Bekenstein–Hawking entropy in expanding universes from black hole theorems
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Publication:2879232
DOI10.1142/S0217732314500916zbMath1295.83044arXiv1405.6816MaRDI QIDQ2879232
Publication date: 8 September 2014
Published in: Modern Physics Letters A (Search for Journal in Brave)
Full work available at URL: https://arxiv.org/abs/1405.6816
Black holes (83C57) Classical and relativistic thermodynamics (80A10) Measures of information, entropy (94A17)
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Cites Work
- Particle creation by black holes
- Is the cosmological singularity thermodynamically possible?
- How does the entropy/information bound work?
- Physically motivated uncertainty relations at the Planck length for an emergent non-commutative spacetime
- The holographic principle
- EXISTENCE OF BLACK HOLES IN FRIEDMANN–ROBERTSON–WALKER UNIVERSE DOMINATED BY DARK ENERGY
- QUANTUM BOUNDS FOR GRAVITATIONAL DE SITTER ENTROPY AND THE CARDY–VERLINDE FORMULA
- Enthalpy and the mechanics of AdS black holes
- Black hole versus cosmological horizon entropy
- The holographic principle for general backgrounds
- The Mass-Particle in an Expanding Universe
- Spin coefficient form of the new laws of black hole dynamics
- The world as a hologram
- The Large Scale Structure of Space-Time
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