Exact Black-Hole Solution With Self-Interacting Scalar Field
广义相对论与量子宇宙学
2010-04-06 v3 高能物理 - 理论
摘要
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.
引用
@article{arxiv.gr-qc/9502011,
title = {Exact Black-Hole Solution With Self-Interacting Scalar Field},
author = {Olaf Bechmann and Olaf Lechtenfeld},
journal= {arXiv preprint arXiv:gr-qc/9502011},
year = {2010}
}
备注
10 pages, uuencoded ps-file, 130 kB, revised: additional Comments and references, minor corrections, notational changes