Two fluid scenario for dark energy model in a scalar-tensor theory of gravitation

DOI10.1007/s10773-012-1454-6zbMath1266.83155OpenAlexW1979792163MaRDI QIDQ1955906

R. Santhi Kumar, D. R. K. Reddy

Publication date: 19 June 2013

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

Full work available at URL: https://doi.org/10.1007/s10773-012-1454-6

zbMATH Keywords

scalar-tensor theorydark energytwo fluid scenario

Mathematics Subject Classification ID

Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15)

Related Items (5)

The complete Brans-Dicke theories ⋮ Transit cosmological models in FRW universe under the two-fluid scenario ⋮ A dark energy quintessence model of the universe ⋮ Cosmological models with a varying polynomial deceleration parameter in \(f(R)\) and \(f(R,T)\)-gravity ⋮ Mesonic cosmological model with two-fluid source in Lyra geometry

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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
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