Neutron star equation of state in density dependent relativistic Hartree-Fock theory

SUN Bao-Yuan; MENG Jie

doi:10.1088/1674-1137/33/S1/024

Chinese Physics C> 2009, Vol. 33> Issue(S1) : 73-75 DOI: 10.1088/1674-1137/33/S1/024

Neutron star equation of state in density dependent relativistic Hartree-Fock theory

SUN Bao-Yuan ,
MENG Jie ^,

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Abstract：
The equation of state of neutron stars is studied in the newly developed density dependent relativistic Hartree-Fock (DDRHF) theory with the effective interaction PKO1 and applied to describe the properties of neutron stars. The results are compared with the recent observational data of compact stars and those calculated with the relativistic mean field (RMF) effective interactions. The maximum mass of neutron stars calculated with PKO1 is about 2.45 M_⊙, which consists with high pulsar mass from PSR B1516+02B recently reported. The influence of Fock terms on the cooling of neutron stars is discussed as well.

References

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SUN Bao-Yuan and MENG Jie. Neutron star equation of state in density dependent relativistic Hartree-Fock theory[J]. Chinese Physics C, 2009, 33(S1): 73-75. doi: 10.1088/1674-1137/33/S1/024

SUN Bao-Yuan and MENG Jie. Neutron star equation of state in density dependent relativistic Hartree-Fock theory[J]. Chinese Physics C, 2009, 33(S1): 73-75. doi: 10.1088/1674-1137/33/S1/024 shu

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Received: 2008-10-22
Revised: 1900-01-01

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通讯作者: 陈斌, bchen63@163.com

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沈阳化工大学材料科学与工程学院沈阳 110142

Neutron star equation of state in density dependent relativistic Hartree-Fock theory

Corresponding author: MENG Jie,

Received Date: 2008-10-22

Accepted Date: 1900-01-01

Available Online: 2009-01-10

Abstract: The equation of state of neutron stars is studied in the newly developed density dependent relativistic Hartree-Fock (DDRHF) theory with the effective interaction PKO1 and applied to describe the properties of neutron stars. The results are compared with the recent observational data of compact stars and those calculated with the relativistic mean field (RMF) effective interactions. The maximum mass of neutron stars calculated with PKO1 is about 2.45 M_⊙, which consists with high pulsar mass from PSR B1516+02B recently reported. The influence of Fock terms on the cooling of neutron stars is discussed as well.

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Neutron star equation of state in density dependent relativistic Hartree-Fock theory

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