Kiselev Black holes in quantum fluctuation modified gravity
arXiv:2411.15854 · doi:10.1140/epjp/s13360-026-07312-5
Abstract
We obtain a new general solution for the gravitational field equations in quantum fluctuation modified gravity, which reduces to different classes of black holes surrounded by fluids, by taking some specific values of the parameter of the equation of state. We discuss the strong energy condition in a general way and also for some special cases of different fluids. In addition, the Hawking temperature associated to the horizons of solutions and constraints on the parameter characterizing the fluctuation of metric are taken into account in our analysis.
20 pages, 11 figures
References in corpus (25)
- Quintessence and black holes
- Twilight for the energy conditions?
- Dirty blackholes: Thermodynamics and horizon structure
- Black Hole Solutions Surrounded by Perfect Fluid in Rastall Theory
- Rotating black hole and quintessence
- The Kiselev black hole is neither perfect fluid, nor is it quintessence
- Kerr-Newman-AdS Black Hole In Quintessential Dark Energy
- Modified gravity from the quantum part of the metric
- Cosmological implications of modified gravity induced by quantum metric fluctuations
- Lovelock black holes surrounded by quintessence
- Semiclassical energy conditions for quantum vacuum states
- Kerr-Newman-NUT-Kiselev black holes in Rastall theory of gravity and Kerr/CFT Correspondence
- Classical and quantum flux energy conditions for quantum vacuum states
- Modified gravity from the nonperturbative quantization of a metric
- Effects of quantum fluctuations of metric on the universe
- Noncommutative Schwarzschild black hole surrounded by quintessence: Thermodynamics, Shadows and Quasinormal modes
- Quantum correlations for the metric
- Hairy Kiselev Black Hole Solutions
- Thermodynamics of Schwarzschild black hole surrounded by quintessence in gravity's rainbow
- Euler-Heisenberg black hole surrounded by quintessence in the background of perfect fluid dark matter: Thermodynamics, Shadows and Quasinormal modes
- Modified Teleparallel Gravity induced by quantum fluctuations
- Black hole solutions in modified gravity induced by quantum metric fluctuations
- Confronting quantum-corrected teleparallel cosmology with observations
- Astrophysical and electromagnetic emissivity properties of black holes surrounded by a quintessence type exotic fluid in the Scalar-Vector-Tensor Modified Gravity
- Baryogenesis in quantum fluctuation modified gravity