LOCV calculation of the equations of state and properties of rapidly rotating neutron stars

被引：0
作者：
A.H.Farajian
M.Bigdeli
S.Belbasi
机构：
[1] DepartmentofPhysics,UniversityofZanjan
来源：
Chinese Physics C | 2018年 / 42卷 / 06期
关键词：
LOCV method; neutron star matter; equation of state; rotating neutron star;
D O I：
暂无
中图分类号：
P145.6 [脉冲星（中子星）];
学科分类号：
070401 ;
摘要：
In this paper, we have investigated the structural properties of rotating neutron stars using the numerical RNS code and equations of state which have been calculated within the lowest order constrained variational（LOCV）approach. In order to calculate the equation of state of nuclear matter, we have used UV14 +TNI and AV18 potentials.We have computed the maximum mass of the neutron star and the corresponding equatorial radius at different angular velocities. We have also computed the structural properties of Keplerian rotating neutron stars for the maximum mass configuration, MK, RK, fK and jmax.
引用
收藏
页码：132 / 137
页数：6
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