Two types of glitches in a solid quark star model
High Energy Astrophysical Phenomena
2015-12-21 v2
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.
Keywords
Cite
@article{arxiv.1512.03520,
title = {Two types of glitches in a solid quark star model},
author = {Jiguang Lu and Enping Zhou},
journal= {arXiv preprint arXiv:1512.03520},
year = {2015}
}
Comments
ACTA Astronomica Sinica, Vol 56, Supplement