Neutron Star in Relativistic Mean-field Approximation

SUN Bao-Xi; JIA Huan-Yu; MENG Jie; ZHAO En-Guang

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《中国物理C》（英文）编辑部

2024年10月30日

Chinese Physics C> 2000, Vol. 24> Issue(S1) : 69-72

Neutron Star in Relativistic Mean-field Approximation

Institute of Theoretical Physics,The Chinese Academy of Sciences,Beijing 100080,China2 Department of Technology Physics,Peking University,Beijing 100871,China3 Center of Theoretical Nuclear Physics,National Laboratory of Heavy Ion,Accelerator,Lanzhou 730000,China

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Abstract：
The equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different couplings of the hyperons.The properties of neutron stars are studied by solving the Oppenheimer-Vollkoff equation.It shows that these properties change distinctly as different couplings of hyperons are concemed.

References

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Heiselberg H, Hjorth-Jensen M. Phys. Rep., 2000,328:2372 Pradash M, Bombaci I, Prakash M et al. Phys. Rep., 1997, 280: 13 Glendenning N K, Moszkowsk; S A. Phys. Rev. Lett., 1991, 67: 24144 Glendenning N K. Compact Star:Nuclear Physics, Particle Physics, and General Relarivity, (Springer-Verlag, New York,1997)

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SUN Bao-Xi, JIA Huan-Yu, MENG Jie and ZHAO En-Guang. Neutron Star in Relativistic Mean-field Approximation[J]. Chinese Physics C, 2000, 24(S1): 69-72.

SUN Bao-Xi, JIA Huan-Yu, MENG Jie and ZHAO En-Guang. Neutron Star in Relativistic Mean-field Approximation[J]. Chinese Physics C, 2000, 24(S1): 69-72. shu

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Received: 1900-01-01
Revised: 1900-01-01

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1.
沈阳化工大学材料科学与工程学院沈阳 110142

Neutron Star in Relativistic Mean-field Approximation

Corresponding author: SUN Bao-Xi,

Institute of Theoretical Physics,The Chinese Academy of Sciences,Beijing 100080,China2 Department of Technology Physics,Peking University,Beijing 100871,China3 Center of Theoretical Nuclear Physics,National Laboratory of Heavy Ion,Accelerator,Lanzhou 730000,China

Received Date: 1900-01-01
Accepted Date: 1900-01-01
Available Online: 2000-07-15

Abstract: The equations of state of the neutron star matter are calculated in the relativistic mean-field approximation with different couplings of the hyperons.The properties of neutron stars are studied by solving the Oppenheimer-Vollkoff equation.It shows that these properties change distinctly as different couplings of hyperons are concemed.