PhysRevB.67.035101
null
cond-mat.str-el cond-mat.mtrl-sci
null
The anisotropy of low energy (0$\sim$5eV) optical excitations in strongly correlated transition-metal oxides is closely related to the spin and orbital orderings. The recent successes of LDA+$U$ method in describing the magnetic and electronic structures enable us to calculate the optical conductivity from first-principles. The LaVO$_3$ and YVO$_3$, both of which have $3d^2$ configuration and have various spin and orbital ordered phases at low temperature, show distinct anisotropy in the optical spectra. The effects of spin and orbital ordering on the anisotropy are studied in detail based on our first-principles calculations. The experimental spectra of both compounds at low temperature phases can be qualitatively explained with our calculations, while the studies for the intermediate temperature phase of YVO$_3$ suggest the substantial persistence of the low temperature phase at elevated temperature.
[{'version': 'v1', 'created': 'Mon, 2 Dec 2002 06:49:23 GMT'}]
2009-11-07
[array(['Fang', 'Zhong', ''], dtype=object) array(['Nagaosa', 'Naoto', ''], dtype=object) array(['Terakura', 'Kiyoyuki', ''], dtype=object)]
1,033
1911.02325
Gustavo Mata
Marcos Barrios and Gustavo Mata
On algebras of $\Omega^n$-finite and $\Omega^{\infty}$-infinite representation type
null
null
null
null
math.RT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Co-Gorenstein algebras were introduced by A. Beligiannis in \cite{B}. In \cite{KM}, the authors propose the following conjecture (Co-GC): if $\Omega^n (\mod A)$ is extension closed for all $n \leq 1$, then $A$ is right Co-Gorenstein, and they prove that the Generalized Nakayama Conjecture implies the Co-GC, also that the Co-GC implies the Nakayama Conjecture. In this article we characterize the subcategory $\Omega^{\infty}(\mod A)$ for algebras of $\Omega^{n}$-finite representation type. As a consequence, we characterize when a truncated path algebra is a Co-Gorenstein algebra in terms of its associated quiver. We also study the behaviour of Artin algebras of $\Omega^{\infty}$-infinite representation type. Finally, it is presented an example of a non Gorenstein algebra of $\Omega^{\infty}$-infinite representation type and an example of a finite dimensional algebra with infinite $\phi$-dimension.
[{'version': 'v1', 'created': 'Wed, 6 Nov 2019 11:50:57 GMT'} {'version': 'v2', 'created': 'Sat, 1 Apr 2023 18:31:14 GMT'}]
2023-04-04
[array(['Barrios', 'Marcos', ''], dtype=object) array(['Mata', 'Gustavo', ''], dtype=object)]
1,034
2012.10520
Ralph Malein
Ralph N. E. Malein, Prince Khatri, Andrew J. Ramsay, Isaac J. Luxmoore
Stimulated emission depletion spectroscopy of color centers in hexagonal boron nitride
null
ACS Photonics 2021, 8, 4, 1007-1012
10.1021/acsphotonics.0c01917
null
cond-mat.mes-hall
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We demonstrate the use of Stimulated Emission Depletion (STED) spectroscopy to map the electron-optical-phonon sideband of the ground state of the radiative transition of color centers in hexagonal boron nitride emitting at 2.0-2.2 eV, with in-plane linear polarization. The measurements are compared to Photoluminescence of Excitation (PLE) spectra, that maps the electron-optical-phonon sideband of the excited state. The main qualitative difference is a red-shift in the longitudinal optical phonon peak associated with $E_{1u}$ symmetry at the zone center. We argue that this is consistent with recent findings for a carbon-based line defect with admixture of energetically similar excited states.
[{'version': 'v1', 'created': 'Fri, 18 Dec 2020 21:30:49 GMT'}]
2021-05-27
[array(['Malein', 'Ralph N. E.', ''], dtype=object) array(['Khatri', 'Prince', ''], dtype=object) array(['Ramsay', 'Andrew J.', ''], dtype=object) array(['Luxmoore', 'Isaac J.', ''], dtype=object)]
1,035
1910.02281
Dan Xie
Dan Xie, Wenbin Yan
4d $\mathcal{N}=2$ SCFTs and lisse W-algebras
55 pages, 8 figures, 23 tables
null
null
null
hep-th math-ph math.MP math.QA math.RT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We continue our studies of the correspondence between 4d $\mathcal{N}=2$ SCFTs and 2d W-algebras. The purpose of this paper is to study the relationship between 2d lisse W-algebras and their 4d SCFT partners. The lisse W-algebra is the W-algebra whose associated Zhu's $C_2$ algebra is finite dimensional. As the associated variety of Zhu's $C_2$ algebra is identified with the Higgs branch in the 4d/2d correspondence, the lisse condition is equivalent to the absence of the Higgs branch on the 4d side. We classify 4d $\mathcal{N}=2$ SCFTs which do not admit Higgs branch, then these theories would give lisse W-algebras through the 4d/2d correspondence. In particular, we predict the existence of a large class of new non-admissible lisse W-algebras, which have not been studied before. The 4d theories corresponding to lisse W-algebra can appear in the Higgs branches of generic 4d $\mathcal{N}=2$ SCFTs, therefore they are crucial to understand the Higgs branches of $\mathcal{N}=2$ SCFTs.
[{'version': 'v1', 'created': 'Sat, 5 Oct 2019 14:58:27 GMT'}]
2019-10-10
[array(['Xie', 'Dan', ''], dtype=object) array(['Yan', 'Wenbin', ''], dtype=object)]
1,036
2011.09745
Osama Idais
Osama Idais and Rainer Schwabe
In- and Equivariance for Optimal Designs in Generalized Linear Models: The Gamma Model
22 pages, 6 figures
null
null
null
math.ST stat.ME stat.TH
http://creativecommons.org/licenses/by/4.0/
We give an overview over the usefulness of the concept of equivariance and invariance in the design of experiments for generalized linear models. In contrast to linear models here pairs of transformations have to be considered which act simultaneously on the experimental settings and on the location parameters in the linear component. Given the transformation of the experimental settings the parameter transformations are not unique and may be nonlinear to make further use of the model structure. The general concepts and results are illustrated by models with gamma distributed response. Locally optimal and maximin efficient design are obtained for the common D- and IMSE-criterion.
[{'version': 'v1', 'created': 'Thu, 19 Nov 2020 09:48:27 GMT'}]
2020-11-20
[array(['Idais', 'Osama', ''], dtype=object) array(['Schwabe', 'Rainer', ''], dtype=object)]
1,037
1107.5131
S. Weinzierl
Stefan Weinzierl
Does one need the O(epsilon)- and O(epsilon^2)-terms of one-loop amplitudes in an NNLO calculation ?
20 pages, minor modifications, version to be published
null
10.1103/PhysRevD.84.074007
null
hep-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
This article discusses the occurences of one-loop amplitudes within a next-to-next-to-leading order calculation. In an NNLO calculation the one-loop amplitude enters squared and one would therefore naively expect that the O(epsilon)- and O(epsilon^2)-terms of the one-loop amplitudes are required. I show that the calculation of these terms can be avoided if a method is known, which computes the O(epsilon^0)-terms of the finite remainder function of the two-loop amplitude.
[{'version': 'v1', 'created': 'Tue, 26 Jul 2011 07:36:03 GMT'} {'version': 'v2', 'created': 'Mon, 12 Sep 2011 19:14:52 GMT'}]
2013-05-29
[array(['Weinzierl', 'Stefan', ''], dtype=object)]
1,038
2110.10074
Gianfranco Bertone
R. Alves Batista, M. A. Amin, G. Barenboim, N. Bartolo, D. Baumann, A. Bauswein, E. Bellini, D. Benisty, G. Bertone, P. Blasi, C.G. B\"ohmer, \v{Z}. Bo\v{s}njak, T. Bringmann, C. Burrage, M. Bustamante, J. Calder\'on Bustillo, C. T. Byrnes, F. Calore, R. Catena, D. G. Cerde\~no, S. S. Cerri, M. Chianese, K. Clough, A. Cole, P. Coloma, A. Coogan, L. Covi, D. Cutting, A.C. Davis, C. de Rham, A. di Matteo, G. Dom\`enech, M. Drewes, T. Dietrich, T. D. P. Edwards, I. Esteban, R. Erdem, C. Evoli, M. Fasiello, S. M. Feeney, R. Z. Ferreira, A. Fialkov, N. Fornengo, S. Gabici, T. Galatyuk, D.Gaggero, D. Grasso, C. Gu\'epin, J. Harz, M. Herrero-Valea, T. Hinderer, N. B. Hogg, D. C. Hooper, F. Iocco, J. Isern, K. Karchev, B. J. Kavanagh, M. Korsmeier, K. Kotera, K. Koyama, B. Krishnan, J. Lesgourgues, J. Levi Said, L. Lombriser, C. S. Lorenz, S. Manconi, M. Mapelli, A. Marcowith, S. B. Markoff, D. J. E. Marsh, M. Martinelli, C.J.A.P. Martins, J. H. Matthews, A. Meli, O. Mena, J. Mifsud, M. M. Miller Bertolami, P. Millington, P. Moesta, K. Nippel, V. Niro, E. O'Connor, F. Oikonomou, C. F. Paganini, G. Pagliaroli, P. Pani, C. Pfrommer, S. Pascoli, L. Pinol, L. Pizzuti, R. A. Porto, A. Pound, F. Quevedo, G. G. Raffelt, A. Raccanelli, E. Ramirez-Ruiz, M. Raveri, S. Renaux-Petel, A. Ricciardone, A. Rida Khalifeh, A. Riotto, R. Roiban, J. Rubio, M. Sahl\'en, N. Sabti, L. Sagunski, N. \v{S}ar\v{c}evi\'c, K. Schmitz, P. Schwaller, T. Schwetz, A. Sedrakian, E. Sellentin, A. Serenelli, P.D. Serpico, E. I. Sfakianakis, S. Shalgar, A. Silvestri, I. Tamborra, K. Tanidis, D. Teresi, A. A. Tokareva, L. Tolos, S. Trojanowski, R. Trotta, C. Uhlemann, F. R. Urban, F. Vernizzi, A. van Vliet, F. L. Villante, A. Vincent, J. Vink, E. Vitagliano, C. Weniger, A. Wickenbrock, W. Winter, S. Zell, M. Zeng
EuCAPT White Paper: Opportunities and Challenges for Theoretical Astroparticle Physics in the Next Decade
White paper of the European Consortium for Astroparticle Theory (EuCAPT). 135 authors, 400 endorsers, 133 pages, 1382 references
null
null
null
astro-ph.HE astro-ph.CO
http://creativecommons.org/licenses/by-nc-nd/4.0/
Astroparticle physics is undergoing a profound transformation, due to a series of extraordinary new results, such as the discovery of high-energy cosmic neutrinos with IceCube, the direct detection of gravitational waves with LIGO and Virgo, and many others. This white paper is the result of a collaborative effort that involved hundreds of theoretical astroparticle physicists and cosmologists, under the coordination of the European Consortium for Astroparticle Theory (EuCAPT). Addressed to the whole astroparticle physics community, it explores upcoming theoretical opportunities and challenges for our field of research, with particular emphasis on the possible synergies among different subfields, and the prospects for solving the most fundamental open questions with multi-messenger observations.
