Cosmological models with a varying polynomial deceleration parameter in \(f(R)\) and \(f(R,T)\)-gravity
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Publication:2096018
DOI10.1007/s11182-022-02524-5OpenAlexW4226257944MaRDI QIDQ2096018
Publication date: 16 November 2022
Published in: Russian Physics Journal (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s11182-022-02524-5
Cites Work
- Kaluza-Klein universe with cosmic strings and bulk viscosity in \(f(R,T)\) gravity
- Cosmological models with linearly varying deceleration parameter
- \(F(T)\) gravity and k-essence
- Two fluid scenario for dark energy model in a scalar-tensor theory of gravitation
- Bianchi type-III cosmological model in \(f(R,T)\) theory of gravity
- A periodic varying deceleration parameter in f(R, T) gravity
- Inflation in terms of a viscous van der Waals coupled fluid
- Einstein's General Theory of Relativity
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