Prospects for gravitational wave and ultra-light dark matter detection with binary resonances beyond the secular approximation

arXiv:2504.16988 · gr-qc, astro-ph.CO, astro-ph.IM, hep-ph · Submitted 2025-04-23 · Read on arXiv

gr-qc, astro-ph.CO, astro-ph.IM, hep-ph

Submitted: 2025-04-23

Updated: 2026-09-23

Comments: 37 pages, 19 figures. Updated to journal published version

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

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