Bulk viscous fluid cosmological models in \(f(R, T)\) gravity
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Publication:6122127
DOI10.1016/J.CJPH.2016.08.008OpenAlexW2508951116WikidataQ126005487 ScholiaQ126005487MaRDI QIDQ6122127
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Publication date: 28 February 2024
Published in: Chinese Journal of Physics (Taipei) (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1016/j.cjph.2016.08.008
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Cites Work
- Early universe cosmology with particle creation: kinematics tests
- Kantowski-Sacks bulk viscous string cosmological models in the presence of zero-mass scalar fields
- Quantum de Sitter cosmology and phantom matter
- Kaluza-Klein cosmological model in \(f(R,T)\) gravity
- Particle creation in higher dimensional space-time with variable \(G\) and \(\Lambda \)
- Reconstruction of modified \(f(R,T)\) gravity with perfect fluid cosmological models
- Bianchi type-III cosmological model in \(f(R,T)\) theory of gravity
- Exact solutions of Bianchi type \(V\) spacetime in \(f(R,T)\) gravity
- LRS Bianchi type-I cosmological model in \(f(R,T)\) theory of gravity
- Bianchi type-VI\({}_0\) perfect fluid cosmological model in a modified theory of 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
- Scale-Covariant Theory of Gravitation and Astrophysical Applications
- Master Equations for Gravitational Perturbations of Static Lovelock Black Holes in Higher Dimensions
- Dynamical instability for non-adiabatic spherical collapse
- Dimensionally continued Oppenheimer–Snyder gravitational collapse: Solutions in odd dimensions
- Dimensionally continued Oppenheimer-Snyder gravitational collapse: Solutions in even dimensions
- Inflationary universe: A possible solution to the horizon and flatness problems
- The Dynamical Instability of Gaseous Masses Approaching the Schwarzschild Limit in General Relativity.
- Thermodynamics and cosmology
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