Mass Independent Area (or Entropy) and Thermodynamic Volume Products in Conformal Gravity
Parthapratim Pradhan

TL;DR
This paper explores the thermodynamic properties of conformal gravity black holes, deriving universal relations for area, entropy, and volume, and analyzing phase transitions in various spacetime backgrounds.
Contribution
It introduces mass-independent area and volume relations in conformal gravity, extending thermodynamic analysis to de-Sitter and anti de-Sitter cases with new phase transition insights.
Findings
Derived universal area (entropy) relations for conformal gravity black holes.
Established thermodynamic volume relations in extended phase space.
Identified conditions for second order phase transitions in different spacetime backgrounds.
Abstract
In this work we investigate the thermodynamic properties of conformal gravity in four dimensions. We compute the \emph{area(or entropy) functional} relation for this black hole. We consider both de-Sitter (dS) and anti de-Sitter (AdS) cases. We derive the \emph{Cosmic-Censorship-Inequality} which is an important relation in general relativity that relates the total mass of a spacetime to the area of all the black hole horizons. Local thermodynamic stability is studied by computing the specific heat. The second order phase transition occurs at a certain condition. Various type of second order phase structure has been given for various values of and the cosmological constant in the Appendix. When , one obtains the result of Schwarzschild-dS and Schwarzschild-AdS cases. In the limit , one obtains the result of Grumiller space-time. Where is non-trivial Rindler…
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