[{'version': 'v1', 'created': 'Tue, 19 Oct 2021 16:00:15 GMT'}]
2021-10-20
[array(['Batista', 'R. Alves', ''], dtype=object) array(['Amin', 'M. A.', ''], dtype=object) array(['Barenboim', 'G.', ''], dtype=object) array(['Bartolo', 'N.', ''], dtype=object) array(['Baumann', 'D.', ''], dtype=object) array(['Bauswein', 'A.', ''], dtype=object) array(['Bellini', 'E.', ''], dtype=object) array(['Benisty', 'D.', ''], dtype=object) array(['Bertone', 'G.', ''], dtype=object) array(['Blasi', 'P.', ''], dtype=object) array(['Böhmer', 'C. G.', ''], dtype=object) array(['Bošnjak', 'Ž.', ''], dtype=object) array(['Bringmann', 'T.', ''], dtype=object) array(['Burrage', 'C.', ''], dtype=object) array(['Bustamante', 'M.', ''], dtype=object) array(['Bustillo', 'J. Calderón', ''], dtype=object) array(['Byrnes', 'C. T.', ''], dtype=object) array(['Calore', 'F.', ''], dtype=object) array(['Catena', 'R.', ''], dtype=object) array(['Cerdeño', 'D. G.', ''], dtype=object) array(['Cerri', 'S. S.', ''], dtype=object) array(['Chianese', 'M.', ''], dtype=object) array(['Clough', 'K.', ''], dtype=object) array(['Cole', 'A.', ''], dtype=object) array(['Coloma', 'P.', ''], dtype=object) array(['Coogan', 'A.', ''], dtype=object) array(['Covi', 'L.', ''], dtype=object) array(['Cutting', 'D.', ''], dtype=object) array(['Davis', 'A. C.', ''], dtype=object) array(['de Rham', 'C.', ''], dtype=object) array(['di Matteo', 'A.', ''], dtype=object) array(['Domènech', 'G.', ''], dtype=object) array(['Drewes', 'M.', ''], dtype=object) array(['Dietrich', 'T.', ''], dtype=object) array(['Edwards', 'T. D. P.', ''], dtype=object) array(['Esteban', 'I.', ''], dtype=object) array(['Erdem', 'R.', ''], dtype=object) array(['Evoli', 'C.', ''], dtype=object) array(['Fasiello', 'M.', ''], dtype=object) array(['Feeney', 'S. M.', ''], dtype=object) array(['Ferreira', 'R. Z.', ''], dtype=object) array(['Fialkov', 'A.', ''], dtype=object) array(['Fornengo', 'N.', ''], dtype=object) array(['Gabici', 'S.', ''], dtype=object) array(['Galatyuk', 'T.', ''], dtype=object) array(['Gaggero', 'D.', ''], dtype=object) array(['Grasso', 'D.', ''], dtype=object) array(['Guépin', 'C.', ''], dtype=object) array(['Harz', 'J.', ''], dtype=object) array(['Herrero-Valea', 'M.', ''], dtype=object) array(['Hinderer', 'T.', ''], dtype=object) array(['Hogg', 'N. B.', ''], dtype=object) array(['Hooper', 'D. C.', ''], dtype=object) array(['Iocco', 'F.', ''], dtype=object) array(['Isern', 'J.', ''], dtype=object) array(['Karchev', 'K.', ''], dtype=object) array(['Kavanagh', 'B. J.', ''], dtype=object) array(['Korsmeier', 'M.', ''], dtype=object) array(['Kotera', 'K.', ''], dtype=object) array(['Koyama', 'K.', ''], dtype=object) array(['Krishnan', 'B.', ''], dtype=object) array(['Lesgourgues', 'J.', ''], dtype=object) array(['Said', 'J. Levi', ''], dtype=object) array(['Lombriser', 'L.', ''], dtype=object) array(['Lorenz', 'C. S.', ''], dtype=object) array(['Manconi', 'S.', ''], dtype=object) array(['Mapelli', 'M.', ''], dtype=object) array(['Marcowith', 'A.', ''], dtype=object) array(['Markoff', 'S. B.', ''], dtype=object) array(['Marsh', 'D. J. E.', ''], dtype=object) array(['Martinelli', 'M.', ''], dtype=object) array(['Martins', 'C. J. A. P.', ''], dtype=object) array(['Matthews', 'J. H.', ''], dtype=object) array(['Meli', 'A.', ''], dtype=object) array(['Mena', 'O.', ''], dtype=object) array(['Mifsud', 'J.', ''], dtype=object) array(['Bertolami', 'M. M. Miller', ''], dtype=object) array(['Millington', 'P.', ''], dtype=object) array(['Moesta', 'P.', ''], dtype=object) array(['Nippel', 'K.', ''], dtype=object) array(['Niro', 'V.', ''], dtype=object) array(["O'Connor", 'E.', ''], dtype=object) array(['Oikonomou', 'F.', ''], dtype=object) array(['Paganini', 'C. F.', ''], dtype=object) array(['Pagliaroli', 'G.', ''], dtype=object) array(['Pani', 'P.', ''], dtype=object) array(['Pfrommer', 'C.', ''], dtype=object) array(['Pascoli', 'S.', ''], dtype=object) array(['Pinol', 'L.', ''], dtype=object) array(['Pizzuti', 'L.', ''], dtype=object) array(['Porto', 'R. A.', ''], dtype=object) array(['Pound', 'A.', ''], dtype=object) array(['Quevedo', 'F.', ''], dtype=object) array(['Raffelt', 'G. G.', ''], dtype=object) array(['Raccanelli', 'A.', ''], dtype=object) array(['Ramirez-Ruiz', 'E.', ''], dtype=object) array(['Raveri', 'M.', ''], dtype=object) array(['Renaux-Petel', 'S.', ''], dtype=object) array(['Ricciardone', 'A.', ''], dtype=object) array(['Khalifeh', 'A. Rida', ''], dtype=object) array(['Riotto', 'A.', ''], dtype=object) array(['Roiban', 'R.', ''], dtype=object) array(['Rubio', 'J.', ''], dtype=object) array(['Sahlén', 'M.', ''], dtype=object) array(['Sabti', 'N.', ''], dtype=object) array(['Sagunski', 'L.', ''], dtype=object) array(['Šarčević', 'N.', ''], dtype=object) array(['Schmitz', 'K.', ''], dtype=object) array(['Schwaller', 'P.', ''], dtype=object) array(['Schwetz', 'T.', ''], dtype=object) array(['Sedrakian', 'A.', ''], dtype=object) array(['Sellentin', 'E.', ''], dtype=object) array(['Serenelli', 'A.', ''], dtype=object) array(['Serpico', 'P. D.', ''], dtype=object) array(['Sfakianakis', 'E. I.', ''], dtype=object) array(['Shalgar', 'S.', ''], dtype=object) array(['Silvestri', 'A.', ''], dtype=object) array(['Tamborra', 'I.', ''], dtype=object) array(['Tanidis', 'K.', ''], dtype=object) array(['Teresi', 'D.', ''], dtype=object) array(['Tokareva', 'A. A.', ''], dtype=object) array(['Tolos', 'L.', ''], dtype=object) array(['Trojanowski', 'S.', ''], dtype=object) array(['Trotta', 'R.', ''], dtype=object) array(['Uhlemann', 'C.', ''], dtype=object) array(['Urban', 'F. R.', ''], dtype=object) array(['Vernizzi', 'F.', ''], dtype=object) array(['van Vliet', 'A.', ''], dtype=object) array(['Villante', 'F. L.', ''], dtype=object) array(['Vincent', 'A.', ''], dtype=object) array(['Vink', 'J.', ''], dtype=object) array(['Vitagliano', 'E.', ''], dtype=object) array(['Weniger', 'C.', ''], dtype=object) array(['Wickenbrock', 'A.', ''], dtype=object) array(['Winter', 'W.', ''], dtype=object) array(['Zell', 'S.', ''], dtype=object) array(['Zeng', 'M.', ''], dtype=object)]
1,039
1111.1572
Pierre Hily-Blant
Vincent Dislaire (IPAG), Pierre Hily-Blant (IPAG), Alexandre Faure (IPAG), S\'ebastien Maret (IPAG), Aurore Bacmann (IPAG), Guillaume Pineau Des For\^ets (IAS, LERMA)
Nitrogen hydrides and the H2 ortho-to-para ratio in dark clouds
Accepted for publication in A\&A
null
10.1051/0004-6361/201117765
null
astro-ph.GA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Nitrogen bearing species are common tracers of the physical conditions in a wide variety of objects, and most remarkably in dark clouds. The reservoir of gaseous nitrogen is expected to be atomic or molecular, but none of the two species are observable in the dark gas. Their abundances therefore derive indirectly from those of N-bearing species through chemical modelling. The recent years have accumulated data which stress our incomplete understanding of the nitrogen chemistry in dark cloud conditions. To tackle this problem of the nitrogen chemistry in cold gas, we have revised the formation of nitrogen hydrides, which is initiated by the key reaction \ce{N+ + H2 -> NH+ + H}. We propose a new rate for this reaction which depends on the ortho-to-para ratio of H2. This new rate allows to reproduce the abundance ratios of the three nitrogen hydrides, NH, \ce{NH2}, and \ce{NH3}, observed towards IRAS16293-2422, provided that the channel leading to NH from the dissociative recombination of \ce{N2H+} is not closed at low temperature. The ortho-to-para ratio of H2 is constrained to O/P=$10^{-3}$ by the abundance ratio NH:NH2, which provides a new method to measure O/P. This work stresses the need for reaction rates at the low temperatures of dark clouds, and for branching ratios of critical dissociative recombination reactions.
[{'version': 'v1', 'created': 'Mon, 7 Nov 2011 13:32:44 GMT'}]
2015-06-03
[array(['Dislaire', 'Vincent', '', 'IPAG'], dtype=object) array(['Hily-Blant', 'Pierre', '', 'IPAG'], dtype=object) array(['Faure', 'Alexandre', '', 'IPAG'], dtype=object) array(['Maret', 'Sébastien', '', 'IPAG'], dtype=object) array(['Bacmann', 'Aurore', '', 'IPAG'], dtype=object) array(['Forêts', 'Guillaume Pineau Des', '', 'IAS, LERMA'], dtype=object)]
1,040
hep-ex/0205071
Alexis Pompili
Alexis Pompili (for the BaBar collaboration)
Charm Mixing and Lifetimes at Babar
5 pages, 2 figures; proceedings of the XXXVII Rencontres de Moriond on Electroweak Interactions and Unified Theories, Les Arcs, France, 9-16 March 2002
null
null
null
hep-ex
null
Preliminary limits on the D^0 mixing parameter y = \Delta \Gamma / 2 \Gamma are obtained using about 57.8 fb^-1 of data collected by BaBar in 2000 and 2001:y = (1.4 \pm 1.0 (stat.) +0.6 -0.7 (syst.))%. y is extracted, provided that CP is conserved, by measuring separately the D^0 lifetime for the Cabibbo-suppressed decay modes K- K+, \pi- \pi+ and the Cabibbo-favoured mode K- \pi+. Backgrounds are suppressed by D*-tag and particle identification requirements.
[{'version': 'v1', 'created': 'Tue, 21 May 2002 19:26:21 GMT'}]
2007-05-23
[array(['Pompili', 'Alexis', '', 'for the BaBar collaboration'], dtype=object) ]
1,041
2207.05768
Yuxun Guo
Yuxun Guo, Xiangdong Ji and Kyle Shiells
Generalized parton distributions through universal moment parameterization: zero skewness case
29 pages, 11 figures
null
10.1007/JHEP09(2022)215
null
hep-ph nucl-th
http://creativecommons.org/licenses/by/4.0/
We present a global analysis program for the generalized parton distributions (GPDs) based on conformal moment expansion. We apply the strategy of universal moment parameterization to fit both the collinear parton distribution functions (PDFs) from phenomenology and generalized form factors from lattice calculations, and show that the parameterization is flexible enough to accommodate these constraints. In addition, we can also fit direct lattice calculations of GPDs from large-momentum effective theory. In this work we focus on the analysis of $t$-dependent PDFs which correspond to GPDs in the $\xi \to 0$ limit. The strategy also applies to the $\xi \not =0$ region with extra parameters, and therefore can be fitted to experimental observables in the future. With a demonstrative example of fitted GPDs, we exhibit the quark transverse angular momentum densities of the proton as well as the impact parameter space distributions of quarks in both unpolarized and transversely polarized protons.
[{'version': 'v1', 'created': 'Tue, 12 Jul 2022 18:00:06 GMT'}]
2022-10-19
[array(['Guo', 'Yuxun', ''], dtype=object) array(['Ji', 'Xiangdong', ''], dtype=object) array(['Shiells', 'Kyle', ''], dtype=object)]
1,042
1501.07116
Pedro Russo
Pedro Russo, Edward Gomez, Thilina Heenatigala and Linda Strubbe
Peer-review Platform for Astronomy Education Activities
8 pages, Published, 2015, eLearning Papers #40 ISSN: 1887-1542
null
null
null
astro-ph.IM physics.ed-ph
http://creativecommons.org/licenses/by/3.0/
Hundreds of thousands of astronomy education activities exist, but their discoverability and quality is highly variable. The web platform for astronomy education activities, astroEDU, presented in this paper tries to solve these issues. Using the familiar peer-review workflow of scientific publications, astroEDU is improving standards of quality, visibility and accessibility, while providing credibility to these astronomy education activities. astroEDU targets activity guides, tutorials and other educational activities in the area of astronomy education, prepared by teachers, educators and other education specialists. Each of the astroEDU activities is peer-reviewed by an educator as well as an astronomer to ensure a high standard in terms of scientific content and educational value. All reviewed materials are then stored in a free open online database, enabling broad distribution in a range of different formats. In this way astroEDU is not another web repository for educational resources but a mechanism for peer-reviewing and publishing high-quality astronomy education activities in an open access way. This paper will provide an account on the implementation and first findings of the use of astroEDU.
[{'version': 'v1', 'created': 'Wed, 28 Jan 2015 14:36:52 GMT'} {'version': 'v2', 'created': 'Tue, 3 Feb 2015 17:27:32 GMT'}]
2015-02-04
[array(['Russo', 'Pedro', ''], dtype=object) array(['Gomez', 'Edward', ''], dtype=object) array(['Heenatigala', 'Thilina', ''], dtype=object) array(['Strubbe', 'Linda', ''], dtype=object)]
1,043
1405.7410
David Fisher
David B. Fisher, Karl Glazebrook, Alberto Bolatto, Danail Obreschkow, Erin Mentuch-Cooper, Emily Wisnioski, Robert BAssett, Roberto G. Abraham, Ivana Damjanov, Andy Green, Peter McGregor
Extreme gas fractions in clumpy, turbulent disk galaxies at z~0.1
Accepted to ApJ Letters
null
10.1088/2041-8205/790/2/L30
null
astro-ph.GA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this letter we report the discovery of CO fluxes, suggesting very high gas fractions in three disk galaxies seen in the nearby Universe (z ~ 0.1). These galaxies were investigated as part of the DYnamics of Newly Assembled Massive Objects (DYNAMO) survey. High-resolution Hubble Space Telescope imaging of these objects reveals the presence of large star forming clumps in the bodies of the galaxies, while spatially resolved spectroscopy of redshifted Halpha reveals the presence of high dispersion rotating disks. The internal dynamical state of these galaxies resembles that of disk systems seen at much higher redshifts (1 < z < 3). Using CO(1-0) observations made with the Plateau de Bure Interferometer, we find gas fractions of 20-30% and depletion times of tdep ~ 0.5 Gyr (assuming a Milky Way-like CO conversion factor). These properties are unlike those expected for low- redshift galaxies of comparable specific star formation rate, but they are normal for their high-z counterparts. DYNAMO galaxies break the degeneracy between gas fraction and redshift, and we show that the depletion time per specific star formation rate for galaxies is closely tied to gas fraction, independent of redshift. We also show that the gas dynamics of two of our local targets corresponds to those expected from unstable disks, again resembling the dynamics of high-z disks. These results provide evidence that DYNAMO galaxies are local analogues to the clumpy, turbulent disks, which are often found at high redshift.
