1993/01/25 by M. Campanelli, C. O. Lousto · 1 citation
Physics and Astronomy · #gr-qc #astro-ph #hep-th
paper · pdf · doi:10.1142/s0218271893000325
published as Int.J.Mod.Phys.D2:451-462,1993 · 13pages, Plain Tex
arxiv created 1993/01/25 · arxiv updated 2010/11/01
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.