Charged Nariai Black Holes With a Dilaton
arXiv:gr-qc/9608053 · doi:10.1103/PhysRevD.55.3614
Abstract
The Reissner-Nordstrom-de Sitter black holes of standard Einstein-Maxwell theory with a cosmological constant have no analogue in dilatonic theories with a Liouville potential. The only exception are the solutions of maximal mass, the Charged Nariai solutions. We show that the structure of the solution space of the Dilatonic Charged Nariai black holes is quite different from the non-dilatonic case. Its dimensionality depends on the exponential coupling constants of the dilaton. We discuss the possibility of pair creating such black holes on a suitable background. We find conditions for the existence of Charged Nariai solutions in theories with general dilaton potentials, and consider specifically a massive dilaton.
20 pages, LaTeX, 4 figures, submitted to Phys. Rev. D
References in corpus (2)
Cited by in corpus (43)
- Loop Quantum Dynamics of the Schwarzschild Interior
- Tunnelling Methods and Hawking's radiation: achievements and prospects
- (Anti-)Evaporation of Schwarzschild-de Sitter Black Holes
- Festina Lente: EFT Constraints from Charged Black Hole Evaporation in de Sitter
- Cosmological Pair Production of Charged and Rotating Black Holes
- Dynamical compactification from de Sitter space
- Emergence of product of constant curvature spaces in loop quantum cosmology
- Quantum Global Structure of de Sitter Space
- Nariai black holes with quintessence
- Cold, ultracold and Nariai black holes with quintessence
- The extremal limits of the C-metric: Nariai, Bertotti-Robinson and anti-Nariai C-metrics
- Complex Instantons and Charged Rotating Black Hole Pair Creation
- Improved Effective Dynamics of Loop-Quantum-Gravity Black Hole and Nariai Limit
- Impulsive waves in the Nariai universe
- Stability of the Schwarzschild Interior in Loop Quantum Gravity
- Pair creation of de Sitter black holes on a cosmic string background
- Codazzi tensors and their space-times, and Cotton gravity
- A dS obstruction and its phenomenological consequences
- On Curvature properties of Nariai Spacetimes
- Understanding quantum black holes from quantum reduced loop gravity
- Pair creation of higher dimensional black holes on a de Sitter background
- Quantum generation of Schwarzschild-de Sitter (Nariai) black holes in effective dilaton-Maxwell gravity
- A quasilocal Hamiltonian for gravity with classical and quantum applications
- Born-Infeld-de Sitter gravity: Cold, ultracold and Nariai black holes
- Dilatonic (Anti-)de Sitter Black Holes and Weak Gravity Conjecture
- Nonexistence of quantum black and white hole horizons in an improved dynamic approach
- Nonextreme black holes near the extreme state and acceleration horizons: thermodynamics and quantum-corrected geometry
- Primordial black holes in a dimensionally reduced universe
- Pair creation of anti-de Sitter black holes on a cosmic string background
- Melvin solution with a dilaton potential
- Min-max minimal surfaces, horizons and electrostatic systems
- The Entropy Function for the Black Holes of Nariai Class
- Charged dilaton black hole with multiple Liouville potentials and gauge fields
- Black Hole Solutions and Pair Creation of Black Holes in Three, Four and Higher Dimensional Spacetimes
- Pair Creation of Dilaton Black Holes in Extended Inflation
- Charged Nariai black holes on the dark bubble
- Primordial black holes in a dimensionally oxidizing Universe
- Hitchhiker's Guide to the Swampland: The Cosmologist's Handbook to the string-theoretical Swampland Programme
- A note on Strong Cosmic Censorship and its violation in Reissner-Nordström de Sitter black hole space-times
- Supersymmetric configurations in Euclidean Freedman-Schwarz model
- The Fate of Nucleated Black Holes in de Sitter Quantum Gravity
- Planckian charged black holes and their cosmological ramifications
- Reissner-Nordström black holes in de Sitter space-time: bounds with quasinormal frequencies