[{'version': 'v1', 'created': 'Wed, 28 May 2014 22:00:11 GMT'}]
2015-06-19
[array(['Fisher', 'David B.', ''], dtype=object) array(['Glazebrook', 'Karl', ''], dtype=object) array(['Bolatto', 'Alberto', ''], dtype=object) array(['Obreschkow', 'Danail', ''], dtype=object) array(['Mentuch-Cooper', 'Erin', ''], dtype=object) array(['Wisnioski', 'Emily', ''], dtype=object) array(['BAssett', 'Robert', ''], dtype=object) array(['Abraham', 'Roberto G.', ''], dtype=object) array(['Damjanov', 'Ivana', ''], dtype=object) array(['Green', 'Andy', ''], dtype=object) array(['McGregor', 'Peter', ''], dtype=object)]
1,044
2206.03556
Md Taimur Ahad
Syeda Nishat Tasnim (American international University), Md Taimur Ahad (American international University)
Toward IoT enabled smart offices: Achieving Sustainable Development Goals
9 pages, 6 figures
null
null
null
cs.HC
http://creativecommons.org/licenses/by/4.0/
Despite research advocating the Internet of Things (IoT) as an effective in-office monitoring system, little research has presented societal and climate centric discussions. Whereas the United Nations (UN) and other development agencies concerned with climate impact, are advocating transformative actions towards smart cities, very little research in the IoT domain analyzes the advantages of IoT in achieving sustainable development goals (SDGs) to fill this gap. In this study, a smart office (SO) was developed in a Cisco packet tracer. We then presented the SO through the lens of SDGs. We suggest that SOs support targets mentioned in Goal 6, 7, 8, 9, 11 and 12 of the SDGs. This research is crucial - both for developing and developed economies, as we move toward industrialization, while ignoring the adverse impacts of industrialization. This work is expected to provide a pathway with technological innovation toward a more sustainable world for IT practitioners, governments and development agencies.
[{'version': 'v1', 'created': 'Tue, 7 Jun 2022 20:14:19 GMT'}]
2022-06-09
[array(['Tasnim', 'Syeda Nishat', '', 'American international University'], dtype=object) array(['Ahad', 'Md Taimur', '', 'American international University'], dtype=object) ]
1,045
2102.00966
Conor F. Hayes
Conor F. Hayes, Mathieu Reymond, Diederik M. Roijers, Enda Howley, Patrick Mannion
Risk Aware and Multi-Objective Decision Making with Distributional Monte Carlo Tree Search
8 pages, 4 figures
null
null
null
cs.LG cs.AI
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In many risk-aware and multi-objective reinforcement learning settings, the utility of the user is derived from the single execution of a policy. In these settings, making decisions based on the average future returns is not suitable. For example, in a medical setting a patient may only have one opportunity to treat their illness. When making a decision, just the expected return -- known in reinforcement learning as the value -- cannot account for the potential range of adverse or positive outcomes a decision may have. Our key insight is that we should use the distribution over expected future returns differently to represent the critical information that the agent requires at decision time. In this paper, we propose Distributional Monte Carlo Tree Search, an algorithm that learns a posterior distribution over the utility of the different possible returns attainable from individual policy executions, resulting in good policies for both risk-aware and multi-objective settings. Moreover, our algorithm outperforms the state-of-the-art in multi-objective reinforcement learning for the expected utility of the returns.
[{'version': 'v1', 'created': 'Mon, 1 Feb 2021 16:47:39 GMT'} {'version': 'v2', 'created': 'Tue, 2 Feb 2021 14:06:18 GMT'}]
2021-02-03
[array(['Hayes', 'Conor F.', ''], dtype=object) array(['Reymond', 'Mathieu', ''], dtype=object) array(['Roijers', 'Diederik M.', ''], dtype=object) array(['Howley', 'Enda', ''], dtype=object) array(['Mannion', 'Patrick', ''], dtype=object)]
1,046
cs/0506069
Remi Monasson
Remi Monasson (LPTENS)
A generating function method for the average-case analysis of DPLL
RANDOM 2005, Berkeley, August 22-24
RANDOM 2005, Berkeley, CA, \'Etats-Unis d'Am\'erique, p.402-413
null
null
cs.CC cond-mat.dis-nn
null
A method to calculate the average size of Davis-Putnam-Loveland-Logemann (DPLL) search trees for random computational problems is introduced, and applied to the satisfiability of random CNF formulas (SAT) and the coloring of random graph (COL) problems. We establish recursion relations for the generating functions of the average numbers of (variable or color) assignments at a given height in the search tree, which allow us to derive the asymptotics of the expected DPLL tree size, 2^{N w + o(N)}, where N is the instance size. w is calculated as a function of the input distribution parameters (ratio of clauses per variable for SAT, average vertex degree for COL), and the branching heuristics.
[{'version': 'v1', 'created': 'Thu, 16 Jun 2005 09:17:21 GMT'}]
2008-06-20
[array(['Monasson', 'Remi', '', 'LPTENS'], dtype=object)]
1,047
1305.2939
Edwin Lee
E. Lee, D. R. Williams, and G. Lapenta
Spectroscopic indication of suprathermal ions in the solar corona
null
null
null
null
astro-ph.SR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Using spectroscopic data, we support the possibility of suprathermal distributions of coronal ions by fitting the equivalent kappa functions to their emission line profiles. We fit different kappa and Gaussian model functions to line profiles of the strong Fe xv line at 284.16 Angstroms, across two large-field spectroscopic rasters taken in a solar active region. Both single- and double-component Gaussian models are applied, as well as two kappa models, one with a free width parameter allowing for and the other with a constrained width that precludes "microturbulence". We then compare the goodness of fit of the computed best fits for each model. The kappa distribution is a generalization, or superset, of the Maxwellian, so they are able to fit line profiles more precisely than a Gaussian. In most of the data, the best-fit kappa model produces much lower residuals across the profile than any single Gaussian and sometimes double Gaussian. Most importantly, the distribution of estimated kappa values is found to lie mostly in the low-kappa range, implying ion populations far from Maxwellian. Even when the width is removed as a free parameter of fit, the kappa model is still able to fit the data credibly, again with low best-fit values of kappa. We find the shape of the Fe xv line, in the vast majority of the data analyzed, to be indicative of a highly suprathermal ion population.
[{'version': 'v1', 'created': 'Mon, 13 May 2013 20:06:57 GMT'}]
2013-05-15
[array(['Lee', 'E.', ''], dtype=object) array(['Williams', 'D. R.', ''], dtype=object) array(['Lapenta', 'G.', ''], dtype=object)]
1,048
2212.08548
Stefano Pierini Prof.
Stefano Pierini
The deterministic excitation paradigm and the late Pleistocene glacial terminations
Submitted to Chaos (American Institute of Physics Publishing)
null
10.1063/5.0127715
null
physics.ao-ph nlin.CD
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A deterministic excitation (DE) paradigm is formulated, according to which the late Pleistocene glacial terminations correspond to the excitation, by the orbital forcing, of nonlinear relaxation oscillations (ROs) internal to the climate system in the absence of any stochastic parameterization. Specific threshold crossing rules parameterizing the activation of internal climate feedbacks leading to RO excitations are derived according to the DE assumption. They are then applied to an energy balance model describing the fluctuations induced by realistic orbital forcing on the glacial state. The timing of the glacial terminations thus obtained in a reference simulation is found to be in good agreement with proxy records. A sensitivity analysis insures the robustness of the timing. The potential irrelevance of noise allowing DE to hold is discussed, and a possible explanation of the 100-kyr cycle problem based on DE is outlined. In conclusion, the DE paradigm characterizes in one of the simplest possible ways the link between orbital forcing and glacial terminations implied by the Milankovitch hypothesis.
[{'version': 'v1', 'created': 'Fri, 16 Dec 2022 15:58:12 GMT'}]
2023-03-22
[array(['Pierini', 'Stefano', ''], dtype=object)]
1,049
1001.2095
Hrachya Nersisyan
H.B. Nersisyan, G. Zwicknagel
Energy transfer in binary collisions of two gyrating charged particles in a magnetic field
12 pages, 4 figures
null
10.1063/1.3476266
null
physics.plasm-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Binary collisions of the gyrating charged particles in an external magnetic field are considered within a classical second-order perturbation theory, i.e., up to contributions which are quadratic in the binary interaction, starting from the unperturbed helical motion of the particles. The calculations are done with the help of a binary collisions treatment which is valid for any strength of the magnetic field and involves all harmonics of the particles cyclotron motion. The energy transfer is explicitly calculated for a regularized and screened potential which is both of finite range and nonsingular at the origin. The validity of the perturbation treatment is evaluated by comparing with classical trajectory Monte Carlo (CTMC) calculations which also allow to investigate the strong collisions with large energy and velocity transfer at low velocities. For large initial velocities on the other hand, only small velocity transfers occur. There the nonperturbative numerical CTMC results agree excellently with the predictions of the perturbative treatment.
[{'version': 'v1', 'created': 'Wed, 13 Jan 2010 08:03:08 GMT'}]
2015-05-14
[array(['Nersisyan', 'H. B.', ''], dtype=object) array(['Zwicknagel', 'G.', ''], dtype=object)]
1,050
2101.01843
Zhenyi Liu
Zhenyi Liu, Joyce Farrell, Brian Wandell
ISETAuto: Detecting vehicles with depth and radiance information
null
null
null
null
cs.CV
http://creativecommons.org/licenses/by/4.0/
Autonomous driving applications use two types of sensor systems to identify vehicles - depth sensing LiDAR and radiance sensing cameras. We compare the performance (average precision) of a ResNet for vehicle detection in complex, daytime, driving scenes when the input is a depth map (D = d(x,y)), a radiance image (L = r(x,y)), or both [D,L]. (1) When the spatial sampling resolution of the depth map and radiance image are equal to typical camera resolutions, a ResNet detects vehicles at higher average precision from depth than radiance. (2) As the spatial sampling of the depth map declines to the range of current LiDAR devices, the ResNet average precision is higher for radiance than depth. (3) For a hybrid system that combines a depth map and radiance image, the average precision is higher than using depth or radiance alone. We established these observations in simulation and then confirmed them using realworld data. The advantage of combining depth and radiance can be explained by noting that the two type of information have complementary weaknesses. The radiance data are limited by dynamic range and motion blur. The LiDAR data have relatively low spatial resolution. The ResNet combines the two data sources effectively to improve overall vehicle detection.
[{'version': 'v1', 'created': 'Wed, 6 Jan 2021 01:37:43 GMT'} {'version': 'v2', 'created': 'Thu, 7 Jan 2021 02:25:02 GMT'}]
2021-01-08
[array(['Liu', 'Zhenyi', ''], dtype=object) array(['Farrell', 'Joyce', ''], dtype=object) array(['Wandell', 'Brian', ''], dtype=object)]
1,051
2102.11940
Martin Roelfs
Martin Roelfs
Geometric invariant decomposition of SU(3)
7 pages
null
null
null
math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A novel invariant decomposition of diagonalizable $n \times n$ matrices into $n$ commuting matrices is presented. This decomposition is subsequently used to split the fundamental representation of $\mathfrak{su}(3)$ Lie algebra elements into at most three commuting elements of $\mathfrak{u}(3)$. As a result, the exponential of an $\mathfrak{su}(3)$ Lie algebra element can be split into three commuting generalized Euler's formulas, or conversely, a Lie group element can be factorized into at most three generalized Euler's formulas. After the factorization has been performed, the logarithm follows immediately.
