Abstract：The stiff and soft hadronic matter equations of state in the framework of the relativistic mean-field (RMF) theory and MIT bag model of quark matter with free parameter-s quark mass are used to construct the model of hybrid stars. The change of the internal structure of the star due to rotation has been investigated, and the effect of different model bringing to configuration of star has been analyzed. The s quark mass is a prominent factor which influences deformation properties of rotating hybrid stars.
收稿日期: 2007-01-25
引用本文:
康缈,潘娜娜,周霞,郑小平. 旋转混合星的结构[J]. , 2007, 46(1): 0-0.
康缈,潘娜娜,周霞,郑小平. The structure of rotating hybrid stars. , 2007, 46(1): 0-0.
