Effects of three-body forces on the maximum mass of neutron stars in the lowest-order constrained variational formalism

被引：31

作者：

Goudarzi, S. ^{[1
]}

Moshfegh, H. R. ^{[1
]}

机构：

[1] Univ Tehran, Dept Phys, Tehran, Iran

来源：

PHYSICAL REVIEW C | 2015年 / 91卷 / 05期

关键词：

ASYMMETRICAL NUCLEAR-MATTER; EQUATION-OF-STATE; LOCV CALCULATIONS; ENERGY;

D O I：

10.1103/PhysRevC.91.054320

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

The equation of state of neutron star matter is calculated within the lowest order constrained variational (LOCV) method using different two-body interactions and an Urbana type three-body force. The core of the neutron star is modelled by beta-stable matter. The corresponding neutron star mass-radius relations are presented and the effect of using a three-body interaction on the maximum gravitational mass of the star is also discussed. It is shown that including the three-body force generally increases the maximum gravitational mass.

引用

页数：10

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