Tolman–Oppenheimer–Volkoff equations in nonlocal f(R) gravity

DOI10.1142/S0217751X15500931zbMath1320.83042arXiv1502.05000MaRDI QIDQ2946309

No author found.

Publication date: 16 September 2015

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

Full work available at URL: https://arxiv.org/abs/1502.05000

zbMATH Keywords

convectionequations of stateneutron starsconductionthermodynamic processeshigher-dimensional gravity and other theories of gravity

Mathematics Subject Classification ID

Classical and relativistic thermodynamics (80A10) Kaluza-Klein and other higher-dimensional theories (83E15) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Observational and experimental questions in relativity and gravitational theory (83B05) Galactic and stellar structure (85A15) Equations of motion in general relativity and gravitational theory (83C10)

Related Items (11)

The realistic models of relativistic stars in f  ( R ) = R + αR ² gravity ⋮ Stellar structures admitting Noether symmetries in f(ℛ,𝒯 ) gravity ⋮ Stellar structures in \(f(\mathcal{G})\) gravity admitting Noether symmetries ⋮ Anisotropic spherical solutions by gravitational decoupling in \(f(R)\) gravity ⋮ Constraining quadratic f(R) gravity from astrophysical observations of the pulsar J0704+6620 ⋮ Stability Analysis of Isotropic Spheres in Einstein Gauss–Bonnet Gravity ⋮ Effects of charge on gravitational decoupled anisotropic solutions in \(f(R)\) gravity ⋮ Analysis of charged compact stars in f(R,T) gravity using Bardeen geometry ⋮ Dynamical behavior of stellar structures in \(f(\mathcal{G})\) gravity ⋮ Mimetic compact stars ⋮ Properties of white dwarfs in Einstein-Λ gravity

Cites Work

• Nonperturbative models of quark stars in \(f(R)\) gravity
• Screening of cosmological constant for de Sitter universe in non-local gravity, phantom-divide crossing and finite-time future singularities
• Modified non-local-\(F(R)\) gravity as the key for the inflation and dark energy
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• One-loop effective action for non-local modified Gauss-Bonnet gravity in de Sitter space
• A new type of isotropic cosmological models without singularity
• Nonlocal Cosmology
• A NOTE ON CONSTANT CURVATURE SOLUTIONS IN CYLINDRICALLY SYMMETRIC METRIC f(R) GRAVITY
• A singularity-free solution for a charged fluid sphere in general relativity
• Effect of Inhomogeneity on Cosmological Models
• CYLINDRICAL SOLUTIONS IN MODIFIED f(T) GRAVITY
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• On Massive Neutron Cores

This page was built for publication: Tolman–Oppenheimer–Volkoff equations in nonlocal f(R) gravity