Interaction of viscous modified Chaplygin gas with f(R, T) gravity
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Publication:5369595
DOI10.1142/S0217732317501516zbMath1372.83067OpenAlexW2750448865MaRDI QIDQ5369595
Aisha Siddiqa, Muhammad Sharif
Publication date: 18 October 2017
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1142/s0217732317501516
Relativistic cosmology (83F05) Relativistic gravitational theories other than Einstein's, including asymmetric field theories (83D05)
Related Items (7)
Non-adiabatic gravitational collapse in f(R,T) gravity with Karmarkar condition for anisotropic fluid ⋮ A view of compact configurations from the R + γe χT scenario ⋮ Propagation of polar gravitational waves in \(f(R, T)\) scenario ⋮ Gravitational collapse for anisotropic radiating star with Karmarkar condition in \(f(\mathscr{R}, \mathscr{T})\) gravity ⋮ Charged perfect fluid gravitational collapse in f(R, T) gravity ⋮ Phantom fluid supporting traversable wormholes in alternative gravity with extra material terms ⋮ Models of charged self-gravitating source in f(R,T) theory
Cites Work
- Modified equation of state, scalar field, and bulk viscosity in Friedmann universe
- Cosmological evolution of quintessence and phantom with a new type of interaction in dark sector
- Unification of dark matter and dark energy: the inhomogeneous Chaplygin gas
- Viscous generalized Chaplygin gas with arbitrary \(\alpha\)
- Viscous generalized Chaplygin gas interacting with f(R,T) gravity
- The emergent universe: inflationary cosmology with no singularity
- RECONSTRUCTION OF f(R, T) GRAVITY DESCRIBING MATTER DOMINATED AND ACCELERATED PHASES
- Cosmological Imprint of an Energy Component with General Equation of State
- An alternative to quintessence
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