Thermodynamics of a transient phantom scenario
arXiv:2304.02735 · doi:10.1016/j.dark.2023.101367
Abstract
This work is devoted to the thermodynamics description of a phantom scenario proposed previously by the authors. The presence of negative chemical potential is unavoidable if we allege for a well defined thermodynamics framework since the cosmological model passages from phantom stage at present time to a future de Sitter evolution. As noted earlier in other works, we find that the negativity of the chemical potential is necessary to save phantom dark energy from thermodynamics inconsistencies.
arXiv comment7 pages, 1 figure. Published version in Physics of the Dark Universe
References in corpus (40)
- In the Realm of the Hubble tension a Review of Solutions
- Effective Field Theory, Black Holes, and the Cosmological Constant
- Entropy Bounds and Dark Energy
- First Law of Thermodynamics and Friedmann Equations of Friedmann-Robertson-Walker Universe
- The Hubble Hunter's Guide
- Unified first law of black-hole dynamics and relativistic thermodynamics
- Dark Matter and Dark Energy Interactions: Theoretical Challenges, Cosmological Implications and Observational Signatures
- New physics in light of the tension: an alternative view
- The Expansion of the Universe is Faster than Expected
- Cosmic Holography
- Hawking Radiation of Apparent Horizon in a FRW Universe
- Negative Absolute Temperature for Motional Degrees of Freedom
- Constraints on the sum of the neutrino masses in dynamical dark energy models with are tighter than those obtained in CDM
- Revisiting a negative cosmological constant from low-redshift data
- The cosmological constant from the QCD Veneziano ghost
- Dark Energy and QCD Ghost
- Phantom thermodynamics
- Modified cosmology through spacetime thermodynamics and Barrow horizon entropy
- Thermodynamics, Spectral Distribution and the Nature of Dark Energy
- Notes on Ghost Dark Energy
- More on QCD Ghost Dark Energy
- Unified dark energy thermodynamics: varying w and the -1-crossing
- Modified cosmology through nonextensive horizon thermodynamics
- Cosmology in cubic and gravity
- Entropic Inflation
- From confinement to dark energy
- On Phantom Thermodynamics
- On four-dimensional Einsteinian gravity, quasitopological gravity, cosmology and black holes
- A Note on the Cardy-Verlinde Formula
- Chemical Potential and the Nature of the Dark Energy: The case of phantom
- The Apparent Universe
- Dark energy and Dark matter interaction in light of the second law of thermodynamics
- Lattice QCD in curved spacetimes
- Thermodynamically allowed phantom cosmology with viscous fluid
- Dynamical de Sitter phase and nontrivial holonomy in strongly coupled gauge theories in expanding Universe
- Cosmology with Negative Absolute Temperatures
- Study of QCD generalized ghost dark energy in FRW universe
- Cosmology in 5D and 4D Einstein-Gauss-Bonnet gravity
- Topological Inflation
- Holography and matter creation revisited