Influence of strange matter admixtures on macroscopic properties of neutron stars

被引：0
|
作者：
Urbanec, M. [1 ]
Betak, E. [1 ]
Stuchlik, Z. [1 ]
机构：
[1] Silesian Univ, Inst Phys, Opava 74061, Czech Republic
来源：
FRONTIERS IN NUCLEAR STRUCTURE, ASTROPHYSICS, AND REACTIONS (FINUSTAR 3) | 2011年 / 1377卷
关键词：
Neutron stars; Equations of state; Dense matter; Asymmetric nuclear matter; Hyperons; Quantum hadrodynamics; Relativistic Brueckner-Hartree-Fock; EQUATION-OF-STATE; FREQUENCY RATIOS; FIELD-EQUATIONS; NUCLEAR;
D O I：
10.1063/1.3628392
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We used the equations of state (EoS) of dense nuclear matter to construct the macroscopic properties of neutron stars and test them using available observational results. The Dirac-Brueckner-Hartree-Fock mean field calculations approximated by their parameterized form are the basis of our calculations for the star interior. We calculated the central pressure, density, radius and mass both without and with allowance for hyperons, and compared these results with astronomical observations.
引用
收藏
页码：275 / 279
页数：5
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