Stability analysis of neutron stars in Palatini f(R, T) gravity

被引：0
|
作者：
M. Z. Bhatti
Z. Yousaf
机构：
[1] University of the Punjab,Department of Mathematics
来源：
General Relativity and Gravitation | 2019年 / 51卷
关键词：
Gravitation; Self-gravitating systems; Relativistic dissipative fluids;
D O I：
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摘要：
In this paper, we have studied the stability of neutron stars in the background of Palatini f(R, T) gravity. In this context, the static spherically symmetric geometry is considered which is assumed to be coupled with an isotropic matter configurations. The evolution of the system is considered with the help of Tolman–Oppenheimer–Volkoff equations and conformal transformations. We found the stable configurations of the spherical stars with some constraints.
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