static, charged black holes, strings and rings with resonant, scalar -hair
arXiv:2207.13114 · doi:10.1007/JHEP10(2022)153
Abstract
A mechanism for circumventing the Mayo-Bekenstein no-hair theorem allows endowing four dimensional asymptotically flat, spherical, electro-vacuum black holes with a minimally coupled -gauged scalar field profile: -. The scalar field must be massive, self-interacting and obey a {\it resonance condition} at the threshold of (charged) superradiance. We establish generality for this mechanism by endowing three different types of static black objects with scalar hair, within a Einstein-Maxwell-gauged scalar field model: asymptotically flat black holes and black rings; and black strings which asymptote to a Kaluza-Klein vacuum. These -hairy black objects share many of the features of their counterparts. In particular, the scalar field is subject to a resonance condition and possesses a -ball type potential. For the static black ring, the charged scalar hair can balance it, yielding solutions that are singularity free on and outside the horizon.
arXiv comment30 pages, 8 figures
References in corpus (66)
- Black Strings and p-Branes are Unstable
- A rotating black ring in five dimensions
- Breaking an Abelian gauge symmetry near a black hole horizon
- Kerr black holes with scalar hair
- Black Holes in Higher Dimensions
- Superradiant Instability and Backreaction of Massive Vector Fields around Kerr Black Holes
- Generalized Weyl Solutions
- Kerr black holes with Proca hair
- Static Axisymmetric Vacuum Solutions and Non-Uniform Black Strings
- Stationary Scalar Clouds Around Rotating Black Holes
- On non-uniform black branes
- No hair for spherical black holes: charged and nonminimally coupled scalar field with self--interaction
- Kerr-Newman scalar clouds
- Explosion and final state of an unstable Reissner-Nordstrom black hole
- Black holes with only one Killing field
- Black Holes and Scalar Fields
- Kerr-Newman black holes with stationary charged scalar clouds
- Connecting black holes and black strings
- Kerr black holes with self-interacting scalar hair: hairier but not heavier
- Hairy black holes and solitons in global AdS 5
- A new spin on black hole hair
- Kaluza-Klein Black Holes with Squashed Horizons
- Non-linear Q-clouds around Kerr black holes
- Small Hairy Black Holes in Global AdS Spacetime
- Small Hairy Black Holes in
- Kerr black holes with synchronised hair: an analytic model and dynamical formation
- Myers-Perry black holes with scalar hair and a mass gap
- Tension Perturbations of Black Brane Spacetimes
- Stationary scalar configurations around extremal charged black holes
- New Phase Diagram for Black Holes and Strings on Cylinders
- Dynamical formation of a Reissner-Nordström black hole with scalar hair in a cavity
- Caged Black Holes: Black Holes in Compactified Spacetimes I -- Theory
- Kerr-Newman black holes with scalar hair
- New nonuniform black string solutions
- On charged boson stars
- Electrically charged dilatonic black rings
- Myers-Perry black holes with scalar hair and a mass gap: unequal spins
- Hairy black holes and the endpoint of AdS charged superradiance
- Charged Proca Stars
- Excited Kerr black holes with scalar hair
- Spherical electro-vacuum black holes with resonant, scalar -hair
- Spherically Symmetric Scalar Hair for Charged Black Holes
- Black rings in more than five dimensions
- Spinning Kerr black holes with stationary massive scalar clouds: The large-coupling regime
- Black holes with synchronised Proca hair: linear clouds and fundamental non-linear solutions
- Magnetized black holes and black rings in the higher dimensional dilaton gravity
- Charged Q-balls and boson stars and dynamics of charged test particles
- Kerr black holes with synchronised scalar hair and higher azimuthal harmonic index
- Kerr black holes with parity-odd scalar hair
- A Positivity Theorem for Gravitational Tension in Brane Spacetimes
- On the Bekenstein-Hawking area law for black objects with conical singularities
- Hairy Black Holes in AdS
- Thermodynamical description of stationary, asymptotically flat solutions with conical singularities
- Charged Boson Stars and Vacuum Instabilities
- Symmetry inheritance of scalar fields
- Quasilocal equilibrium condition for black ring
- Black resonators and geons in AdS
- Charged black holes in non-linear Q-clouds with O(3) symmetry
- New generalized nonspherical black hole solutions
- Probing the universality of synchronised hair around rotating black holes with Q-clouds
- Q-stars and charged q-stars
- Higher dimensional black holes
- Generalized Weyl solutions in d=5 Einstein-Gauss-Bonnet theory: the static black ring
- Charged Balanced Black Rings in Five Dimensions
- Black ringoids: spinning balanced black objects in dimensions -- the codimension-two case
- Balancing a static black ring with a phantom scalar field