WARM-POLYTROPIC INFLATIONARY UNIVERSE MODEL
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Publication:2866942
DOI10.1142/S0218271813500417zbMath1277.83119arXiv1307.7117OpenAlexW3103705620MaRDI QIDQ2866942
M. J. S. Houndjo, Mohammad R. Setare, Vahid Kamali
Publication date: 10 December 2013
Published in: International Journal of Modern Physics D (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1307.7117
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (4)
Polytropic inspired inflation on the brane ⋮ Constant roll warm inflation in high dissipative regime ⋮ Warm-polytropic cosmology with and without bulk viscosity ⋮ Warm gauge-flation with general dissipative coefficient
Cites Work
- Cardassian expansion: a model in which the universe is flat, matter dominated, and accelerating
- Static spherically symmetric electromagnetic mass models with charged dust sources in Einstein-Cartan theory: Lane-Emden models
- An Alternative to Compactification
- DARK ENERGY WITH POLYTROPIC EQUATION-OF-STATE
- 4D gravity on a brane in 5D Minkowski space
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