[{'version': 'v1', 'created': 'Tue, 23 Feb 2021 21:04:07 GMT'}]
2021-02-25
[array(['Roelfs', 'Martin', ''], dtype=object)]
1,052
1609.05287
Lin Lin
Lin Lin, Cheng Li, Yanqin He, Ting Xiao, Enci Wang
Bar-induced central star formation as revealed by integral field spectroscopy from CALIFA
19 pages, 10 figures, ApJ accepted
null
10.3847/1538-4357/aa657a
null
astro-ph.GA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the recent star formation history (SFH) in the inner region of 57 nearly face-on spiral galaxies selected from the Calar Alto Legacy Integral Field Area (CALIFA) survey. For each galaxy we use the integral field spectroscopy from CALIFA to obtain two-dimensional maps and radial profiles of three parameters that are sensitive indicators of the recent SFH: the 4000\AA\ break (D$_n$(4000)), and the equivalent width of H$\delta$ absorption (EW(H$\delta_A$)) and H$\alpha$ emission (EW(H$\alpha$)). We have also performed photometric decomposition of bulge/bar/disk components based on SDSS optical image. We identify a class of 17 "turnover" galaxies whose central region present significant drop in D$_n$(4000), and most of them correspondingly show a central upturn in EW(H$\delta_A$) and EW(H$\alpha$). This indicates that the central region of the turnover galaxies has experienced star formation in the past 1-2 Gyr, which makes the bulge younger and more star-forming than surrounding regions. We find almost all (15/17) the turnover galaxies are barred, while only half of the barred galaxies in our sample (15/32) are classified as a turnover galaxy. This finding provides strong evidence in support of the theoretical expectation that the bar may drive gas from the disc inward to trigger star formation in galaxy center, an important channel for the growth/rejuvenation of pseudobulges in disc galaxies.
[{'version': 'v1', 'created': 'Sat, 17 Sep 2016 07:12:41 GMT'} {'version': 'v2', 'created': 'Wed, 8 Mar 2017 08:14:59 GMT'}]
2017-04-05
[array(['Lin', 'Lin', ''], dtype=object) array(['Li', 'Cheng', ''], dtype=object) array(['He', 'Yanqin', ''], dtype=object) array(['Xiao', 'Ting', ''], dtype=object) array(['Wang', 'Enci', ''], dtype=object)]
1,053
1511.06639
Pierre-Olivier Amblard
Augusto Zebadua, Pierre-Olivier Amblard, Eric Moisan and Olivier .J.J. Michel
Compressed and quantized correlation estimators
submitted
null
null
null
stat.AP cs.IT math.IT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In passive monitoring using sensor networks, low energy supplies drastically constrain sensors in terms of calculation and communication abilities. Designing processing algorithms at the sensor level that take into account these constraints is an important problem in this context. We study here the estimation of correlation functions between sensors using compressed acquisition and one-bit-quantization. The estimation is achieved directly using compressed samples, without considering any reconstruction of the signals. We show that if the signals of interest are far from white noise, estimation of the correlation using $M$ compressed samples out of $N\geq M$ can be more advantageous than estimation of the correlation using $M$ consecutive samples. The analysis consists of studying the asymptotic performance of the estimators at a fixed compression rate. We provide the analysis when the compression is realized by a random projection matrix composed of independent and identically distributed entries. The framework includes widely used random projection matrices, such as Gaussian and Bernoulli matrices, and it also includes very sparse matrices. However, it does not include subsampling without replacement, for which a separate analysis is provided. When considering one-bit-quantization as well, the theoretical analysis is not tractable. However, empirical evidence allows the conclusion that in practical situations, compressed and quantized estimators behave sufficiently correctly to be useful in, for example, time-delay estimation and model estimation.
[{'version': 'v1', 'created': 'Fri, 20 Nov 2015 15:29:35 GMT'}]
2015-11-23
[array(['Zebadua', 'Augusto', ''], dtype=object) array(['Amblard', 'Pierre-Olivier', ''], dtype=object) array(['Moisan', 'Eric', ''], dtype=object) array(['Michel', 'Olivier . J. J.', ''], dtype=object)]
1,054
1711.03715
Liming Yang
Liming Yang
Bounded Point Evaluations For Certain Polynomial And Rational Modules
null
Journal of Mathematical Analysis and Applications Volume 474, Issue 1, (2019), 219-241
null
null
math.FA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Let $K$ be a compact subset of the complex plane $\mathbb C.$ Let $P(K)$ and $R(K)$ be the closures in $C(K)$ of analytic polynomials and rational functions with poles off $K,$ respectively. Let $A(K) \subset C(K)$ be the algebra of functions that are analytic in the interior of $K$. For $1\le t <\infty,$ let $P^t(1, \phi_1,...,\phi_N,K)$ be the closure of $P(K)+P(K)\phi_1+...+P(K)\phi_N$ in $L^t(dA|_K),$ where $dA|_K$ is the area measure restricted to $K$ and $\phi_1,...,\phi_N\in L^t(dA|_K).$ Let $HP(\phi_1,...,\phi_N,K)$ be the closure of $P(K)\phi_1+...+P(K)\phi_N +R(K)$ in $C(K),$ where $\phi_1,...,\phi_N\in C(K).$ In this paper, we prove if $R(K)\ne C(K),$ then there exists an analytic bounded point evaluation for both $P^t(1, \phi_1,...,\phi_N,K)$ and $HP(\phi_1,...,\phi_N,K)$ for certain smooth functions $\phi_1,...,\phi_N,$ in particular, for $\bar z,\bar z^2,...,\bar z^N.$ We show that $A(K)\subset HP(\bar z,\bar z^2,...,\bar z^N,K)$ if and only if $R(K) = A(K).$ In particular, $C(K) \ne HP(\bar z,\bar z^2,...,\bar z^N,K)$ unless $R(K) = C(K).$ We also give an example of $K$ showing the results are not valid if we replace $\bar z^n$ by certain $\phi_n,$ that is, there exist $K$ and a function $\phi\in A(K)$ such that $R(K) \ne A(K),$ but $A(K) = HP (\phi ,K).$
[{'version': 'v1', 'created': 'Fri, 10 Nov 2017 07:13:36 GMT'}]
2019-03-21
[array(['Yang', 'Liming', ''], dtype=object)]
1,055
hep-th/9203067
Vincent G. J. Rodgers
Ralph Lano and V.G.J. Rodgers
Applications of W-algebras to BF theories, QCD and 4D Gravity
14 pages
Mod.Phys.Lett. A7 (1992) 1725-1736
10.1142/S0217732392001427
null
hep-th
null
We are able to show that BF theories naturally emerge from the coadjoint orbits of $W_2$ and $w_\infty$ algebras which includes a Kac-Moody sector. Since QCD strings can be identified with a BF theory, we are able to show a relationship between the orbits and monopole-string solutions of QCD. Furthermore, we observe that when 4D gravitation is cast into a BF form through the use of Ashtekar variables, we are able to get order $\hbar$ contributions to gravity which can be associated with the $W_2$ anomaly. We comment on the relationship to gravitational monopoles.
[{'version': 'v1', 'created': 'Wed, 25 Mar 1992 00:32:41 GMT'} {'version': 'v2', 'created': 'Wed, 25 Mar 1992 17:40:51 GMT'}]
2009-10-22
[array(['Lano', 'Ralph', ''], dtype=object) array(['Rodgers', 'V. G. J.', ''], dtype=object)]
1,056
1708.03563
Pieter Moree
Bernadette Faye, Florian Luca and Pieter Moree
On the discriminator of Lucas sequences
21 pages
Ann. Math. Qu\'ebec 43 (2019), 51--71
null
null
math.NT
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We consider the family of Lucas sequences uniquely determined by $U_{n+2}(k)=(4k+2)U_{n+1}(k) -U_n(k),$ with initial values $U_0(k)=0$ and $U_1(k)=1$ and $k\ge 1$ an arbitrary integer. For any integer $n\ge 1$ the discriminator function $\mathcal{D}_k(n)$ of $U_n(k)$ is defined as the smallest integer $m$ such that $U_0(k),U_1(k),\ldots,U_{n-1}(k)$ are pairwise incongruent modulo $m$. Numerical work of Shallit on $\mathcal{D}_k(n)$ suggests that it has a relatively simple characterization. In this paper we will prove that this is indeed the case by showing that for every $k\ge 1$ there is a constant $n_k$ such that ${\mathcal D}_{k}(n)$ has a simple characterization for every $n\ge n_k$. The case $k=1$ turns out to be fundamentally different from the case $k>1$.
[{'version': 'v1', 'created': 'Fri, 11 Aug 2017 14:53:49 GMT'}]
2020-08-27
[array(['Faye', 'Bernadette', ''], dtype=object) array(['Luca', 'Florian', ''], dtype=object) array(['Moree', 'Pieter', ''], dtype=object)]
1,057
2203.06536
Yulong Liu
Sishi Wu, Yulong Liu, Qichun Liu, Shuai-Peng Wang, Zhen Chen and Tiefu Li
Hybridized Frequency Combs in Multimode Cavity Electromechanical System
6 pages, 4 figures
Phys. Rev. Lett. 128, 153901 (2022)
10.1103/PhysRevLett.128.153901
null
quant-ph nlin.CD physics.atom-ph physics.optics
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The cavity electromechanical devices with radiation-pressure-interaction induced Kerr-like nonlinearity are promising candidates to generate microwave frequency combs. We construct a silicon-nitride-membrane-based superconducting cavity electromechanical device and study two mechanical modes mediated synergistic frequency combs. Around the threshold of intracavity field instability, we firstly show independent frequency combs with tooth spacing equalling to each mechanical mode frequency. At the overlap boundaries of these two individual mechanical mode mediated instability thresholds, we observe hybridization of frequency combs based on the cavity field mediated indirect coupling between these two mechanical modes. The spectrum lines turn to be unequally spaced but can be recognized into combinations of the coexisting frequency combs. Beyond the boundary, the comb reverts to the single-mode case, and which mechanical mode frequency will the tooth spacing depend on the mode competition. Our work demonstrates mechanical mode competition enabled switchability of frequency comb tooth spacing and can be extended to other devices with multiple nonlinearities.
[{'version': 'v1', 'created': 'Sat, 12 Mar 2022 23:56:08 GMT'}]
2022-04-14
[array(['Wu', 'Sishi', ''], dtype=object) array(['Liu', 'Yulong', ''], dtype=object) array(['Liu', 'Qichun', ''], dtype=object) array(['Wang', 'Shuai-Peng', ''], dtype=object) array(['Chen', 'Zhen', ''], dtype=object) array(['Li', 'Tiefu', ''], dtype=object)]
1,058
cond-mat/9703025
David A. Head
D.A.Head and G.J.Rodgers
Slowly Driven Sandpile Formation with Granular Mixtures
6 pages, RevTEX, 7 postscript figures and psfig.sty included
Phys. Rev. E 56, 1976 (1997).
10.1103/PhysRevE.56.1976
null
cond-mat.stat-mech
null
We introduce a one-dimensional sandpile model with $N$ different particle types and an infinitesimal driving rate. The parameters for the model are the N^2 critical slopes for one type of particle on top of another. The model is trivial when N=1, but for N=2 we observe four broad classes of sandpile structure in different regions of the parameter space. We describe and explain the behaviour of each of these classes, giving quantitative analysis wherever possible. The behaviour of sandpiles with N>2 essentially consists of combinations of these four classes. We investigate the model's robustness and highlight the key areas that any experiment designed to reproduce these results should focus on.
[{'version': 'v1', 'created': 'Mon, 3 Mar 1997 11:22:00 GMT'}]
2009-10-30
[array(['Head', 'D. A.', ''], dtype=object) array(['Rodgers', 'G. J.', ''], dtype=object)]
1,059
2103.10898
Markus Rademacher
Markus Rademacher, Michael Konopik, Maxime Debiossac, David Grass, Eric Lutz, Nikolai Kiesel
Nonequilibrium control of thermal and mechanical changes in a levitated system
null
Phys. Rev. Lett. 128, 070601 (2022)
10.1103/PhysRevLett.128.070601
null
cond-mat.stat-mech quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Fluctuation theorems are fundamental extensions of the second law of thermodynamics for small nonequilibrium systems. While work and heat are equally important forms of energy exchange, fluctuation relations have not been experimentally assessed for the generic situation of simultaneous mechanical and thermal changes. Thermal driving is indeed generally slow and more difficult to realize than mechanical driving. Here, we use feedback cooling techniques to implement fast and controlled temperature variations of an underdamped levitated microparticle that are one order of magnitude faster than the equilibration time. Combining mechanical and thermal control, we verify the validity of a fluctuation theorem that accounts for both contributions, well beyond the range of linear response theory. Our results allow the investigation of general far-from-equilibrium processes in microscopic systems that involve fast mechanical and thermal changes at the same time.
[{'version': 'v1', 'created': 'Fri, 19 Mar 2021 16:43:48 GMT'} {'version': 'v2', 'created': 'Tue, 24 Aug 2021 21:02:40 GMT'}]
2022-02-24
[array(['Rademacher', 'Markus', ''], dtype=object) array(['Konopik', 'Michael', ''], dtype=object) array(['Debiossac', 'Maxime', ''], dtype=object) array(['Grass', 'David', ''], dtype=object) array(['Lutz', 'Eric', ''], dtype=object) array(['Kiesel', 'Nikolai', ''], dtype=object)]
1,060
1004.2297
Gustavo Lima
G. Lima, E. S. G\'omez, A. Vargas, R. O. Vianna, and C. Saavedra
Fast entanglement detection for unknown states of two spatial qutrits
8 pages, 6 figures
Physical Review A 82, 012302 (2010)
10.1103/PhysRevA.82.012302
null
quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We investigate the practicality of the method proposed by Maciel et al. [Phys. Rev. A. 80, 032325(2009)] for detecting the entanglement of two spatial qutrits (3-dimensional quantum systems), which are encoded in the discrete transverse momentum of single photons transmitted through a multi-slit aperture. The method is based on the acquisition of partial information of the quantum state through projective measurements, and a data processing analysis done with semi-definite programs. This analysis relies on generating gradually an optimal entanglement witness operator, and numerical investigations have shown that it allows for the entanglement detection of unknown states with a cost much lower than full state tomography.
