Hawking radiation by spherically-symmetric static black holes for all spins: Teukolsky equations and potentials
Résumé
In the context of the dynamics and stability of black holes in modified theories of gravity, we derive the Teukolsky equations for massless fields of all spins in general spherically symmetric and static metrics. We then compute the short-ranged potentials associated with the radial dynamics of spin 1 and spin 1/2 fields, thereby completing the existing literature on spin 0 and 2. These potentials are crucial for the computation of Hawking radiation and quasinormal modes emitted by black holes. In addition to the Schwarzschild metric, we apply these results and give the explicit formulas for the radial potentials in the case of charged (Reissner–Nordström) black holes, higher-dimensional black holes, and polymerized black holes arising from loop quantum gravity. These results are, in particular, relevant and applicable to a large class of regular black hole metrics. The phenomenological applications of these formulas will be the subject of a companion paper.
Mots clés
General relativity
alternative theories of gravity
radiation: Hawking
black hole: static
black hole: higher-dimensional
black hole: stability
black hole: charge
spin: 1/2
spin: 0
spin: 1
spin: 2
metric: Schwarzschild
quantum gravity: loop space
Teukolsky equation
Reissner-Nordstroem
gravitation
symmetry: rotation
gravitation: model
field theory: massless
quasinormal mode
quantization: polymer
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