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5. Gravitational waves from the axial oscillation of neutron star considering non-Newtonian gravity

Gravitational waves from the axial oscillation of neutron star considering non-Newtonian gravity

来源 :核技术：英文版 | 被引量 : 0次 | 上传用户：ljyxq13571302523

【摘 要】

：

The eigen-frequencies of the axial w-modes of neutron star described by a super-soft equation of state(EOS) are investigated,by considering the non-Newtonian gr

【作 者】

：

WEN Dehua ZHOU Ying 

【机 构】

：

DepartmentofPhysics

【出 处】

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核技术：英文版

【发表日期】

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2013年5期

【关键词】

：

非牛顿引力 中子星 轴向 引力波 摆动 本征频率 恒星质量 EOS Neutron stars  Oscillation  Non-Newtonian grav 

【基金项目】

：

Supported by National Natural Science Foundation of China （Nos.10947023, 11275073 and 11205061）, and Fundamental Research Funds for the Central University, China （No. 2012ZZ0079）. The project is spons

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论文部分内容阅读

The eigen-frequencies of the axial w-modes of neutron star described by a super-soft equation of state(EOS) are investigated,by considering the non-Newtonian gravity.The results show that at the same stellar mass,the frequencies of wI and wI2 for our mode

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