Bianchi type IX cosmological model with perfect fluid in \(f(R,T)\) theory of gravity
DOI10.1007/s10714-023-03103-wzbMath1528.83169MaRDI QIDQ6174859
M. R. Ugale, Siddharth B. Deshmukh
Publication date: 15 July 2023
Published in: General Relativity and Gravitation (Search for Journal in Brave)
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) Dark matter and dark energy (83C56) Mathematical modeling or simulation for problems pertaining to relativity and gravitational theory (83-10)
Cites Work
- Some homogeneous Bianchi type IX viscous fluid cosmological models with a varying \(\Lambda\)
- Bianchi type-III dark energy model in \(f(R,T)\) gravity
- Dark energy cosmology: the equivalent description via different theoretical models and cosmography tests
- Bianchi type-III cosmological model in \(f(R,T)\) theory of gravity
- Universe filled with dark energy (DE) from a wet dark fluid (WDF) in \(f(R,T)\) gravity
- A new class of Bianchi cosmological models in \(f(R,T)\) gravity
- From Inflation to Dark Energy in the Non-Minimal Modified Gravity
- Super inflation mechanism with oscillating scalar fields in F(R,T) gravity
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