[{'version': 'v1', 'created': 'Wed, 14 Apr 2010 00:50:46 GMT'}]
2015-05-18
[array(['Lima', 'G.', ''], dtype=object) array(['Gómez', 'E. S.', ''], dtype=object) array(['Vargas', 'A.', ''], dtype=object) array(['Vianna', 'R. O.', ''], dtype=object) array(['Saavedra', 'C.', ''], dtype=object)]
1,061
2203.03542
Fatemah Husain
Fatemah Husain and Ozlem Uzuner
Fine-Tuning Approach for Arabic Offensive Language Detection System: BERT-Based Model
5 pages. Future Technologies and Innovations (FTI) Proceedings, 4th International Conference on Computer Applications and Information Security (ICCAIS 2021). arXiv admin note: substantial text overlap with arXiv:2102.05708
null
null
null
cs.CL
http://creativecommons.org/licenses/by/4.0/
The problem of online offensive language limits the health and security of online users. It is essential to apply the latest state-of-the-art techniques in developing a system to detect online offensive language and to ensure social justice to the online communities. Our study investigates the effects of fine-tuning across several Arabic offensive language datasets. We develop multiple classifiers that use four datasets individually and in combination in order to gain knowledge about online Arabic offensive content and classify users comments accordingly. Our results demonstrate the limited effects of transfer learning on the classifiers performance, particularly for highly dialectal comments.
[{'version': 'v1', 'created': 'Mon, 7 Feb 2022 17:26:35 GMT'}]
2022-03-08
[array(['Husain', 'Fatemah', ''], dtype=object) array(['Uzuner', 'Ozlem', ''], dtype=object)]
1,062
1811.07496
Satoko Sorahana
Satoko Sorahana, Tadashi Nakajima, and Yoshiki Matsuoka
Evaluation of the Vertical Scale Height of L dwarfs in the Galactic Thin Disk
32 pages, 9 figures, accepted for publication in ApJ
null
10.3847/1538-4357/aaf1a7
null
astro-ph.GA astro-ph.SR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Using the data release 1 of the Hyper Suprime-Cam Subaru Strategic Program covering about 130 square degrees at high galactic latitudes, we have obtained L dwarf counts based on the selection criteria on colors, limiting magnitude and PSF morphology using $i$, $z$, and $y$ bands. 3665 L dwarfs brighter than $z=24$ have been detected by these criteria. The surface number counts obtained differentially in $z$ magnitude are compared with predictions of an exponential disk model to estimate the thin-disk scale height in the vicinity of the Sun. In the exponential disk model, we first fix the local luminosity function (LLF) to the mean LLF of Cruz et al. (2007) and derive the best fit scale height of 260 pc. However this fit appears to be poor. We then allow the LLF to vary along with the scale height. We use the LLF of Cruz et al. as a starting point. The best-fit model is found for the vertical scale height of 380 pc. However the $\chi^2$ minimum is rather broad and the 90% confidence interval is between 320 and 520 pc. We investigate another model by varying the scale height and the density of the brightest magnitude bin, while other magnitude bins are fixed to the mean LLF of Cruz et al.. We find an equally good fit with the two free parameters and the best-fit scale height is again 380 pc, but the 90% confidence interval is between 340 and 420 pc.
[{'version': 'v1', 'created': 'Mon, 19 Nov 2018 04:38:05 GMT'}]
2019-01-23
[array(['Sorahana', 'Satoko', ''], dtype=object) array(['Nakajima', 'Tadashi', ''], dtype=object) array(['Matsuoka', 'Yoshiki', ''], dtype=object)]
1,063
0706.4403
Bertrand Eynard
Bertrand Eynard (SPhT)
Recursion between Mumford volumes of moduli spaces
Latex, 18 pages
null
null
SPHT-T07/104
math.AG hep-th math-ph math.MP
null
We propose a new proof, as well as a generalization of Mirzakhani's recursion for volumes of moduli spaces. We interpret those recursion relations in terms of expectation values in Kontsevich's integral, i.e. we relate them to a Ribbon graph decomposition of Riemann surfaces. We find a generalization of Mirzakhani's recursions to measures containing all higher Mumford's kappa classes, and not only kappa1 as in the Weil-Petersson case.
[{'version': 'v1', 'created': 'Fri, 29 Jun 2007 12:46:44 GMT'}]
2007-07-10
[array(['Eynard', 'Bertrand', '', 'SPhT'], dtype=object)]
1,064
1703.01420
Seyed Akbar Jafari
S. A. Jafari
Exact phase diagram and topological phase transitions of the XYZ spin chain
6 Figs
Phys. Rev. E 96 (2017) 012159
10.1103/PhysRevE.96.012159
null
cond-mat.str-el cond-mat.supr-con
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Within the block spin renormalization group we are able to construct the "exact" phase diagram of the XYZ spin chain. First we identify the Ising order along $\hat x$ or $\hat y$ as attractive renormalization group fixed points of the Kitaev chain. Then in a global phase space composed of the anisotropy $\lambda$ of the XY interaction and the coupling $\Delta$ of the $\Delta\sigma^z\sigma^z$ interaction we find that the above fixed points remain attractive in the two dimesional parameter space. We therefore classify the gapped phases of the XYZ spin chain as: (1) either attracted to the Ising limit of the Kitaev-chain which in turn is characterized by winding number $\pm 1$ depending whether the Ising order parameter is along $\hat x$ or $\hat y$ directions; or (2) attracted to the Mott phases of the underlying Jordan-Wigner fermions which is characterized by zero winding number. We therefore establish that the exact phase boundaries of the XYZ model in Baxter's solution indeed correspond to topological phase transitions. The topological nature of the phase transitions of the XYZ model justifies why our analytical solution of the three-site problem which is at the core of the renormalization group treatment is able to produce the exact phase diagram of Baxter's solution. We argue that the distribution of the winding numbers between the three Ising phases is a matter of choice of the coordinate system, and therefore the Mott-Ising phase is entitled to host apprpriate form of zero modes. We further observe that the renormalization group flow can be cast into a geometric progression of a properly identified parameter. We show that this new parameter is actually the size of the (Majorana) zero modes.
[{'version': 'v1', 'created': 'Sat, 4 Mar 2017 08:59:56 GMT'}]
2017-08-21
[array(['Jafari', 'S. A.', ''], dtype=object)]
1,065
math/0702591
Radford M. Neal
Longhai Li, Jianguo Zhang, and Radford M. Neal
A Method for Avoiding Bias from Feature Selection with Application to Naive Bayes Classification Models
null
null
null
null
math.ST stat.TH
null
For many classification and regression problems, a large number of features are available for possible use - this is typical of DNA microarray data on gene expression, for example. Often, for computational or other reasons, only a small subset of these features are selected for use in a model, based on some simple measure such as correlation with the response variable. This procedure may introduce an optimistic bias, however, in which the response variable appears to be more predictable than it actually is, because the high correlation of the selected features with the response may be partly or wholely due to chance. We show how this bias can be avoided when using a Bayesian model for the joint distribution of features and response. The crucial insight is that even if we forget the exact values of the unselected features, we should retain, and condition on, the knowledge that their correlation with the response was too small for them to be selected. In this paper we describe how this idea can be implemented for ``naive Bayes'' models of binary data. Experiments with simulated data confirm that this method avoids bias due to feature selection. We also apply the naive Bayes model to subsets of data relating gene expression to colon cancer, and find that correcting for bias from feature selection does improve predictive performance.
[{'version': 'v1', 'created': 'Tue, 20 Feb 2007 20:02:24 GMT'}]
2007-06-13
[array(['Li', 'Longhai', ''], dtype=object) array(['Zhang', 'Jianguo', ''], dtype=object) array(['Neal', 'Radford M.', ''], dtype=object)]
1,066
2303.13841
Sang-In Shim
Sang-In Shim, Kazuki Yoshida, Kazuyuki Ogata
Systematic analysis of the nuclear absorption effect on the cross section of the knockout reaction
8 pages, 4 figures
null
null
null
nucl-th
http://creativecommons.org/licenses/by/4.0/
Recent studies on nucleon and alpha knockout reactions have shown that the distorted-wave impulse approximation (DWIA) is a simple and accurate method to describe these reactions. As it has been argued for decades, the nuclear absorption is one of the most important ingredients of the DWIA calculation. In this work, we systematically investigate the absorption effects on the cross sections of the nucleon and alpha knockout reactions. To do this, we calculate the ratio of the cross sections of the DWIA and plane-wave impulse approximation (PWIA) and examine its dependence on the mass number and single-particle orbital of the knocked-out particles. We will discuss the specific characteristics of the absorption effect for each reaction.
[{'version': 'v1', 'created': 'Fri, 24 Mar 2023 07:34:05 GMT'} {'version': 'v2', 'created': 'Tue, 4 Jul 2023 09:52:27 GMT'}]
2023-07-06
[array(['Shim', 'Sang-In', ''], dtype=object) array(['Yoshida', 'Kazuki', ''], dtype=object) array(['Ogata', 'Kazuyuki', ''], dtype=object)]
1,067
1012.1311
Benjamin Beeker
Benjamin Beeker
Abelian JSJ decomposition of graphs of free abelian groups
19 pages, 6 figures
null
null
null
math.GR
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A group G is a vGBS group if it admits a decomposition as a finite graph of groups with all edge and vertex groups finitely generated and free abelian. We construct the JSJ decomposition of a vGBS group over abelian groups. We prove that this decomposition is explicitly computable, and may be obtained by local changes on the initial graph of groups.
[{'version': 'v1', 'created': 'Mon, 6 Dec 2010 20:57:03 GMT'}]
2010-12-07
[array(['Beeker', 'Benjamin', ''], dtype=object)]
1,068
1102.2186
A. V. Maccio'
J.C. Mu\~noz-Cuartas (AIP), Andrea V. Macci\`o (MPIA), Stefan Gottl\"ober (AIP), Aaron Dutton (UVic)
The Redshift Evolution of LCDM Halo Parameters
9 pages, 4 figures. Proceedings of CRF2010, DESY Hamburg, Nov 9-12 2010
null
null
null
astro-ph.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the mass and redshift dependence of the concentration parameter in Nbody simulations spanning masses from $10^{10} \hMsun$ to $10^{15} \hMsun$ and redshifts from 0 to 2. We present a series of fitting formulas that accurately describe the time evolution of the concentration-mass relation since z=2. Using arguments based on the spherical collapse model we study the behaviour of the scale length of the density profile during the assembly history of haloes, obtaining physical insights on the origin of the observed time evolution of the concentration mass relation. We present preliminary results of the implementation of this model in the prediction of the values of the concentration parameter for different masses and redshifts.
[{'version': 'v1', 'created': 'Thu, 10 Feb 2011 17:41:58 GMT'} {'version': 'v2', 'created': 'Fri, 11 Feb 2011 13:04:36 GMT'}]
2011-02-14
[array(['Muñoz-Cuartas', 'J. C.', '', 'AIP'], dtype=object) array(['Macciò', 'Andrea V.', '', 'MPIA'], dtype=object) array(['Gottlöber', 'Stefan', '', 'AIP'], dtype=object) array(['Dutton', 'Aaron', '', 'UVic'], dtype=object)]
1,069
0801.4198
Kazutaka Nakamura
Kazutaka Nakamura, Toshiyuki Tanaka
Microscopic Analysis for Decoupling Principle of Linear Vector Channel
null
null
null
null
cs.IT math.IT
null
This paper studies the decoupling principle of a linear vector channel, which is an extension of CDMA and MIMO channels. We show that the scalar-channel characterization obtained via the decoupling principle is valid not only for collections of a large number of elements of input vector, as discussed in previous studies, but also for individual elements of input vector, i.e. the linear vector channel for individual elements of channel input vector is decomposed into a bank of independent scalar Gaussian channels in the large-system limit, where dimensions of channel input and output are both sent to infinity while their ratio fixed.
[{'version': 'v1', 'created': 'Mon, 28 Jan 2008 06:59:42 GMT'}]
2008-01-29
[array(['Nakamura', 'Kazutaka', ''], dtype=object) array(['Tanaka', 'Toshiyuki', ''], dtype=object)]
1,070
1708.09395
Dean Robinson
Vladimir V. Gligorov, Simon Knapen, Michele Papucci, Dean J. Robinson
Searching for Long-lived Particles: A Compact Detector for Exotics at LHCb
12 pages, 8 figures, 2 tables; published version
Phys. Rev. D 97, 015023 (2018)
10.1103/PhysRevD.97.015023
null
hep-ph hep-ex
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We advocate for the construction of a new detector element at the LHCb experiment, designed to search for displaced decays of beyond standard model long-lived particles, taking advantage of a large shielded space in the LHCb cavern that is expected to soon become available. We discuss the general features and putative capabilities of such an experiment, as well as its various advantages and complementarities with respect to the existing LHC experiments and proposals such as SHiP and MATHUSLA. For two well-motivated beyond Standard Model benchmark scenarios -- Higgs decay to dark photons and $B$ meson decays via a Higgs mixing portal -- the reach either complements or exceeds that predicted for other LHC experiments.
