vix.ing · top · new · best · stats

Two types of glitches in a solid quark star model

2015/12/11 by J. G. Lu, Jiguang Lu, Enping Zhou +3
Physics and Astronomy · #Cosmology and Gravitation Theories #FOS: Physical sciences #Gamma-ray bursts and supernovae #High Energy Astrophysical Phenomena (astro-ph.HE) #Pulsars and Gravitational Waves Research #astro-ph.HE

paper · pdf · doi:10.48550/arxiv.1512.03520

ACTA Astronomica Sinica, Vol 56, Supplement

openalex publication_date 2015/12/11 · arxiv created 2015/12/18 · arxiv updated 2015/12/21 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28

Abstract

TThe glitch of anomalous X-ray pulsars & soft gamma repeaters (AXP/SGRs) usually accompanied with detectable energy releases manifesting as X-ray bursts or outbursts, while the glitch of some pulsars like Vela release negligible energy. We find that these two types of glitches can naturally correspond to two types of starquake of solid strange stars. By applying the EoS of quark cluster star and some realistic pulsar parameters, we can reproduce consistent results compared with previous constraints and observations.

Related