Role of σR2 + γRμνTμν model on anisotropic polytropes

DOI10.1142/S021827181950007XzbMath1425.83069arXiv1812.11037OpenAlexW3098500794MaRDI QIDQ4972815

Arfa Waseem, Muhammad Sharif

Publication date: 27 November 2019

Published in: International Journal of Modern Physics D (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/1812.11037

zbMATH Keywords

compact objects\(f(R, T, Q)\) gravitypolytropic equation-of-state

Mathematics Subject Classification ID

Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Galactic and stellar structure (85A15)

Cites Work

• \(f(R, T, R_{\mu \nu} T^{\mu \nu})\) gravity phenomenology and \(\lambda\)CDM universe
• Structure of neutron stars in \(R\)-squared gravity
• Consistency of \(f(R)\) gravity models around solar polytropes
• General Relativistic Fluid Spheres
• Bounds on the basic physical parameters for anisotropic compact general relativistic objects
• The realistic models of relativistic stars in f  ( R ) = R + αR ² gravity
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• General Relativistic Polytropic Fluid Spheres.
• The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• On Massive Neutron Cores
• Unnamed Item

This page was built for publication: Role of σR2 + γRμνTμν model on anisotropic polytropes