{"paper":{"title":"Distinguishing black-hole spin-orbit resonances by their gravitational-wave signatures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Davide Gerosa, Emanuele Berti, Michael Kesden, Richard O'Shaughnessy, Ulrich Sperhake","submitted_at":"2014-03-27T17:50:25Z","abstract_excerpt":"If binary black holes form following the successive core collapses of sufficiently massive binary stars, precessional dynamics may align their spins $\\mathbf S_1$ and $\\mathbf S_2$ and the orbital angular momentum $\\mathbf L$ into a plane in which they jointly precess about the total angular momentum $\\mathbf J$. These spin orientations are known as spin-orbit resonances since $\\mathbf S_1$, $\\mathbf S_2$, and $\\mathbf L$ all precess at the same frequency to maintain their planar configuration. Two families of such spin-orbit resonances exist, alike in dignity but differentiated by whether the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1403.7147","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"}