Abstract
Scalar fields coupled to the Gauss-Bonnet invariant evade the known no-hair theorems and have nontrivial configurations around black holes. We focus on a scalar field that couples linearly to the Gauss-Bonnet invariant and hence exhibits shift symmetry. We study its dynamical evolution and the formation of scalar hair in a Schwarzschild background. We show that the evolution eventually settles to the known static hairy solutions in the appropriate limit.
Original language | English (US) |
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Article number | 121503 |
Journal | Physical Review D |
Volume | 94 |
Issue number | 12 |
DOIs | |
State | Published - Dec 28 2016 |
Externally published | Yes |
ASJC Scopus subject areas
- Physics and Astronomy (miscellaneous)