Thermodynamics of rotating black holes in conformal gravity
Negin Kamvar, Reza Saffari, and Saheb Soroushfar

TL;DR
This paper investigates the thermodynamics of rotating black holes in conformal gravity, deriving key quantities like temperature, entropy, and angular momentum, and confirming the validity of the first law of thermodynamics in this context.
Contribution
It provides a detailed analysis of thermodynamic properties of rotating black holes in conformal gravity, including new calculations of angular momentum and verification of thermodynamic laws.
Findings
Thermodynamical quantities are derived for rotating black holes in conformal gravity.
The first law of thermodynamics is confirmed to hold for these black holes.
Effective angular momentum is calculated at the event horizon and beyond.
Abstract
In this paper we consider a metric of a rotating black hole in conformal gravity. We calculate the thermodynamical quantities for this rotating black hole including Hawking temperature and entropy in four dimensional space-time, as we obtain the effective value of Komar angular momentum. The result is valid on the event horizon of the black hole, and at any radial distance out of it. Also we verify that the first law of thermodynamics will be held for this type of black hole.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
