Anisotropic quark stars in f(R) = R 1+ϵ gravity

DOI10.1088/1361-6382/ac7a88zbMath1498.85006arXiv2202.04467OpenAlexW4283210086MaRDI QIDQ5090236

J. M. Z. Pretel, S. B. Duarte

Publication date: 18 July 2022

Published in: Classical and Quantum Gravity (Search for Journal in Brave)

Full work available at URL: https://arxiv.org/abs/2202.04467

zbMATH Keywords

anisotropic fluidquark stars\(f(R)\) modified gravity

Mathematics Subject Classification ID

Anisotropy in solid mechanics (74E10) Strong interaction, including quantum chromodynamics (81V05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Asymptotic procedures (radiation, news functions, (mathcal{H} )-spaces, etc.) in general relativity and gravitational theory (83C30) Galactic and stellar structure (85A15)

Related Items (4)

Charged quark stars in metric f(R) gravity ⋮ Neutron stars in modified teleparallel gravity ⋮ Impact of minimal matter-geometry coupling on anisotropic quark stars ⋮ The criteria of the anisotropic quark star models in Rastall gravity

Cites Work

• Nonperturbative models of quark stars in \(f(R)\) gravity
• Do consistent \(F(R)\) models mimic general relativity plus \(\Lambda\)?
• \(f(R)\) theories
• Extended gravity description for the GW190814 supermassive neutron star
• Stellar structure models in modified theories of gravity: lessons and challenges
• Relativistic model for anisotropic strange stars
• Causal thermodynamics of a gravitational collapse model for an anisotropic fluid with dissipative flows
• Modeling of compact stars: an anisotropic approach
• Anisotropic quark stars in \(R^2\) gravity
• Anisotropic compact stars: constraining model parameters to account for physical features of tidal love numbers
• Modified gravity theories on a nutshell: inflation, bounce and late-time evolution
• A new type of isotropic cosmological models without singularity
• <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mi>f</mml:mi><mml:mrow><mml:mo>(</mml:mo><mml:mi>R</mml:mi><mml:mo>)</mml:mo></mml:mrow></mml:mrow></mml:math>theories of gravity
• Radial pulsations and stability of anisotropic stars with a quasi-local equation of state
• Behavior of Anisotropic Compact Stars in f(R, ϕ) Gravity*
• INTRODUCTION TO MODIFIED GRAVITY AND GRAVITATIONAL ALTERNATIVE FOR DARK ENERGY
• Spherically symmetric solutions in f ( R ) gravity via the Noether symmetry approach
• Slowly rotating anisotropic neutron stars in general relativity and scalar–tensor theory
• CURVATURE QUINTESSENCE
• Determination of the charge for strange stars
• The confrontation between general relativity and experiment
• Bardeen compact stars in modified \(f(R)\) gravity

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