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Coupling Constants as Conserved Charges in Black Hole Thermodynamics
Kamal Hajian1,2, Bayram Tekin2
1Institute of Physics, University of Oldenburg, P.O. Box 2503, D-26111 Oldenburg, Germany.
This study introduces a new method to treat coupling constants in gravity theories as variable parameters, not fixed constants. This approach successfully extends black hole thermodynamics, including the Smarr formula and first law.
Area of Science:
- Theoretical physics
- Gravitational physics
- Black hole thermodynamics
Background:
- The Smarr formula for black holes is essential for understanding their thermodynamics.
- Coupling constants in gravity theories are typically fixed parameters, limiting their role in solutions.
- Existing methods do not adequately incorporate these constants into black hole thermodynamics.
Purpose of the Study:
- To develop a robust method for treating coupling constants as free parameters in gravity theories.
- To systematically extend the first law and Smarr formula for black holes.
- To apply the method to a quadratic gravity theory as a case study.
Main Methods:
- Introducing auxiliary scalar and gauge fields for each coupling constant.
- Identifying couplings as conserved charges of implemented gauge symmetry.
- Defining conjugate chemical potentials as electric potentials on the black hole horizon.
Main Results:
- A generalized framework for black hole thermodynamics that incorporates variable coupling constants.
- The derived conserved charges and their conjugate potentials systematically extend the first law and Smarr formula.
- Successful application to a quadratic gravity theory, demonstrating the method's efficacy.
Conclusions:
- The presented method provides a powerful tool for analyzing black hole thermodynamics in generic gravity theories.
- Treating coupling constants as dynamical parameters offers new insights into black hole solutions.
- This approach unifies the treatment of constants and variables in gravitational theories.
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