A thermodynamic motivation for dark energy
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Publication:2429501
DOI10.1007/s10714-011-1299-yzbMath1238.83087arXiv1012.0474OpenAlexW2116062189MaRDI QIDQ2429501
Publication date: 27 April 2012
Published in: General Relativity and Gravitation (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1012.0474
Relativistic cosmology (83F05) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10) Astrophysical cosmology (85A40)
Related Items (15)
Thermodynamic equilibrium and rise of complexity in an accelerated universe ⋮ Thermodynamical description of modified generalized Chaplygin gas model of dark energy ⋮ Phase space analysis of bulk viscous matter dominated universe ⋮ Generalized Second Law of Thermodynamics in Parabolic LTB Inhomogeneous Cosmology ⋮ Thermodynamical description of the ghost dark energy model ⋮ Does the entropy of the universe tend to a maximum? ⋮ A probe of cosmological models in modified teleparallel gravity ⋮ Thermodynamics of diffusive DM/DE systems ⋮ Generalized holographic Ricci dark energy and generalized second law of thermodynamics in Bianchi type I universe ⋮ Thermal stability of Tsallis holographic dark energy in nonflat universe ⋮ Why the expansion of the Universe is accelerated ⋮ Null trajectories and bending of light in charged black holes with quintessence ⋮ Necessity of dark energy from thermodynamic arguments ⋮ Type V singularities with inhomogeneous equations of state ⋮ A note on the relations between thermodynamics, energy definitions and Friedmann equations
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