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Stability analysis of neutron stars in Palatini f(RT) gravity

  • M. Z. BhattiEmail author
  • Z. Yousaf
  • Zarnoor
Research Article
  • 41 Downloads

Abstract

In this paper, we have studied the stability of neutron stars in the background of Palatini f(RT) 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.

Keywords

Gravitation Self-gravitating systems Relativistic dissipative fluids 

Notes

Acknowledgements

The works of MZB and ZY are supported by National Research Project for Universities (NRPU), Higher Education Commission, Islamabad under the research Project No. 8769.

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© Springer Science+Business Media, LLC, part of Springer Nature 2019

Authors and Affiliations

  1. 1.Department of MathematicsUniversity of the PunjabLahorePakistan

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