Small Black holes vs horizonless solutions in AdS
arXiv:0910.3225 · doi:10.1103/PhysRevD.81.024003
Abstract
It is argued that the appropriate macroscopic description of half-BPS mesonic chiral operators in generic toric gauge theories is in terms of the geometric quantization of smooth horizonless configurations. The relevance of different ensemble macroscopic descriptions is emphasized : lorentzian vs euclidean configurations as (semiclassical) microstates vs saddle points in an euclidean path integral.
10 pages; v2 improved entropy discussion and new references included
References in corpus (20)
- The fuzzball proposal for black holes
- Counting Gauge Invariants: the Plethystic Program
- Sasaki-Einstein Manifolds and Volume Minimisation
- Quantum Entropy Function from AdS(2)/CFT(1) Correspondence
- Gravity solutions for the D1-D5 system with angular momentum
- Black Holes as Effective Geometries
- Mergers and Typical Black Hole Microstates
- Supersymmetric states of N=4 Yang-Mills from giant gravitons
- Gauged supergravity from type IIB string theory on Y^{p,q} manifolds
- Arithmetic of Quantum Entropy Function
- Bubbling AdS and droplet descriptions of BPS geometries in IIB supergravity
- Typicality versus thermality: An analytic distinction
- Dual Giant Gravitons in Sasaki-Einstein Backgrounds
- Brane webs and 1/4-BPS geometries
- A description of 1/4 BPS configurations in minimal type IIB SUGRA
- Quantum geometry and gravitational entropy
- Two Charge System Revisited: Small Black Holes or Horizonless Solutions?
- Strings on conifolds from strong coupling dynamics, part I
- Microstate Dependence of Scattering from the D1-D5 System
- Half BPS states in AdS_5 x Y^{p,q}
Cited by in corpus (6)
- Thermodynamics and Thermodynamic geometry of Park black hole
- Extremal black holes, Holography & Coarse graining
- Hints of Integrability Beyond the Planar Limit: Nontrivial Backgrounds
- Correlations vs connectivity in R-charge
- Area spectrum and thermodynamics of KS black holes in Hořava gravity
- A Universal Behavior of Half BPS Probes in the Superstar Ensemble