[{'version': 'v1', 'created': 'Wed, 30 Aug 2017 18:00:02 GMT'} {'version': 'v2', 'created': 'Fri, 4 May 2018 13:59:00 GMT'}]
2018-05-07
[array(['Gligorov', 'Vladimir V.', ''], dtype=object) array(['Knapen', 'Simon', ''], dtype=object) array(['Papucci', 'Michele', ''], dtype=object) array(['Robinson', 'Dean J.', ''], dtype=object)]
1,071
2110.08644
Aleksander Stanislavsky A.
Aleksander A. Stanislavsky, Igor N. Bubnov, Artem A. Koval, Serge N. Yerin
Parker Solar Probe detects solar radio bursts related with a behind-the-limb active region
8 pages, 6 figures, 2 tables, accepted to be published in Astronomy and Astrophysics 2021
A&A 657, A21 (2022)
10.1051/0004-6361/202141984
null
astro-ph.SR physics.space-ph
http://creativecommons.org/licenses/by/4.0/
The interpretation of solar radio bursts observed by Parker Solar Probe (PSP) in the encounter phase plays a key role in understanding intrinsic properties of the emission mechanism in the solar corona. Lower time-frequency resolution of the PSP receiver can be overcome by simultaneous ground-based observations using more advanced antennas and receivers. In this paper we present such observations for which the active active region 12765, begetter of type III, J, and U solar bursts, was within sight of ground-based instruments and behind the solar limb of the PSP spacecraft. We used a subarray of the Giant Ukrainian Radio Telescope (GURT) to get the spectral properties of radio bursts at the frequency range of 8-80 MHz, as well as the PSP radio instruments with a bandwidth of 10.5 kHz - 19.2 MHz, during solar observations on June 5, 2020. We directly detected the radio events initiated by the active region behind the solar limb of the PSP spacecraft, using special conditions in the solar corona, due to the absence of active regions from the PSP side. Following the generation mechanism of solar radio emission, we refined the density model for the solar corona above the active region 12765 responsible for the radio bursts. Based on the PSP spacecraft position near the Sun and delays of radio waves between space- and ground-based records, we found the corresponding radio responses on the PSP spectrogram. The absence of sunspots from the PSP side contributes to the propagation of radio waves from a dense loop of the Sun to quiet regions with low densities, through which PSP instruments can detect the radiation.
[{'version': 'v1', 'created': 'Sat, 16 Oct 2021 19:18:05 GMT'}]
2021-12-22
[array(['Stanislavsky', 'Aleksander A.', ''], dtype=object) array(['Bubnov', 'Igor N.', ''], dtype=object) array(['Koval', 'Artem A.', ''], dtype=object) array(['Yerin', 'Serge N.', ''], dtype=object)]
1,072
1807.04742
Ashvin Nair
Ashvin Nair, Vitchyr Pong, Murtaza Dalal, Shikhar Bahl, Steven Lin, Sergey Levine
Visual Reinforcement Learning with Imagined Goals
15 pages, NeurIPS 2018
null
null
null
cs.LG cs.CV cs.RO stat.ML
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
For an autonomous agent to fulfill a wide range of user-specified goals at test time, it must be able to learn broadly applicable and general-purpose skill repertoires. Furthermore, to provide the requisite level of generality, these skills must handle raw sensory input such as images. In this paper, we propose an algorithm that acquires such general-purpose skills by combining unsupervised representation learning and reinforcement learning of goal-conditioned policies. Since the particular goals that might be required at test-time are not known in advance, the agent performs a self-supervised "practice" phase where it imagines goals and attempts to achieve them. We learn a visual representation with three distinct purposes: sampling goals for self-supervised practice, providing a structured transformation of raw sensory inputs, and computing a reward signal for goal reaching. We also propose a retroactive goal relabeling scheme to further improve the sample-efficiency of our method. Our off-policy algorithm is efficient enough to learn policies that operate on raw image observations and goals for a real-world robotic system, and substantially outperforms prior techniques.
[{'version': 'v1', 'created': 'Thu, 12 Jul 2018 17:51:16 GMT'} {'version': 'v2', 'created': 'Tue, 4 Dec 2018 08:44:08 GMT'}]
2018-12-05
[array(['Nair', 'Ashvin', ''], dtype=object) array(['Pong', 'Vitchyr', ''], dtype=object) array(['Dalal', 'Murtaza', ''], dtype=object) array(['Bahl', 'Shikhar', ''], dtype=object) array(['Lin', 'Steven', ''], dtype=object) array(['Levine', 'Sergey', ''], dtype=object)]
1,073
0908.3159
Gunter M. Ziegler
Thilo R\"orig, G\"unter M. Ziegler
Polyhedral Surfaces in Wedge Products
17 pages, 5 figures
null
null
null
math.MG math.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We introduce the wedge product of two polytopes. The wedge product is described in terms of inequality systems, in terms of vertex coordinates as well as purely combinatorially, from the corresponding data of its constituents. The wedge product construction can be described as an iterated ``subdirect product'' as introduced by McMullen (1976); it is dual to the ``wreath product'' construction of Joswig and Lutz (2005). One particular instance of the wedge product construction turns out to be especially interesting: The wedge products of polygons with simplices contain certain combinatorially regular polyhedral surfaces as subcomplexes. These generalize known classes of surfaces ``of unusually large genus'' that first appeared in works by Coxeter (1937), Ringel (1956), and McMullen, Schulz, and Wills (1983). Via ``projections of deformed wedge products'' we obtain realizations of some of the surfaces in the boundary complexes of 4-polytopes, and thus in R^3. As additional benefits our construction also yields polyhedral subdivisions for the interior and the exterior, as well as a great number of local deformations (``moduli'') for the surfaces in R^3. In order to prove that there are many moduli, we introduce the concept of ``affine support sets'' in simple polytopes. Finally, we explain how duality theory for 4-dimensional polytopes can be exploited in order to also realize combinatorially dual surfaces in R^3 via dual 4-polytopes.
[{'version': 'v1', 'created': 'Fri, 21 Aug 2009 16:07:26 GMT'}]
2009-08-24
[array(['Rörig', 'Thilo', ''], dtype=object) array(['Ziegler', 'Günter M.', ''], dtype=object)]
1,074
1306.6142
David A. Craig
David A. Craig and Parampreet Singh
Consistent probabilities in loop quantum cosmology
22 pages, 3 figures. Matches published version
Class. Quantum Grav. 30 (2013) 205008
10.1088/0264-9381/30/20/205008
PI-QG-249
gr-qc quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
A fundamental issue for any quantum cosmological theory is to specify how probabilities can be assigned to various quantum events or sequences of events such as the occurrence of singularities or bounces. In previous work, we have demonstrated how this issue can be successfully addressed within the consistent histories approach to quantum theory for Wheeler-DeWitt-quantized cosmological models. In this work, we generalize that analysis to the exactly solvable loop quantization of a spatially flat, homogeneous and isotropic cosmology sourced with a massless, minimally coupled scalar field known as sLQC. We provide an explicit, rigorous and complete decoherent histories formulation for this model and compute the probabilities for the occurrence of a quantum bounce vs. a singularity. Using the scalar field as an emergent internal time, we show for generic states that the probability for a singularity to occur in this model is zero, and that of a bounce is unity, complementing earlier studies of the expectation values of the volume and matter density in this theory. We also show from the consistent histories point of view that all states in this model, whether quantum or classical, achieve arbitrarily large volume in the limit of infinite `past' or `future' scalar `time', in the sense that the wave function evaluated at any arbitrary fixed value of the volume vanishes in that limit. Finally, we briefly discuss certain misconceptions concerning the utility of the consistent histories approach in these models.
[{'version': 'v1', 'created': 'Wed, 26 Jun 2013 06:50:58 GMT'} {'version': 'v2', 'created': 'Tue, 1 Oct 2013 05:31:23 GMT'}]
2013-10-02
[array(['Craig', 'David A.', ''], dtype=object) array(['Singh', 'Parampreet', ''], dtype=object)]
1,075
1507.08961
Matteo Semplice
Gabriella Puppo, Matteo Semplice, Andrea Tosin, Giuseppe Visconti
Kinetic models for traffic flow resulting in a reduced space of microscopic velocities
Replaced with revised version
Kinet. Relat. Models, 10(3):823-854, 2017
10.3934/krm.2017033
null
math.NA
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The purpose of this paper is to study the properties of kinetic models for traffic flow described by a Boltzmann-type approach and based on a continuous space of microscopic velocities. In our models, the particular structure of the collision kernel allows one to find the analytical expression of a class of steady-state distributions, which are characterized by being supported on a quantized space of microscopic speeds. The number of these velocities is determined by a physical parameter describing the typical acceleration of a vehicle and the uniqueness of this class of solutions is supported by numerical investigations. This shows that it is possible to have the full richness of a kinetic approach with the simplicity of a space of microscopic velocities characterized by a small number of modes. Moreover, the explicit expression of the asymptotic distribution paves the way to deriving new macroscopic equations using the closure provided by the kinetic model.
[{'version': 'v1', 'created': 'Fri, 31 Jul 2015 17:55:46 GMT'} {'version': 'v2', 'created': 'Fri, 10 Jun 2016 13:16:44 GMT'}]
2016-12-30
[array(['Puppo', 'Gabriella', ''], dtype=object) array(['Semplice', 'Matteo', ''], dtype=object) array(['Tosin', 'Andrea', ''], dtype=object) array(['Visconti', 'Giuseppe', ''], dtype=object)]
1,076
1109.0384
Andrew Smerald
Andrew Smerald and Nic Shannon
Angle-resolved NMR: quantitative theory of 75As T1 relaxation rate in BaFe2As2
18 pages, 10 figures
Phys. Rev. B 84, 184437 (2011)
10.1103/PhysRevB.84.184437
null
cond-mat.str-el
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
While NMR measurements of nuclear energy spectra are routinely used to characterize the static properties of quantum magnets, the dynamical information locked in NMR 1/T1 relaxation rates remains notoriously difficult to interpret. The difficulty arises from the fact that information about all possible low-energy spin excitations of the electrons, and their coupling to the nuclear moments, is folded into a single number, 1/T1. Here we develop a quantitative theory of the NMR 1/T1 relaxation rate in a collinear antiferromagnet, focusing on the specific example of BaFe2As2. One of the most striking features of magnetism in BaFe2As2 is a strong dependence of 1/T1 on the orientation of the applied magnetic field. By careful analysis of the coupling between the nuclear and electronic moments, we show how this anisotropy arises from the "filtering" of spin fluctuations by the form-factor for transferred hyperfine interactions. This allows us to make convincing, quantitative, fits to experimental 1/T1 data for BaFe2As2, for different field orientations. We go on to show how a quantitative, angle-dependent theory for the relaxation rate leads to new ways of measuring the dynamical parameters of magnetic systems, in particular the spin wave velocities.
[{'version': 'v1', 'created': 'Fri, 2 Sep 2011 09:00:08 GMT'} {'version': 'v2', 'created': 'Wed, 30 Nov 2011 10:37:58 GMT'}]
2011-12-01
[array(['Smerald', 'Andrew', ''], dtype=object) array(['Shannon', 'Nic', ''], dtype=object)]
1,077
hep-ph/0005118
Lee Jae Sik
Eri Asakawa, S.Y. Choi, and Jae Sik Lee
Probing the MSSM Higgs Boson Sector with Explicit CP Violation through Third Generation Fermion Pair Production at Muon Colliders
30 pages, 7 figures including 5 eps ones. Typos corrected and references added. To appear in Phys. Rev. D
Phys.Rev. D63 (2001) 015012
10.1103/PhysRevD.63.015012
KIAS-P00021, OCHA-PP-156
hep-ph
null
We perform a systematic study of the production of a third-generation fermion-pair, $\mu^+\mu^-\to f\bar{f}$ for $f=\tau^-,b$, and t in the minimal supersymmetric standard model (MSSM) with explicit CP violation, which is induced radiatively by soft trilinear interactions related to squarks of the third generation. We classify all the observables for probing the CP property of the Higgs bosons constructed by the initial muon beam polarization along with the unpolarized final fermions and with the final-fermion polarization configuration of equal helicity, respectively. The observables allow for complete determination of CP property of the neutral Higgs bosons. The interference between the Higgs boson and gauge boson contributions also could provide a powerful method for the determination of the CP property of two heavy Higgs bosons in the top-quark pair production near the energy region of the Higgs-boson resonances. For the lightest Higgs-boson mass there is no sizable interference between scalar and vector contributions for the determination of the CP property of the lightest Higgs boson. We give a detailed numerical analysis to show how the radiatively-induced CP violation in the Higgs sector of the MSSM can be measured.
[{'version': 'v1', 'created': 'Fri, 12 May 2000 03:47:41 GMT'} {'version': 'v2', 'created': 'Tue, 1 Aug 2000 06:18:10 GMT'} {'version': 'v3', 'created': 'Thu, 5 Oct 2000 02:50:48 GMT'}]
2009-10-31
[array(['Asakawa', 'Eri', ''], dtype=object) array(['Choi', 'S. Y.', ''], dtype=object) array(['Lee', 'Jae Sik', ''], dtype=object)]
1,078
0904.1872
Joshua Feinberg
Joshua Feinberg
Statistics of Resonances in One Dimensional Continuous Systems
latex, 8 pages, no figures; original material, based on an invited lecture at the Homi Bhabha Centenary conference on "Non-Hermitian operators in quantum physics", Bhaba Atomic Research Center, Mumbai, January 2009
null
10.1007/s12043-009-0108-6
null
cond-mat.dis-nn hep-th math-ph math.MP quant-ph
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the average density of resonances (DOR) of a disordered one-dimensional continuous open system. The disordered system is semi-infinite, with white-noise random potential, and it is coupled to the external world by a semi-infinite continuous perfect lead. Our main result is an integral representation for the DOR which involves the probability density function of the logarithmic derivative of the wave function at the contact point.
