Horizon of quantum black holes in various dimensions

We adapt the horizon wave-function formalism to describe massive static spherically symmetric sources in a general (1+D)-dimensional space-time, for D>3 and including the D=1 case. We find that the probability PBH that such objects are (quantum) black holes behaves similarly to the probability in...

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Bibliographic Details
Main Authors: Roberto Casadio, Rogerio T. Cavalcanti, Andrea Giugno, Jonas Mureika
Format: Article
Language:English
Published: Elsevier 2016-09-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269316302957