Cosmology in modified f(R,T)-gravity theory in a variant Λ(T) scenario-revisited
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Publication:4600596
DOI10.1142/S0219887818500147zbMath1381.83156MaRDI QIDQ4600596
Umesh Kumar Sharma, Anirudh Pradhan
Publication date: 11 January 2018
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
Relativistic cosmology (83F05) Classes of solutions; algebraically special solutions, metrics with symmetries for problems in general relativity and gravitational theory (83C20) Space-time singularities, cosmic censorship, etc. (83C75) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (7)
Relationship between magnetic field and anisotropy parameter in gravitation theories ⋮ Traversable wormholes with logarithmic shape function in f(R,T) gravity ⋮ Bulk viscous cosmological model in f(R,T) theory of gravity ⋮ FRW cosmology in f(R,T) gravity ⋮ Various dark energy models for variables G and Λ in f(R, T) modified theory ⋮ Magnetized string cosmological models of accelerated expansion of the Universe in f(R,T) theory of gravity ⋮ Axially Symmetric Bulk Viscous Cosmological Model in F(R, T) Theory of Gravity
Cites Work
- Unnamed Item
- Friedmann cosmology with matter creation in modified \(f(R,T)\) gravity
- Kantowski-Sachs universe filled with perfect fluid in \(f(R,T)\) theory of gravity
- Cosmological models with linearly varying deceleration parameter
- Bianchi type-II string cosmological model with magnetic field in \(f(R,T)\) gravity
- Bianchi type-II dark energy model in \(f(R,T)\) gravity
- Magnetized string cosmology in anisotropic Bianchi-II space-time with variable cosmological term-\(\Lambda\)
- Cosmological reconstruction and stability in \(f(R,T)\) gravity
- Perfect fluid quantum universe in the presence of negative cosmological constant
- Bianchi type-III dark energy model in \(f(R,T)\) gravity
- Higher dimensional cosmological models filled with perfect fluid in \(f(R,T)\) theory of gravity
- Universe filled with dark energy (DE) from a wet dark fluid (WDF) in \(f(R,T)\) gravity
- LRS Bianchi type-I cosmological model in \(f(R,T)\) theory of gravity
- Non-existence of Bianchi type-III bulk viscous string cosmological model in \(f(R,T)\) gravity
- Bianchi type-\(V\) cosmology in \(f(R,T)\) gravity with \(\varLambda (T)\)
- A new class of Bianchi cosmological models in \(f(R,T)\) gravity
- Asymptotic behavior of homogeneous cosmological models in the presence of a positive cosmological constant
- A study of angular size-redshift relation for models in which Λ decays as the energy density
- Cosmological constant Λ in f(R,T) modified gravity
- A dynamical system analysis of f(R,T) gravity
- THE CAUCHY PROBLEM FOR f(R)-GRAVITY: AN OVERVIEW
- Viscous generalized Chaplygin gas interacting with f(R,T) gravity
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- Anisotropic cosmological models in f(R,T) gravity with variable deceleration parameter
- IS GRAVITY AN INTRINSICALLY QUANTUM PHENOMENON? DYNAMICS OF GRAVITY FROM THE ENTROPY OF SPACE–TIME AND THE PRINCIPLE OF EQUIVALENCE
- THE CAUCHY PROBLEM FOR METRIC-AFFINE f(R)-GRAVITY IN PRESENCE OF A KLEIN–GORDON SCALAR FIELD
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