On the Near Horizon Canonical Quantum Microstates from and Conformal Weyl Gravity
arXiv:1707.05796 · doi:10.3390/universe3030056
Abstract
We compute the full asymptotic symmetry group of black holes belonging to the same equivalence class of solutions within the Conformal Weyl Gravity formalism. We do this within an correspondence and by performing a Robinson-Wilczek two dimensional reduction, thus enabling the construction of an effective quantum theory of the remaining field content. The resulting energy momentum tensors generate asymptotic Virasoro algebras, to -wave, with calculable central extensions. These centers in conjunction with their proper regularized lowest Virasoro eigen-modes yield the Bekenstein-Hawking black hole entropy via the statistical Cardy formula. We also analyze quantum holomorphic fluxes of the dual CFTs in the near horizon, giving rise to finite Hawking temperatures weighted by the central charges of the respective black hole spacetimes. We conclude with a discussion and outlook for future work.
18 pages, no figures. Accepted version contributed to mdpi's Universe collection on open questions in black hole physics
References in corpus (7)
- Anomalies, Hawking Radiations and Regularity in Rotating Black Holes
- No Dynamics in the Extremal Kerr Throat
- Hawking radiation from rotating black holes in anti-de Sitter spaces via gauge and gravitational anomalies
- Gravitational anomalies: a recipe for Hawking radiation
- Entropy and Temperature From Black-Hole/Near-Horizon-CFT Duality
- A Near Horizon CFT Dual for Kerr-Newman-
- Hawking radiation, chirality, and the principle of effective theory of gravity