Phase transition between flat space cosmology and hot flat spacetimes in GMMG and EGMG models
DOI10.1088/1361-6382/ac03f7zbMath1482.83146arXiv2012.00002OpenAlexW3165312549MaRDI QIDQ5162820
S. N. Sajadi, Mohammad R. Setare
Publication date: 5 November 2021
Published in: Classical and Quantum Gravity (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/2012.00002
phase transitionexotic general massive gravitygeneral minimal massive gravityflat space cosmologyhot flat spacetimes
Relativistic cosmology (83F05) Stefan problems, phase changes, etc. (80A22) Gravitational energy and conservation laws; groups of motions (83C40) Classical and relativistic thermodynamics (80A10) Measures of information, entropy (94A17) Approximation procedures, weak fields in general relativity and gravitational theory (83C25)
Related Items (1)
Cites Work
- Critical points of the exotic massive 3D gravity
- On the generalized minimal massive gravity
- Central charges in the canonical realization of asymptotic symmetries: An example from three dimensional gravity
- Enhanced asymptotic \(BMS_{3}\) algebra of the flat spacetime solutions of generalized minimal massive gravity
- Exotic massive 3D gravity
- Entropy of three-dimensional asymptotically flat cosmological solutions
- Near horizon symmetries of the non-extremal black hole solutions of generalized minimal massive gravity
- Exotic massive 3D gravities from truncation
- Energy of asymptotically AdS black holes in exotic massive gravity and its log-extension
- On the new massive gravity and AdS/CFT
- Black hole conserved charges in generalized minimal massive gravity
- Black hole in three-dimensional spacetime
- Logarithmic corrections to black hole entropy, from the Cardy formula
- On asymptotic charges in 3D gravity
- Minimal massive 3D gravity
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