Exact Black-Hole Solution With Self-Interacting Scalar Field
Olaf Bechmann, Olaf Lechtenfeld (Univ. of Hannover, Germany)

TL;DR
This paper presents a new exact black-hole solution in Einstein gravity coupled to a self-interacting scalar field, featuring scalar hair with a complex potential, supported by analytical and numerical analysis.
Contribution
It introduces a novel black-hole solution with scalar hair and a unique potential, expanding the set of known solutions in scalar-tensor gravity.
Findings
Explicit construction of a black-hole solution with scalar hair.
Analysis of a triple-well scalar potential with non-analytic minimum.
Numerical and series expansion data supporting the solution.
Abstract
Einstein gravity minimally coupled to a self-interacting scalar field is investigated in the static and isotropic situation. We explicitly construct in partially closed form a new black-hole solution with exponentially decaying scalar hair. The symmetric interaction potential has both signs and a triple-well shape with a smooth but non-analytic minimum at vanishing field. We present numerical data as well as double series expansions around spatial infinity.
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