Where are the BTZ Black Hole Degrees of Freedom? The Rotating Case

Abstract

Recent work has shown that the entropy of the non-rotating BTZ black hole can be derived from a dual conformal description at any spatial location. In this followup it is shown that a dual conformal description exists at any spatial location for the rotating BTZ black hole as well. As in the non-rotating case, two copies of the central charge $c^{\pm }=3\ell /2G$ are recovered and the microcanonical Cardy formula yields the correct Bekenstein-Hawking entropy.

10 pages, 1 figure; fixed/added references

References in corpus (3)

• Effective Conformal Descriptions of Black Hole Entropy
• Liouville theory beyond the cosmological horizon
• Where are the BTZ Black Hole Degrees of Freedom?

Cited by in corpus (3)

• Symplectic and Killing Symmetries of AdS${}_3$ Gravity: Holographic vs Boundary Gravitons
• On 3d Bulk Geometry of Virasoro Coadjoint Orbits: Orbit invariant charges and Virasoro hair on locally AdS3 geometries
• Horizon Fluffs: Near Horizon Soft Hairs as Microstates of Generic AdS3 Black Holes