R-mode instability of strange stars and observations of neutron stars in LMXBs

Chun-Mei、Pi Pi、Shuhua、Yang、Xiaoping、Zheng Zheng

2015天文和天体物理学研究：英文版Physics and Astronomy被引 3

摘要

Using a realistic equation of state(EOS) of strange quark matter, namely,the modified bag model, and considering the constraints on the parameters of EOS by the observational mass limit of neutron stars, we investigate the r-mode instability window of strange stars, and find the same result as in the brief study of Haskell,Degenaar and Ho in 2012 that these instability windows are not consistent with the spin frequency and temperature observations of neutron stars in low mass X-ray binaries.

引用本文（GB/T 7714）

Chun-Mei, Pi Pi, Shuhua, 等. R-mode instability of strange stars and observations of neutron stars in LMXBs[J]. 天文和天体物理学研究：英文版, 2015.

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