GUP corrections to black hole thermodynamics in the extended phase space approach
arXiv:2302.09137 · doi:10.1142/S0218271822501255
Abstract
In this work, we study corrections to black hole temperature and entropy in the context of the generalized uncertainty principle. In particular, we obtain corrected asymptotically anti de-Sitter black hole solutions following the extended phase space scheme in which the cosmological constant is considered as a thermodynamic pressure satisfying certain equation of state. Among all the possibilities, we consider that the cosmological pressure satisfies either a Polytropic or a Chaplygin equation of state. The physical plausibility of the solutions is studied based on the energy conditions and the associated heat capacity.
References in corpus (9)
- Universality of Quantum Gravity Corrections
- Discreteness of Space from the Generalized Uncertainty Principle
- The effects of minimal length and maximal momentum on the transition rate of ultra cold neutrons in gravitational field
- Thermodynamics and P-v criticality of Bardeen-AdS Black Hole in 4-D Einstein-Gauss-Bonnet Gravity
- Black hole thermodynamics with generalized uncertainty principle
- Semiclassical corrections to black hole entropy and the generalized uncertainty principle
- Generalized uncertainty principle and Asymptotic Safe gravity
- GUP modified Hawking Radiation and Transmission/Reflection Coefficients of Rotating Polytropic Black Hole
- Generalised Uncertainty Relations and the Problem of Dark Energy