Anisotropic spherical solutions through extended gravitational decoupling approach

DOI10.1016/j.aop.2020.168122zbMath1434.83028arXiv2004.07925OpenAlexW3102513597MaRDI QIDQ2175165

Qanitah Ama-Tul-Mughani, Muhammad Sharif

Publication date: 28 April 2020

Published in: Annals of Physics (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2004.07925

zbMATH Keywords

anisotropyexact solutionsextended geometric deformation

Mathematics Subject Classification ID

Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Galactic and stellar structure (85A15)

Related Items (7)

Geodesic motion around hairy black holes ⋮ Exploring physical properties of minimally deformed strange star model and constraints on maximum mass limit in f(𝒬) gravity ⋮ Braneworld‐Klein‐Gordon System in the Framework of Gravitational Decoupling ⋮ Complexity‐Free Anisotropic Solution of Buchdahl's Model and Energy Exchange Between Relativistic Fluids by Extended Gravitational Decoupling ⋮ Minimally Deformed Wormholes Inspired by Noncommutative Geometry ⋮ Complexity factor of spherically anisotropic polytropes from gravitational decoupling ⋮ Anisotropic Tolman V solution by minimal gravitational decoupling approach

Cites Work

• Sharp bounds on the critical stability radius for relativistic charged spheres
• Decoupling gravitational sources in general relativity: the extended case
• Anisotropic spherical solutions by gravitational decoupling in \(f(R)\) gravity
• The minimal geometric deformation approach extended
• Extended gravitational decoupling in 2  +  1 dimensional space-times
• Sound speeds, cracking and the stability of self-gravitating anisotropic compact objects
• SEARCHING EXACT SOLUTIONS FOR COMPACT STARS IN BRANEWORLD: A CONJECTURE
• 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
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