Black Holes with Surrounding Matter in Scalar-Tensor Theories

Vitor Cardose, Paolo Pani, Thomas P. Sotiriou, I.P. Carucci

77 Citationer (Scopus)

Abstract

We uncover two mechanisms that can render Kerr black holes unstable in scalar-tensor gravity, both associated with the presence of matter in the vicinity of the black hole and the fact that this introduces an effective mass for the scalar. Our results highlight the importance of understanding the structure of spacetime in realistic, astrophysical black holes in scalar-tensor theories.

OriginalsprogEngelsk
Artikelnummer111101
TidsskriftPhysical Review Letters
Vol/bind111
Udgave nummer11
ISSN0031-9007
DOI
StatusUdgivet - 10 sep. 2013

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