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We show that, for signal-to-noise ratios $\\lesssim 100$, LISA can distinguish gravitational waveforms from binaries embedded in such halo overdensities. Our analysis indicates that LISA can probe","authors_text":"Carlos Palenzuela Luque, Samuel G\\'omez G\\'omez, Xisco Jimenez Forteza","cross_cats":["astro-ph.HE","hep-ph"],"headline":"Axion-like particles forming halos around black holes cause detectable dephasing in LISA waveforms from inspiraling binaries.","license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2026-05-17T18:33:22Z","title":"Impact of the axion-like self-interactions in gravitational atoms for LISA"},"references":{"count":57,"internal_anchors":6,"resolved_work":57,"sample":[{"cited_arxiv_id":"","doi":"","is_internal_anchor":false,"ref_index":1,"title":"These were calculated by recovering different param- eter injections in logL. 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