Scalar probe spectra on new rotating black holes and solitons in 5D Einstein-Gauss-Bonnet gravity give gapped mass towers, real soliton frequencies, and rotation-dependent damping.
A black hole solution in conformal supergravity
1 Pith paper cite this work. Polarity classification is still indexing.
abstract
We present a three-parameter family of analytic black-hole solutions in the bosonic sector of a four-dimensional supersymmetric model with matter fields in the adjoint representation. The solutions are endowed with curvature and torsional singularities which are both surrounded by an event horizon. They are asymptotically Lorentz flat, representing the torsional generalization of the Riegert black hole in conformal gravity. We compute the partition function to first order in the saddle-point approximation which turns out to be finite without any reference to boundary counterterms. We find a non-maximmally symmetric thermalized ground state, whose existence is relevant when studying Hawking-Page phase transitions. Finally, we discuss future directions regarding its extended phase space.
fields
hep-th 1years
2024 1verdicts
CONDITIONAL 1representative citing papers
citing papers explorer
-
(Quasi-)normal modes of rotating black holes and new solitons in Einstein-Gauss-Bonnet
Scalar probe spectra on new rotating black holes and solitons in 5D Einstein-Gauss-Bonnet gravity give gapped mass towers, real soliton frequencies, and rotation-dependent damping.