On the Equivalence of Brans-Dicke and Einstein Theories with Static Black Holes
Eloy Ay\'on (Grupo de F\'isica Te\'orica, Centro de Matem\'aticas y, F\'isica Te\'orica, ICIMAF, Cuba)

TL;DR
This paper proves that under certain conditions, Brans-Dicke theory with matter of definite-sign trace is equivalent to Einstein gravity with a zero-trace energy-momentum tensor, especially in the context of static black holes.
Contribution
It establishes a no-hair theorem for the Brans-Dicke field, showing equivalence to Einstein gravity under specific conditions for static black holes.
Findings
Brans-Dicke theory reduces to Einstein gravity with T=0 for matter with definite-sign trace.
A no-hair theorem for the Brans-Dicke field in static black hole spacetimes is proven.
Equivalence holds when the trace of the energy-momentum tensor has a definite sign.
Abstract
A `no-hair' theorem for the Brans-Dicke field, in the domain of outer communications of a static black hole, is established, when the trace of the energy-momentum tensor, T, is a definite-sign scalar. This implies that Brans-Dicke theory of gravitation, for matter with T of definite sign, is equivalent to Einstein gravity with the constraint T=0.
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Taxonomy
TopicsBlack Holes and Theoretical Physics · Cosmology and Gravitation Theories · Relativity and Gravitational Theory
