Static and Dynamic Charged Black Holes
arXiv:1908.07970 · doi:10.1140/epjc/s10052-019-7477-x
Abstract
We consider a class of Einstein-Maxwell-dilaton theories in general dimensions and construct both static and dynamic charged black holes. We adopt the reverse engineering procedure and make a specific ansatz for the scalar field and then derive the necessary scalar potential and the non-minimal coupling function between the scalar and the Maxwell field. The resulting static black holes contain mass and electric charge as integration constants. We find that some of the static solutions can be promoted to become dynamical ones in the Eddington-Finkelstein-like coordinates. The collapse solutions describe the evolution from a smaller charged black hole to a larger black hole state, driven by the scalar field.
arXiv comment26pages, 2figures
References in corpus (26)
- Gauge Theory Correlators from Non-Critical String Theory
- The Large N Limit of Superconformal Field Theories and Supergravity
- Enthalpy and the Mechanics of AdS Black Holes
- Black Hole Enthalpy and an Entropy Inequality for the Thermodynamic Volume
- On weakly turbulent instability of anti-de Sitter space
- Thermalization of Strongly Coupled Field Theories
- Holographic Thermalization
- Exact black hole solution with a minimally coupled scalar field
- Black holes and asymptotics of 2+1 gravity coupled to a scalar field
- Boson Stars in AdS
- Scalar Collapse in AdS
- Four-Dimensional Asymptotically AdS Black Holes with Scalar Hair
- Scalar Hairy Black Holes in General Dimensions
- Hairy planar black holes in higher dimensions
- On holographic thermalization and gravitational collapse of tachyonic scalar fields
- Exact Black Hole Formation in Asymptotically (A)dS and Flat Spacetimes
- Static and Dynamic Hairy Planar Black Holes
- (Super-)renormalizably dressed black holes
- No-Go Theorem in Spacetimes with Two Commuting Spacelike Killing Vectors
- Exact black hole formation in three dimensions
- Critical Behavior in a Massless Scalar Field Collapse with Self-interaction Potential
- Butterfly Velocity Bound and Reverse Isoperimetric Inequality
- Exact Collapse Solutions in D=4, N=4 Gauged Supergravity and Their Generalizations
- Exact formation of hairy planar black holes
- AdS and Lifshitz Scalar Hairy Black Holes in Gauss-Bonnet Gravity
- Exact black-hole formation with a conformally coupled scalar field in three dimensions
Cited by in corpus (5)
- Charged Ellis Wormhole and Black Bounce
- Trapping Horizons of the Evolving Charged Wormhole and Black Bounce
- Microlensing effect of charged spherically symmetric wormhole
- Microlensing and event rate of static spherically symmetric wormhole
- Perturbations of Einstein--Maxwell--phantom spacetime: Instabilities of charged Ellis--Bronnikov wormholes and quasinormal modes of black holes