Holographic dark energy model with interaction and cosmological constant in the flat space-time
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Publication:454228
DOI10.1007/S10773-011-1070-XzbMath1252.83121OpenAlexW2021458252MaRDI QIDQ454228
Publication date: 1 October 2012
Published in: International Journal of Theoretical Physics (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1007/s10773-011-1070-x
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55)
Related Items (8)
Stability of dark energy models on the brane universes ⋮ Dark matter density from heavy neutrino decays ⋮ Accretion of some classes of holographic DE onto higher-dimensional Schwarzschild black holes ⋮ Time-dependent density of modified cosmic Chaplygin gas with variable cosmological constant in non-flat universe ⋮ Effect of varying bulk viscosity on generalized Chaplygin gas ⋮ Viscous new varying modified cosmic Chaplygin gas with cosmological constant in non-flat universe ⋮ Interacting modified cosmic Chaplygin gas with variable cosmological constant and viscosity ⋮ Warm-polytropic cosmology with and without bulk viscosity
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