PreprintCC BY 4.0arXiv
Black hole sensitivity in Einstein--aether theory
Abstract
We numerically find the solutions for slowly moving Schwarzschild black holes in Einstein--aether theory. We use these solutions to compute the sensitivity parameter which describes the coupling of the black hole to the aether field within point-particle effective theory. A simple analytic approximation for the dependence of the sensitivity on the Einstein--aether parameters is derived.
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BibTeX
@misc{kidnew2026black,
title = {{Black hole sensitivity in Einstein--aether theory}},
author = {Morgan Kidnew and Andrew Kovachik and Sergey Sibiryakov},
howpublished = {arXiv},
year = {2026},
month = oct,
doi = {10.48550/arxiv.2610.00503},
eprint = {2610.00503},
archivePrefix = {arXiv},
url = {https://arxiv.org/abs/2610.00503},
note = {CC BY 4.0},
}
RIS
TY - UNPB
TI - Black hole sensitivity in Einstein--aether theory
AU - Morgan Kidnew
AU - Andrew Kovachik
AU - Sergey Sibiryakov
PY - 2026
DA - 2026/10/01
PB - arXiv
DO - 10.48550/arxiv.2610.00503
UR - https://arxiv.org/abs/2610.00503
AB - We numerically find the solutions for slowly moving Schwarzschild black holes in Einstein--aether theory. We use these solutions to compute the sensitivity parameter which describes the coupling of the black hole to the aether field within point-particle effective theory. A simple analytic approximation for the dependence of the sensitivity on the Einstein--aether parameters is derived.
ER -