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"Are Black Holes in Brans-Dicke Theory precisely the same as in General Relativity?"

We study a three-parameters family of solutions of the Brans-Dicke field equations. They are static and spherically symmetric. We find the range of parameters for which this solution represents a black hole different from the Schwarzschild one. We find a subfamily of solutions which agrees with experiments and observations in the solar system. We discuss some astrophysical applications and the consequences on the "no hair" theorems for black holes.

preprint1993arXivOpen access
M. CampanelliC. O. Lousto
astro-phgr-qchep-th
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M. CampanelliC. O. Lousto

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