Teorico

Quantum integrable black holes

by Roberto Casadio (Istituto Nazionale di Fisica Nucleare)

Europe/Rome
Aula ConversI (Dipartimento di Fisica - Ed. G.Marconi)

Aula ConversI

Dipartimento di Fisica - Ed. G.Marconi

Description

It is common to assume that quantum gravity belongs at the Planck scale, but a possibly much larger width for the ground state emerges in the (non-perturbative) quantisation of the Oppenheimer-Snyder model of dust collapse that naturally recovers Bekenstein’s area law. The effective geometry for such quantum black holes can then be obtained from coherent states which describe integrable singularities without inner horizons. The extension to quantum (differentially) rotating black holes with similar properties is also described. 

Organised by

G.Franciolini, P.Pani