Thermodynamics of Extended Gravity Black Holes
Guido Cognola, Lorenzo Sebastiani, Sergio Zerbini
TL;DR
This paper explores the thermodynamic properties of static spherically symmetric black holes in extended gravity theories, focusing on energy, entropy, and temperature calculations.
Contribution
It provides a detailed analysis of black hole thermodynamics in extended gravity, utilizing the Wald method and Clausius relation derivation from equations of motion.
Findings
Black hole entropy evaluated via Wald method.
Energy and temperature relations established.
Insights into thermodynamics of extended gravity black holes.
Abstract
Thermodynamics of extended gravity static spherically symmetric black hole solutions is investigated. The energy issue is discussed making use of the derivation of Clausius relation from equations of motion, evaluating the black hole entropy by the Wald method and computing the related Hawking temperature.
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.