[{'version': 'v1', 'created': 'Sun, 12 Apr 2009 15:18:13 GMT'}]
2015-05-13
[array(['Feinberg', 'Joshua', ''], dtype=object)]
1,079
funct-an/9312005
Ya. Alber
Ya. I. Alber
The Penalty Method for Variational Inequalities with Nonsmooth Unbounded Operators in Banach Space
14 pages, LaTex
null
null
null
funct-an math.FA
null
The existence of a solution, convergence and stability of the penalty method for variational inequalities with nonsmooth unbounded uniformly and properly monotone operators in Banach spase $B$ are investigated. All the objects of the inequality - the operator A, "the right-hand part" $f$ and the set of constrains $\Omega $ - are to be perturbed. The stability theorems are formulated in terms of geometric characteristics of the spaces $B$ and $B^*$. The results of this paper are continuity and generalization of the Lions' ones, published earlier in \cite{l}. They are new even in Hilbert spaces.
[{'version': 'v1', 'created': 'Wed, 29 Dec 1993 16:21:10 GMT'}]
2008-02-03
[array(['Alber', 'Ya. I.', ''], dtype=object)]
1,080
1601.02449
Lilia Anguelova
Lilia Anguelova
Glueball Inflation and Gauge/Gravity Duality
9 pages, contribution to the proceedings of the 11th international workshop "Lie Theory and its Applications in Physics", Varna, 2015
Springer Proc. Math. Stat. 191 (2016) 285-293
null
null
hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We summarize our work on building glueball inflation models with the methods of the gauge/gravity duality. We review the relevant five-dimensional consistent truncation of type IIB supergravity. We consider solutions of this effective theory, whose metric has the form of a $dS_4$ foliation over a radial direction. By turning on small (in an appropriate sense) time-dependent deformations around these solutions, one can build models of glueball inflation. We discuss a particular deformed solution, describing an ultra-slow roll inflationary regime.
[{'version': 'v1', 'created': 'Mon, 11 Jan 2016 14:02:56 GMT'}]
2017-03-20
[array(['Anguelova', 'Lilia', ''], dtype=object)]
1,081
1301.5788
Tapan Chatterji
Tapan Chatterji, Mohamed Zbiri, Stephane Rols
Phonon-Magnon coupling in CoF$_2$ investigated by time-of-flight neutron spectroscopy
null
Solid State Communication 174, 55 (2013)
10.1016/j.ssc.2013.08.012
null
cond-mat.mtrl-sci
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We report the results of inelastic neutron scattering investigation on the model antiferromagnet CoF$_2$ by time-of-flight neutron spectroscopy. We measured the details of the scattering function $S(Q,\omega)$ as a function of temperature with two different incident neutron wavelengths. The temperature and Q dependence of the measured scattering function suggests the presence of magnon-phonon coupling in almost all branches. The present results are in agreement with the strong magnetoelastic effects observed previously.
[{'version': 'v1', 'created': 'Thu, 24 Jan 2013 14:22:40 GMT'}]
2015-06-12
[array(['Chatterji', 'Tapan', ''], dtype=object) array(['Zbiri', 'Mohamed', ''], dtype=object) array(['Rols', 'Stephane', ''], dtype=object)]
1,082
2303.07526
Alois Schiessl
Alois Schiessl
Just another solution to the Basel Problem
3 pages
null
null
null
math.HO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The Basel problem consists in finding the sum of the reciprocals of the squares of the positive integers. It was finally solved in 1735 by Leonhard Euler. In this paper, we propose a simple proof based on the Weierstrass Sine product formula and L'H\^opital's rule.
[{'version': 'v1', 'created': 'Mon, 13 Mar 2023 23:27:44 GMT'}]
2023-03-15
[array(['Schiessl', 'Alois', ''], dtype=object)]
1,083
1312.1617
Fei Yang
Fei Yang and Jinsong Zeng
On the dynamics of a family of renormalization transformations
21 pages, 5 figures, to appear in J. Math. Anal. Appl
null
10.1016/j.jmaa.2013.11.068
null
math.DS math.CV
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study the family of renormalization transformations of the generalized $d$--dimensional diamond hierarchical Potts model in statistical mechanic and prove that their Julia sets and non-escaping loci are always connected, where $d\geq 2$. In particular, we prove that their Julia sets can never be a Sierpi\'{n}ski carpet if the parameter is real. We show that the Julia set is a quasicircle if and only if the parameter lies in the unbounded capture domain of these models. Moreover, the asymptotic formula of the Hausdorff dimension of the Julia set is calculated as the parameter tends to infinity.
[{'version': 'v1', 'created': 'Thu, 5 Dec 2013 17:03:34 GMT'}]
2013-12-06
[array(['Yang', 'Fei', ''], dtype=object) array(['Zeng', 'Jinsong', ''], dtype=object)]
1,084
1007.3737
Chang-Soon Park
Hirosi Ooguri and Chang-Soon Park
Holographic End-Point of Spatially Modulated Phase Transition
21 pages, 22 figures. v2: a note and a reference added
Phys.Rev.D82:126001,2010
10.1103/PhysRevD.82.126001
CALT-68-2796, IPMU10-0110
hep-th cond-mat.str-el gr-qc
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In the previous paper [arXiv:0911.0679], we showed that the Reissner-Nordstrom black hole in the 5-dimensional anti-de Sitter space coupled to the Maxwell theory with the Chern-Simons term is unstable when the Chern-Simons coupling is sufficiently large. In the dual conformal field theory, the instability suggests a spatially modulated phase transition. In this paper, we construct and analyze non-linear solutions which describe the end-point of this phase transition. In the limit where the Chern-Simons coupling is large, we find that the phase transition is of the second order with the mean field critical exponent. However, the dispersion relation with the Van Hove singularity enhances quantum corrections in the bulk, and we argue that this changes the order of the phase transition from the second to the first. We compute linear response functions in the non-linear solution and find an infinite off-diagonal DC conductivity in the new phase.
[{'version': 'v1', 'created': 'Wed, 21 Jul 2010 20:00:03 GMT'} {'version': 'v2', 'created': 'Mon, 30 Aug 2010 20:25:18 GMT'}]
2010-12-24
[array(['Ooguri', 'Hirosi', ''], dtype=object) array(['Park', 'Chang-Soon', ''], dtype=object)]
1,085
1402.0893
Marco Moretti Sala
M. Moretti Sala, K. Ohgushi, A. Al-Zein, Y. Hirata, G. Monaco and M. Krisch
CaIrO3: a Spin-Orbit Mott Insulator Beyond the jeff = 1/2 Ground State
5 pages, 4 figures
Phys. Rev. Lett. 112, 176402 (2014)
10.1103/PhysRevLett.112.176402
null
cond-mat.str-el
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In CaIrO3 electronic correlation, spin-orbit coupling, and tetragonal crystal field splitting are predicted to be of comparable strength. However, the nature of its ground state is still object of debate, with contradictory experimental and theoretical results. We probe the ground state of CaIrO3 and assess the effective tetragonal crystal field splitting and spin-orbit coupling at play in this system by means of resonant inelastic x-ray scattering. We conclude that insulating CaIrO3 is not a jeff = 1/2 iridate and discuss the consequences of our finding to the interpretation of previous experiments. In particular, we clarify how the Mott insulating state in iridates can be readily extended beyond the jeff = 1/2 ground state.
[{'version': 'v1', 'created': 'Tue, 4 Feb 2014 21:53:58 GMT'}]
2014-05-02
[array(['Sala', 'M. Moretti', ''], dtype=object) array(['Ohgushi', 'K.', ''], dtype=object) array(['Al-Zein', 'A.', ''], dtype=object) array(['Hirata', 'Y.', ''], dtype=object) array(['Monaco', 'G.', ''], dtype=object) array(['Krisch', 'M.', ''], dtype=object)]
1,086
2012.05287
Sophie Spirkl
Maria Chudnovsky, Alex Scott, Paul Seymour, Sophie Spirkl
A note on simplicial cliques
Accepted manuscript; see DOI for journal version
Discrete Mathematics, Volume 344, Issue 9, September 2021, 112470
10.1016/j.disc.2021.112470
null
math.CO
http://creativecommons.org/licenses/by-nc-nd/4.0/
Motivated by an application in condensed matter physics and quantum information theory, we prove that every non-null even-hole-free claw-free graph has a simplicial clique, that is, a clique $K$ such that for every vertex $v \in K$, the set of neighbours of $v$ outside of $K$ is a clique. In fact, we prove the existence of a simplicial clique in a more general class of graphs defined by forbidden induced subgraphs.
[{'version': 'v1', 'created': 'Wed, 9 Dec 2020 19:55:23 GMT'} {'version': 'v2', 'created': 'Fri, 1 Oct 2021 16:11:41 GMT'}]
2021-10-04
[array(['Chudnovsky', 'Maria', ''], dtype=object) array(['Scott', 'Alex', ''], dtype=object) array(['Seymour', 'Paul', ''], dtype=object) array(['Spirkl', 'Sophie', ''], dtype=object)]
1,087
2304.11932
Philippe Schnoebelen
Philippe Schnoebelen and Julien Veron
On arch factorization and subword universality for words and compressed words
Accepted for publication in Proc. 14th Int. Conf. Combinatorics on Words (WORDS 2023)
null
null
null
cs.FL
http://creativecommons.org/licenses/by-nc-nd/4.0/
Using arch-jumping functions and properties of the arch factorization of words, we propose a new algorithm for computing the subword circular universality index of words. We also introduce the subword universality signature for words, that leads to simple algorithms for the universality indexes of SLP-compressed words.
[{'version': 'v1', 'created': 'Mon, 24 Apr 2023 09:17:37 GMT'}]
2023-04-25
[array(['Schnoebelen', 'Philippe', ''], dtype=object) array(['Veron', 'Julien', ''], dtype=object)]
1,088
2103.10111
Misa Ogata
Misa Ogata, Ryosuke Hirai, Kotaro Hijikawa
Observability of inflated companion stars after supernovae in massive binaries
15 pages, 15 figures, Accepted for publication in MNRAS
null
10.1093/mnras/stab1439
null
astro-ph.SR astro-ph.HE
http://creativecommons.org/licenses/by/4.0/
We carry out a systematic study of the response of companion stars in massive binaries after being impacted by supernova ejecta. A total of 720 1D stellar evolution calculations are performed to follow the inflation and contraction of the star in response to the energy injection and how it depends on various parameters. We find that the maximum luminosity achieved during the inflated phase is only dependent on the stellar mass and we derive an analytic formula to describe the relation. There is also a tight correlation between the duration of expansion and the intersected energy. These correlations will be useful to constrain pre-supernova binary parameters from future detections of inflated companions. We also discuss the possible outcomes of the binary system when the companion inflation is taken into account. Based on simple binary population synthesis, we estimate that $\sim$1-3% of stripped-envelope supernovae may have observable inflated companions. Finally, we apply our models to the observed companion of SN2006jc and place strong constraints on the possible pre-supernova binary parameters.
[{'version': 'v1', 'created': 'Thu, 18 Mar 2021 09:37:19 GMT'} {'version': 'v2', 'created': 'Thu, 27 May 2021 11:22:36 GMT'}]
2021-05-28
[array(['Ogata', 'Misa', ''], dtype=object) array(['Hirai', 'Ryosuke', ''], dtype=object) array(['Hijikawa', 'Kotaro', ''], dtype=object)]
1,089
hep-ph/9705381
Jiri Chyla
Jiri Chyla, Jiri Rames
Jet rates in deep inelastic scattering: wherefrom comes the sensitivity to \alpha_s?
13 pages, Latex with macro for Zhys. C., 6 figures in PS format attached, to be published in ZPhys. C
null
null
PRA-HEP/97-7
hep-ph
null
For theoretically consistent determination of $\alpha_s$ from jet rates in deep inelastic scattering the dependence on $\alpha_s$ of parton distribution functions is in principle as important as that of hard scattering cross-sections. For the kinematical region accessible at HERA we investigate in detail numerical importance of these two sources of the $\alpha_s$ dependence of jet rates.
[{'version': 'v1', 'created': 'Wed, 21 May 1997 15:48:09 GMT'}]
2007-05-23
[array(['Chyla', 'Jiri', ''], dtype=object) array(['Rames', 'Jiri', ''], dtype=object)]
1,090
1502.01733
Othman Soufan
Othman Soufan and Samer Arafat
Arrhythmia Detection using Mutual Information-Based Integration Method
6 pages, 1 figure, 7 tables, WConSC 2011 conference http://www.ece.ualberta.ca/~reform/WConSC/ (2011)
null
null
null
cs.CE cs.LG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
The aim of this paper is to propose an application of mutual information-based ensemble methods to the analysis and classification of heart beats associated with different types of Arrhythmia. Models of multilayer perceptrons, support vector machines, and radial basis function neural networks were trained and tested using the MIT-BIH arrhythmia database. This research brings a focus to an ensemble method that, to our knowledge, is a novel application in the area of ECG Arrhythmia detection. The proposed classifier ensemble method showed improved performance, relative to either majority voting classifier integration or to individual classifier performance. The overall ensemble accuracy was 98.25%.
