Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Pulsar glitch and nuclear EoS: Applicability of superfluid model   In this contribution, we have made use of the contemporary equation of states
(EOSs) for the complete neutron star structure, and confronted them with one
particular glitch constrain for the crustal moment of inertia (MOI). We find
that with these EOSs, the radii of three millisecond pulsars selected by NICER:
PSR J0437-4715, PSR J1614-2230, PSR J0751+1807, are all around 12.5 km. Also, a
star with $M \lesssim 1.55 M_{\odot}$ would fulfill the MOI calculation for
glitch constrain with the latest neutron superfluidity density, and the glitch
crisis might not be present.

10
The categories of this paper are: q-bio
28
The categories of this paper are: alg-geom
2
The categories of this paper are: math
37
The categories of this paper are: supr-con
32
The categories of this paper are: atom-ph
21
The categories of this paper are: adap-org
15
The categories of this paper are: nucl-ex
7
The categories of this paper are: hep-th
26
The categories of this paper are: bayes-an
30
The categories of this paper are: q-alg
20
The categories of this paper are: acc-phys
8
The categories of this paper are: hep-ex
3
The categories of this paper are: physics
4
The categories of this paper are: cond-mat
16
The categories of this paper are: stat
0
The categories of this paper are: hep-ph