Role of structure scalars on viscous and heat conducting spherical systems in f(R,T) gravity

DOI10.1142/S0218271817501553zbMath1431.83136OpenAlexW2741349813WikidataQ125290183 ScholiaQ125290183MaRDI QIDQ5242305

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Publication date: 6 November 2019

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

Full work available at URL: https://doi.org/10.1142/s0218271817501553

zbMATH Keywords

gravitationrelativistic dissipative fluidsstructure scalars

Mathematics Subject Classification ID

Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Quantum hydrodynamics and relativistic hydrodynamics (76Y05)

Related Items (1)

FRW cosmology in f(R,T) gravity

Cites Work

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• Charged adiabatic LTB gravitational collapse in \(f(R)\) gravity
• Modified Gauss-Bonnet theory as gravitational alternative for dark energy
• \(f(R)\) theories
• Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
• LRS Bianchi type-I cosmological model in \(f(R,T)\) theory of gravity
• <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
• RECONSTRUCTING f(R, T) GRAVITY FROM HOLOGRAPHIC DARK ENERGY
• RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
• Cylindrical collapse and gravitational waves

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