Strange stars in energy–momentum-conserved f(R,T) gravity

DOI10.1142/S0218271820500753zbMath1443.83043arXiv1911.02484MaRDI QIDQ5125307

S. I. dos Santos Jr., M. Malheiro, G. A. Carvalho, P. H. R. S. Moraes

Publication date: 6 October 2020

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

Full work available at URL: https://arxiv.org/abs/1911.02484

zbMATH Keywords

modified theories of gravitystrange starsTOV equation

Mathematics Subject Classification ID

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

Related Items (2)

Stellar structure models in modified theories of gravity: lessons and challenges ⋮ Traversable wormholes in the traceless f(R,T) gravity

Uses Software

• Python

Cites Work

• Nonperturbative models of quark stars in \(f(R)\) gravity
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• <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
• f(R) GRAVITY AND ITS COSMOLOGICAL IMPLICATIONS
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• Charged perfect fluid gravitational collapse in f(R, T) gravity
• Strange stars inf(R,𝒯) gravity
• Constraining values of bag constant for strange star candidates
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• General Relativistic Polytropic Fluid Spheres.
• COSMOLOGICAL DYNAMICS OF f(R) GRAVITY SCALAR DEGREE OF FREEDOM IN EINSTEIN FRAME
• SOLAR SYSTEM TESTS OF f(R) GRAVITY
• The cosmological constant problem
• Static Solutions of Einstein's Field Equations for Spheres of Fluid
• On Massive Neutron Cores

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