Spectroscopy of an AdS Reissner-Nordstrom black hole
C. Dappiaggi, S. Raschi
TL;DR
This paper extends black hole spectroscopy to AdS Reissner-Nordstrom black holes, deriving their area spectrum using Hamiltonian methods in a spacetime with negative cosmological constant.
Contribution
It introduces a Hamiltonian-based method to determine the area spectrum of charged black holes in AdS spacetime, expanding previous flat spacetime results.
Findings
Derived the area spectrum for AdS Reissner-Nordstrom black holes.
Extended black hole spectroscopy to include negative cosmological constant.
Provided a new framework for quantizing black hole horizons in AdS spacetime.
Abstract
In the framework of black hole spectroscopy, we extend the results obtained for a charged black hole in an asymptotically flat spacetime to the scenario with non vanishing negative cosmological constant. In particular, exploiting Hamiltonian techniques, we construct the area spectrum for an AdS Reissner-Nordstrom black hole.
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