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Astrophysics > High Energy Astrophysical Phenomena

arXiv:2108.00560 (astro-ph)
[Submitted on 29 Jul 2021 (v1), last revised 9 Oct 2021 (this version, v2)]

Title:Revisiting the post-glitch relaxation of the 2000 Vela glitch with the neutron star equation of states in the Brueckner and relativistic Brueckner theories

Authors:Xinle Shang, Ang Li
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Abstract:We revisit the short-term post-glitch relaxation of the Vela 2000 glitch in the simple two-component model of pulsar glitch by making use of the latest realistic equations of states from the microscopic Brueckner and the relativistic Brueckner theories for neutron stars, which can reconcile with the available astrophysical constraints. We show that to fit both the glitch size and the post-glitch jumps in frequency derivatives approximately one minute after the glitch, the mass of the Vela pulsar is necessarily small, and there may be demands for a stiff equation of state (which results in a typical stellar radius larger than $\sim\negthickspace12.5\,\rm km$) and a strong suppression of the pairing gap in the nuclear medium. We discuss the implications of this result on the understanding of pulsar glitches.
Comments: 13 pages, 5 figures, 1 table, version accepted for publication in ApJ
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE); General Relativity and Quantum Cosmology (gr-qc); Nuclear Theory (nucl-th)
Cite as: arXiv:2108.00560 [astro-ph.HE]
  (or arXiv:2108.00560v2 [astro-ph.HE] for this version)
  https://doi.org/10.48550/arXiv.2108.00560
Journal reference: 2021 ApJ 923, 108
Related DOI: https://doi.org/10.3847/1538-4357/ac2e94

Submission history

From: Ang Li [view email]
[v1] Thu, 29 Jul 2021 09:01:31 UTC (612 KB)
[v2] Sat, 9 Oct 2021 05:33:09 UTC (624 KB)
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