The gravitational field of a clump of ultralight axion like particles (ALPs) in its core with a rotating binary system of dwarf stars is computed. It is established that the induced quadrupole mass moment of the clump is controlled parametrically by the Ma/M mass ratio of the axion clump and the the binary core.
@article{arxiv.2407.19782,
title = {Axion halo around a binary system of dwarf stars},
author = {András Patkós},
journal= {arXiv preprint arXiv:2407.19782},
year = {2024}
}
Comments
Contribution to Procs. of Bolyai-Gauss-Lobachevsky 2024 Conference. Reference list updated