Expanding universe: thermodynamical aspects from different models
From MaRDI portal
Publication:2348831
DOI10.1007/S10509-012-1156-9zbMath1314.83061arXiv1206.6333OpenAlexW2051785760MaRDI QIDQ2348831
Publication date: 16 June 2015
Published in: Astrophysics and Space Science (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1206.6333
Relativistic cosmology (83F05) Gravitational energy and conservation laws; groups of motions (83C40) Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.) (83C55) Classical and relativistic thermodynamics (80A10)
Cites Work
- Dark energy and the generalized second law
- Validity of thermodynamical laws in dark energy filled universe
- Generalized second law of thermodynamics in quintom dominated universe
- Holographic Chaplygin gas model
- Thermodynamical interpretation of the interacting holographic dark energy model in a non-flat universe
- Validity of the generalized second law of thermodynamics of the universe bounded by the event horizon in holographic dark energy model
- VALIDITY OF THE THERMODYNAMICAL PROPERTIES OF THE DARK ENERGY MODEL WITH THE EQUATION OF STATE: w = w0 + w1 · z(1 + z)/(1 + z2)
- DYNAMICS OF DARK ENERGY
- THERMODYNAMIC STABILITY OF A FLUID WITH VARIABLE EQUATION OF STATE
- Does the validity of the first law of thermodynamics imply that the generalized second law of thermodynamics of the universe is bounded by the event horizon?
- Measurements of Ω and Λ from 42 High‐Redshift Supernovae
- Type Ia Supernova Discoveries atz> 1 from theHubble Space Telescope: Evidence for Past Deceleration and Constraints on Dark Energy Evolution
- Cosmological Imprint of an Energy Component with General Equation of State
- An alternative to quintessence
This page was built for publication: Expanding universe: thermodynamical aspects from different models