[{'version': 'v1', 'created': 'Thu, 5 Feb 2015 21:31:25 GMT'}]
2015-02-09
[array(['Soufan', 'Othman', ''], dtype=object) array(['Arafat', 'Samer', ''], dtype=object)]
1,091
1404.1525
John Goodrick
John Goodrick, Byunghan Kim, and Alexei Kolesnikov
Type-amalgamation properties and polygroupoids in stable theories
37 pages
null
null
null
math.LO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We show that in a stable first-order theory, the failure of higher-dimensional type amalgamation can always be witnessed by algebraic structures which we call n-ary polygroupoids. This generalizes a result of Hrushovski that failures of 4-amalgamation in stable theories are witnessed by definable groupoids (which are 2-ary polygroupoids in our terminology). The n-ary polygroupoids are definable in a mild expansion of the language (adding a unary predicate for an infinite Morley sequence).
[{'version': 'v1', 'created': 'Sat, 5 Apr 2014 22:21:44 GMT'}]
2014-04-08
[array(['Goodrick', 'John', ''], dtype=object) array(['Kim', 'Byunghan', ''], dtype=object) array(['Kolesnikov', 'Alexei', ''], dtype=object)]
1,092
1111.2559
Jose I. Liberati
Carina Boyallian and Jos\'e I. Liberati
On pseudo-bialgebras
arXiv admin note: substantial text overlap with arXiv:math/0007121
null
null
null
math.QA math-ph math.MP
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
We study pseudoalgebras from the point of view of pseudo-dual of classical Lie coalgebra structures. We define the notions of Lie H-coalgebra and Lie pseudo-bialgebra. We obtain the analog of the CYBE, the Manin triples and Drinfeld's double for Lie pseudo-bialgebras. We also get a natural description of the annihilation algebra associated to a pseudoalgebra as a convolution algebra, clarifying this constructions in the theory of pseudoalgebras.
[{'version': 'v1', 'created': 'Thu, 10 Nov 2011 18:58:24 GMT'}]
2011-11-11
[array(['Boyallian', 'Carina', ''], dtype=object) array(['Liberati', 'José I.', ''], dtype=object)]
1,093
2305.11996
Su-Kyoung Kim
Niklas Kueper, Kartik Chari, Judith B\"utef\"ur, Julia Habenicht, Su Kyoung Kim, Tobias Rossol, Marc Tabie, Frank Kirchner, and Elsa Andrea Kirchner
EEG and EMG dataset for the detection of errors introduced by an active orthosis device
Revised references to our datasets, general corrections to typos, and latex template format changes, Overall Content unchanged
null
null
null
cs.HC cs.AI cs.RO
http://creativecommons.org/licenses/by/4.0/
This paper presents a dataset containing recordings of the electroencephalogram (EEG) and the electromyogram (EMG) from eight subjects who were assisted in moving their right arm by an active orthosis device. The supported movements were elbow joint movements, i.e., flexion and extension of the right arm. While the orthosis was actively moving the subject's arm, some errors were deliberately introduced for a short duration of time. During this time, the orthosis moved in the opposite direction. In this paper, we explain the experimental setup and present some behavioral analyses across all subjects. Additionally, we present an average event-related potential analysis for one subject to offer insights into the data quality and the EEG activity caused by the error introduction. The dataset described herein is openly accessible. The aim of this study was to provide a dataset to the research community, particularly for the development of new methods in the asynchronous detection of erroneous events from the EEG. We are especially interested in the tactile and haptic-mediated recognition of errors, which has not yet been sufficiently investigated in the literature. We hope that the detailed description of the orthosis and the experiment will enable its reproduction and facilitate a systematic investigation of the influencing factors in the detection of erroneous behavior of assistive systems by a large community.
[{'version': 'v1', 'created': 'Fri, 19 May 2023 20:42:28 GMT'} {'version': 'v2', 'created': 'Thu, 25 May 2023 10:33:50 GMT'}]
2023-05-26
[array(['Kueper', 'Niklas', ''], dtype=object) array(['Chari', 'Kartik', ''], dtype=object) array(['Bütefür', 'Judith', ''], dtype=object) array(['Habenicht', 'Julia', ''], dtype=object) array(['Kim', 'Su Kyoung', ''], dtype=object) array(['Rossol', 'Tobias', ''], dtype=object) array(['Tabie', 'Marc', ''], dtype=object) array(['Kirchner', 'Frank', ''], dtype=object) array(['Kirchner', 'Elsa Andrea', ''], dtype=object)]
1,094
cond-mat/0210333
Yukitoshi Motome
Nobuo Furukawa and Yukitoshi Motome
Spin-wave Hamiltonian in double-exchange systems
2 pages, to be published in Physica B (Proc. to LT23)
Physica B: Cond. Matter 329-333, 759 (2003)
10.1016/S0921-4526(02)02503-6
null
cond-mat.str-el cond-mat.stat-mech
null
A simple derivation of the effective spin-wave Hamiltonian for a double-exchange system with infinitely large Hund's-rule coupling is demonstrated. The formalism can be applied to models with arbitrary range of hopping as well as those with randomness. The result shows that, within the leading order of the 1/S expansion, one magnon excitation spectrum can be described by the Heisenberg model.
[{'version': 'v1', 'created': 'Tue, 15 Oct 2002 22:29:46 GMT'}]
2007-05-23
[array(['Furukawa', 'Nobuo', ''], dtype=object) array(['Motome', 'Yukitoshi', ''], dtype=object)]
1,095
1906.02883
Liwei Zhang
Xiaoying Dai and Liwei Zhang and Aihui Zhou
Adaptive Step Size Strategy for Orthogonality Constrained Line Search Methods
27 pages, 5 figures, 4 tables
null
null
null
math.OC
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In this paper, we propose an adaptive step size strategy for a class of line search methods for orthogonality constrained minimization problems, which avoids the classic backtracking procedure. We prove the convergence of the line search methods equipped with our adaptive step size strategy under some mild assumptions.We then apply the adaptive algorithm to electronic structure calculations, which show that our strategy is efficient and recommended.
[{'version': 'v1', 'created': 'Fri, 7 Jun 2019 03:21:02 GMT'} {'version': 'v2', 'created': 'Thu, 20 Feb 2020 07:24:47 GMT'}]
2020-02-21
[array(['Dai', 'Xiaoying', ''], dtype=object) array(['Zhang', 'Liwei', ''], dtype=object) array(['Zhou', 'Aihui', ''], dtype=object)]
1,096
2302.07549
Mila Nambiar
Milashini Nambiar and Supriyo Ghosh and Priscilla Ong and Yu En Chan and Yong Mong Bee and Pavitra Krishnaswamy
Deep Offline Reinforcement Learning for Real-world Treatment Optimization Applications
null
null
null
null
cs.LG
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
There is increasing interest in data-driven approaches for recommending optimal treatment strategies in many chronic disease management and critical care applications. Reinforcement learning methods are well-suited to this sequential decision-making problem, but must be trained and evaluated exclusively on retrospective medical record datasets as direct online exploration is unsafe and infeasible. Despite this requirement, the vast majority of treatment optimization studies use off-policy RL methods (e.g., Double Deep Q Networks (DDQN) or its variants) that are known to perform poorly in purely offline settings. Recent advances in offline RL, such as Conservative Q-Learning (CQL), offer a suitable alternative. But there remain challenges in adapting these approaches to real-world applications where suboptimal examples dominate the retrospective dataset and strict safety constraints need to be satisfied. In this work, we introduce a practical and theoretically grounded transition sampling approach to address action imbalance during offline RL training. We perform extensive experiments on two real-world tasks for diabetes and sepsis treatment optimization to compare performance of the proposed approach against prominent off-policy and offline RL baselines (DDQN and CQL). Across a range of principled and clinically relevant metrics, we show that our proposed approach enables substantial improvements in expected health outcomes and in accordance with relevant practice and safety guidelines.
[{'version': 'v1', 'created': 'Wed, 15 Feb 2023 09:30:57 GMT'} {'version': 'v2', 'created': 'Tue, 13 Jun 2023 12:24:32 GMT'}]
2023-06-14
[array(['Nambiar', 'Milashini', ''], dtype=object) array(['Ghosh', 'Supriyo', ''], dtype=object) array(['Ong', 'Priscilla', ''], dtype=object) array(['Chan', 'Yu En', ''], dtype=object) array(['Bee', 'Yong Mong', ''], dtype=object) array(['Krishnaswamy', 'Pavitra', ''], dtype=object)]
1,097
1607.03598
Bikash Bhattacharjya
Hiranmoy Pal, Bikash Bhattacharjya
Pretty Good State Transfer on Circulant Graphs
null
The Electronic Journal of Combinatorics, 24(2): P2.23 (2017)
null
null
math.CO
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Let $G$ be a graph with adjacency matrix $A$. The transition matrix of $G$ relative to $A$ is defined by $H(t):=\exp{\left(-itA\right)},\;t\in\Rl$. The graph $G$ is said to admit pretty good state transfer between a pair of vertices $u$ and $v$ if there exists a sequence of real numbers $\{t_k\}$ and a complex number $\gamma$ of unit modulus such that $\lim\limits_{k\rightarrow\infty} H(t_k) e_u=\gamma e_v.$ We find that pretty good state transfer occurs in a cycle on $n$ vertices if and only if $n$ is a power of two and it occurs between every pair of antipodal vertices. In addition, we look for pretty good state transfer in more general circulant graphs. We prove that union (edge disjoint) of an integral circulant graph with a cycle, each on $2^k$ $(k\geq 3)$ vertices, admits pretty good state transfer. The complement of such union also admits pretty good state transfer. This enables us to find some non-circulant graphs admitting pretty good state transfer. Among the complement of cycles we also find a class of graphs not exhibiting pretty good state transfer.
[{'version': 'v1', 'created': 'Wed, 13 Jul 2016 06:04:17 GMT'}]
2019-01-08
[array(['Pal', 'Hiranmoy', ''], dtype=object) array(['Bhattacharjya', 'Bikash', ''], dtype=object)]
1,098
1312.4916
Marco Schreck MS
M. Schreck
Quantum field theoretic properties of Lorentz-violating operators of nonrenormalizable dimension in the photon sector
25 pages, 2 figures
Phys. Rev. D 89, 105019 (2014)
10.1103/PhysRevD.89.105019
null
hep-th
http://arxiv.org/licenses/nonexclusive-distrib/1.0/
In the context of the nonminimal Standard-Model Extension a special subset of the CPT-even higher-dimensional operators in the photon sector is discussed from a quantum-field theoretical point of view. The modified dispersion laws, photon polarization vectors plus the gauge field propagator are obtained and their properties are analyzed. It is demonstrated that for certain sectors of the modified theory a puzzle arises for the optical theorem at tree-level. This is followed by a discussion of how it can be interpreted and resolved at first order Lorentz violation. Furthermore the commutator of two gauge fields that are evaluated at different spacetime points is obtained and discussed. The structure of the theory is shown to resemble the structure of the modification based on the corresponding dimension-4 operator. However some properties are altered due to the nonrenormalizable nature of the theory considered. The results provide more insight into the characteristics of Lorentz-violating quantum field theories that rest upon contributions of nonrenormalizable dimension.
[{'version': 'v1', 'created': 'Tue, 17 Dec 2013 19:53:17 GMT'}]
2014-05-28
[array(['Schreck', 'M.', ''], dtype=object)]
1,099
2211.00231
Bo-Qiang Ma
Yanqi Huang, Bo-Qiang Ma
Ultra-high energy cosmic neutrinos from gamma-ray bursts
8 latex pages, 3 figures, final version for journal publication
null
10.1016/j.fmre.2022.05.022
null
astro-ph.HE gr-qc hep-ph
http://creativecommons.org/licenses/by/4.0/
Based on recent proposal to associate IceCube TeV and PeV neutrino events with gamma-ray bursts~(GRBs) by considering the Lorentz violation of neutrinos, we provide a new estimate on the GRB neutrino flux and such result is much bigger than previous results by the IceCube Collaboration. Among these 24 neutrino ``shower" events above 60~TeV, 12 events are associated with GRBs. Such result is comparable with the prediction from GRB fireball models. Analysis of track events provide consistent result with the shower events to associate high energy cosmic neutrinos with GRBs under the same Lorentz violation features of neutrinos. We also make a background estimation and reveal GRBs as a significant source for the ultra-high energy IceCube neutrino events. Our work supports the Lorentz violation and $CPT$-violation of neutrinos, indicating new physics beyond relativity.
[{'version': 'v1', 'created': 'Tue, 1 Nov 2022 02:36:59 GMT'} {'version': 'v2', 'created': 'Fri, 4 Nov 2022 14:23:41 GMT'}]
2022-11-07
[array(['Huang', 'Yanqi', ''], dtype=object) array(['Ma', 'Bo-Qiang', ''], dtype=object)]