Logarithmic Corrections to Gravitational Entropy and the Null Energy Condition
arXiv:1612.06949 · doi:10.1016/j.physletb.2016.07.071
Abstract
Using a relation between the thermodynamics of local horizons and the null energy condition, we consider the effects of quantum corrections to the gravitational entropy. In particular, we find that the geometric form of the null energy condition is not affected by the inclusion of logarithmic corrections to the Bekenstein-Hawking entropy.
arXiv commentLaTex, 10 pages
References in corpus (17)
- Thermodynamics of Spacetime: The Einstein Equation of State
- Black Hole Entropy is Noether Charge
- Hawking Radiation as Tunneling
- Logarithmic correction to the Bekenstein-Hawking entropy
- Logarithmic Corrections to Black Hole Entropy from the Cardy Formula
- Hawking Radiation and Black Hole Thermodynamics
- A Secret Tunnel Through The Horizon
- Universality of Quantum Entropy for Extreme Black Holes
- Proof of the Quantum Null Energy Condition
- Black Holes in Gravity with Conformal Anomaly and Logarithmic Term in Black Hole Entropy
- Logarithmic correction to the Bekenstein-Hawking entropy of the BTZ black hole
- Achronal averaged null energy condition
- A comment on black hole entropy or does Nature abhor a logarithm?
- Proof of the averaged null energy condition in a classical curved spacetime using a null-projected quantum inequality
- Derivation of the Null Energy Condition
- Thermodynamic Origin of the Null Energy Condition
- Two Roads to the Null Energy Condition