Dual Dressed Black Holes as the end point of the Charged Superradiant instability in Yang Mills
arXiv:2409.18178 · doi:10.21468/SciPostPhys.18.4.137
Abstract
Charged Black holes in suffer from superradiant instabilities over a range of energies. Hairy black hole solutions (constructed within gauged supergravity) have previously been proposed as endpoints to this instability. We demonstrate that these hairy black holes are themselves unstable to the emission of large dual giant gravitons. We propose that the endpoint to this instability is given by Dual Dressed Black Holes (DDBH)s; configurations consisting of one, two, or three very large dual giant gravitons surrounding a core black hole with one, two, or three chemical potentials equal to unity. The dual giants each live at radial coordinates of order and each carry charge of order . The large separation makes DDBHs a very weakly interacting mix of their components and allows for a simple computation of their thermodynamics. We conjecture that DDBHs dominate the phase diagram of Yang-Mills over a range of energies around the BPS plane, and provide an explicit construction of this phase diagram, briefly discussing the interplay with supersymmetry. We develop the quantum description of dual giants around black hole backgrounds and explicitly verify that DDBHs are stable to potential tunneling instabilities, precisely when the chemical potentials of the core black holes equal unity. We also construct the 10-dimensional DDBH bulk solutions.
arXiv comment86 pages + Appendices, 16 figures; Corrected typos, added references, updated the text in section 5.1 and added 4 Figures in Section 3.4 and Appendix D.1
References in corpus (48)
- A Stress Tensor for Anti-de Sitter Gravity
- Building an AdS/CFT superconductor
- Nonlinear Fluid Dynamics from Gravity
- Holographic Superconductors
- Breaking an Abelian gauge symmetry near a black hole horizon
- Bubbling AdS space and 1/2 BPS geometries
- Embedding AdS Black Holes in Ten and Eleven Dimensions
- Invasion of the Giant Gravitons from Anti-de Sitter Space
- Towards strange metallic holography
- Holographic Probes of Anti-de Sitter Spacetimes
- General supersymmetric AdS5 black holes
- Large branes in AdS and their field theory dual
- Supersymmetric AdS5 black holes
- SUSY and Goliath
- An extremization principle for the entropy of rotating BPS black holes in AdS
- Charged Kerr-de Sitter Black Holes in Five Dimensions
- A Bohr-Sommerfeld quantization formula for quasinormal frequencies of AdS black holes
- Hairy black holes and solitons in global AdS 5
- Forced Fluid Dynamics from Gravity
- Phase Diagram of N=4 Super-Yang-Mills Theory with R-Symmetry Chemical Potentials
- A theory of first order dissipative superfluid dynamics
- Small Hairy Black Holes in Global AdS Spacetime
- Small Hairy Black Holes in
- Charged Rotating Black Holes in Five Dimensional U(1)^3 Gauged N=2 Supergravity
- Dissipative superfluid dynamics from gravity
- Bubbling AdS and droplet descriptions of BPS geometries in IIB supergravity
- Holographic Stress Tensors for Kerr-AdS Black Holes
- Counting 1/8-BPS Dual-Giants
- A gravity interpretation for the Bethe Ansatz expansion of the SYM index
- Words to describe a black hole
- Constraints on Superfluid Hydrodynamics from Equilibrium Partition Functions
- Emergent Quantum Near-Criticality from Baryonic Black Branes
- Membranes with Topological Charge and AdS4/CFT3 Correspondence
- Hairy Black Holes in AdS
- Rotating Hairy Black Holes in AdSS
- Supersymmetric States in M5/M2 CFTs
- Decoding stringy near-supersymmetric black holes
- Novel color superconducting phases of = 4 super Yang-Mills at strong coupling
- Stringy corrections to the entropy of electrically charged supersymmetric black holes with asymptotics
- Metastability of R-Charged Black Holes
- A Supersymmetric Color Superconductor from Holography
- On uniqueness of charged Kerr-AdS black holes in five dimensions
- Brane nucleation instabilities in non-AdS/non-CFT
- New phases of SYM at finite chemical potential
- Holographic Higgs Phases
- Following Black Hole States
- The Kerr-Fermi Sea
- Holographic covering and the fortuity of black holes