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Neutron Stars in the Model of Non—linear Realization of SU(2) Chiral Symmetry Spontaneous Breaking
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作者 WANGNan SUNBao-Xi +1 位作者 luexiao-fu ZHAOEn-Guang 《Communications in Theoretical Physics》 SCIE CAS CSCD 2003年第5期603-606,共4页
The properties of neutron stars are studied in a relativistic mean-field model with SU(2) chiral symmetry spontaneous breaking being considered. The calculation results indicate that the effects of the chiral symmetry... The properties of neutron stars are studied in a relativistic mean-field model with SU(2) chiral symmetry spontaneous breaking being considered. The calculation results indicate that the effects of the chiral symmetry spontaneous breaking are not negligible. 展开更多
关键词 neutron star chiral symmetry spontaneous breaking relativistic mean-field approximation
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