Scalar field cosmology in \(f(R,T)\) gravity with \(\Lambda\)
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Publication:2320486
DOI10.1134/S0202289318030039zbMath1423.83047OpenAlexW2888007017MaRDI QIDQ2320486
P. K. Sahoo, Binaya K. Bishi, Can Aktaş, Sezgin Aygün
Publication date: 23 August 2019
Published in: Gravitation \& Cosmology (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1134/s0202289318030039
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05) Exact solutions to problems in general relativity and gravitational theory (83C15) Astrophysical cosmology (85A40)
Related Items (3)
Massive and massless scalar field models for Kaluza–Klein universe in f(R, T) gravity ⋮ Various dark energy models for variables G and Λ in f(R, T) modified theory ⋮ Bulk viscous Bianchi-I embedded cosmological model in f(R,T) = f1(R) + f2(R)f3(T) gravity
Cites Work
- Friedmann equations of FRW universe in scalar-tensor gravity, \(f(R)\) gravity and first law of thermodynamics
- Non-existence of a massive scalar field for the Marder universe in Lyra and Riemannian geometries
- Plane-symmetric mesonic viscous fluid cosmological model
- Bianchi type-III cosmological models in Lyra's geometry in the presence of massive scalar field
- Über eine Modifikation der Riemannschen Geometrie
- Class of Einstein-Maxwell dilatons, an ansatz for new families of rotating solutions
- Cosmological constant Λ in f(R,T) modified gravity
- Gödel-type solution in f(R,T) modified gravity
- A dynamical system analysis of f(R,T) gravity
- Mach's Principle and a Relativistic Theory of Gravitation
- Self-similar spherically symmetric cosmological models with a perfect fluid and a scalar field
- Scalar fields as dark matter in spiral galaxies
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- The cosmological constant problem
- Bulk viscous fluid cosmological models in \(f(R, T)\) gravity
- Geodesic deviation equation in \(f(R, T)\) gravity
- Cosmic transit and anisotropic models in \(f(R, T)\) gravity
- Scalar field and time varying cosmological constant in \(f(R, T)\) gravity for Bianchi type-I universe
- Magnetized strange quark matter solutions in \(f(R, T)\) gravity with cosmological constant
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