Quantum rotating black holes
Roberto CasadioDipartimento di Fisica e Astronomia, Università di Bologna, via Irnerio 46, 40126, Bologna, ItalyAndrea GiustiInstitute for Theoretical Physics, ETH Zurich, Wolfgang-Pauli-Strasse 27, 8093, Zurich, SwitzerlandJorge OvalleResearch Centre of Theoretical Physics and Astrophysics, Institute of Physics, Silesian University in Opava, CZ-746 01, Opava, Czech Republic
2023en
ABI
Аннотация
A bstract We consider black holes generically sourced by quantum matter described by regular wavefunctions. This allows for integrable effective energy densities and the removal of Cauchy horizons in spherically symmetric configurations. Moreover, we identify the ultrarigid rotation of the Kerr spacetime as causing the existence of an inner horizon in rotating systems, and describe general properties for quantum matter cores at the centre of rotating black holes with integrable singularities and no Cauchy horizon.
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