作者: Xiao-Ping Zheng , Shu-Hua Yang , Chun-Mei Pi
DOI: 10.1088/1674-4527/15/6/009
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摘要: Using a realistic equation of state (EOS) strange quark matter, namely, the modified bag model, and considering constraints to parameters EOS by observational mass limit neutron stars, we study r-mode instability window find same result as brief Haskell, Degenaar Ho in 2012 that these windows are not consistent with spin frequency temperature observations stars LMXBs.