Investigation on the stability and quantum phase transition of the charged rotating Kiselev black hole embedded in quintessence field with quantum fluctuation of entropy
From MaRDI portal
Publication:6489957
DOI10.1142/S021988782450021XMaRDI QIDQ6489957
Mayukh Bandyopadhyay, Ritabrata Biswas
Publication date: 22 April 2024
Published in: International Journal of Geometric Methods in Modern Physics (Search for Journal in Brave)
black hole thermodynamicscharged rotating black holesquintessence fieldgeneralised uncertainty principle
Black holes (83C57) Methods of quantum field theory in general relativity and gravitational theory (83C47)
Cites Work
- Entropy of the Schwarzschild black hole to all orders in the Planck length
- Particle creation by black holes
- Quantum-corrected black hole thermodynamics to all orders in the Planck length
- Charged dilaton, energy, momentum and angular-momentum in teleparallel theory equivalent to general relativity
- Charged axially symmetric solution and energy in teleparallel theory equivalent to general relativity
- Universality of quantum entropy for extreme black holes
- The generalized uncertainty principle and black hole remnants
- GUP parameter from quantum corrections to the Newtonian potential
- Generalized uncertainty principle and angular momentum
- Quantum gravity effects on Hořava-Lifshitz black hole
- Black holes in the Einstein-Gauss-Bonnet theory and the geometry of their thermodynamics. II
- Thermal fluctuations of AdS black holes in three-dimensional rainbow gravity
- On the position representation of Pedram's higher order GUP
- Minimal length scale scenarios for quantum gravity
- The entropy of the noncommutative acoustic black hole based on generalized uncertainty principle
- Quantum-corrected self-dual black hole entropy in tunneling formalism with GUP
- Testing quantum gravity through dumb holes
- The four laws of black hole mechanics
- Counting dyons in \(N=4\) string theory
- REISSNER–NORDSTRÖM SOLUTIONS AND ENERGY IN TELEPARALLEL THEORY
- REISSNER–NORDSTRÖM SPACE–TIME IN THE TETRAD THEORY OF GRAVITATION
- Spherically symmetric black-hole entropy without brick walls
- Will we observe black holes at the LHC?
- General logarithmic corrections to black-hole entropy
- Black-hole entropy in loop quantum gravity
- Quintessence and black holes
- Holographic principle and string cosmology
- Repulsive gravitational force and quintessence field in f(T) gravity: How anisotropic compact stars in strong energy condition behave
- Rotating AdS black holes in Maxwell- f ( T ) gravity
- Quantum corrections to a finite temperature BIon
- KERR–NEWMAN SOLUTION AND ENERGY IN TELEPARALLEL EQUIVALENT OF EINSTEIN THEORY
- Black Holes and Entropy
- Black hole explosions?
- Quantized Space-Time
- The Electromagnetic Field in Quantized Space-Time
- Holographic principle in the closed universe: a resolution with negative pressure matter
Related Items (2)
Isolated compact star \(RXJ 1856.5 - 3754\) in \(f(R, T)\) modified gravity in Tolman-Kuchowicz spacetime ⋮ Investigating the equation-of-state, stability and mass-radius relationship of anisotropic and massive neutron stars embedded in \(f(R, T)\) modified gravity
This page was built for publication: Investigation on the stability and quantum phase transition of the charged rotating Kiselev black hole embedded in quintessence field with quantum fluctuation of entropy