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Rotational Deformation of Neutron Stars
作者姓名:文德华 陈伟 刘良钢
作者单位:[1]DepartmentofPhysics,SouthChinaUniversityofTechnology,Guangzhou510641 [2]DepartmentofPhysics,JinanUniversity,Guangzhou510632_ [3]DepartmentofPhysics,ZhongshanUniversity,Guangzhou510275
摘    要:The rotational deformations of two kinds of neutron stars are calculated by using Hartle‘s slow-rotation formulism. The results show that only the faster rotating neutron star gives an obvious deformation. For the slow rotating neutron star with a period larger than hundreds of millisecond, the rotating deformation is very weak.

关 键 词:中子星 旋转形变 哈特曼苏旋转公式 自旋速度
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