riassunto2

MG12 - Talk detail
 

Back to previous page

 Participant 

Stefanov, Ivan

Institution

Sofia University, Faculty of Physics  - 5 James Bourchier Blvd. - Sofia - - Bulgaria

Session

Talk

Abstract

MGAT8

Phases of 4D black holes in scalar-tensor theories of gravity with non-linear electrodynamics

According to the no-scalar-hair conjecture, black-hole solutions in scalar-tensor theories of gravity (STT) can be fully classifed by their asymptotic preserved charges - mass, electric (magnetic) charge and angular momentum, exactly as in General Relativity (GR). This makes the black holes in STT undistinguishable from those in GR for a distant observer. There is a series of theorems that confirm the conjecture in the vacuum and electrovacuum cases. The present talk is dedicated to new non-unique, numerical solutions that serve as counter-examples of the no-scalar-hair conjecture. They describe charged black holes coupled to non-linear electrodynamics in special classes of STT that posses primary scalar hair.

Back to previous page