{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:Z25ZEMQMCBWHL74G3LZ6QF7BNB","short_pith_number":"pith:Z25ZEMQM","schema_version":"1.0","canonical_sha256":"cebb92320c106c75ff86daf3e817e1687d5329e0279a2d2c38d24d27e6357456","source":{"kind":"arxiv","id":"gr-qc/0612060","version":2},"attestation_state":"computed","paper":{"title":"Gravitational waves from intermediate-mass-ratio inspirals for ground-based detectors","license":"","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Chao Li, Duncan A. Brown, Geoffrey Lovelace, Hua Fang, Ilya Mandel, Jeandrew Brink, Jonathan R. Gair, Kip S. Thorne","submitted_at":"2006-12-11T20:14:56Z","abstract_excerpt":"We explore the prospects for Advanced LIGO to detect gravitational waves from neutron stars and stellar mass black holes spiraling into intermediate-mass ($M\\sim 50 M_\\odot$ to $350 M_\\odot$) black holes. We estimate an event rate for such \\emph{intermediate-mass-ratio inspirals} (IMRIs) of up to $\\sim 10$--$30 \\mathrm{yr}^{-1}$. Our numerical simulations show that if the central body is not a black hole but its metric is stationary, axisymmetric, reflection symmetric and asymptotically flat then the waves will likely be tri-periodic, as for a black hole. We report generalizations of a theorem"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"gr-qc/0612060","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2006-12-11T20:14:56Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"178979c8838ee20763bff19c79f357d773464bd8b494aa6c58438e5253e32072","abstract_canon_sha256":"4d829908d3afd30e66a4b5925efbb3b420ec228ba78d19707ac9edb1faaf5ad3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:37:40.891397Z","signature_b64":"DtVBdg4xDFxiqCJPrFADCg4Kl9HORGzbCrhBYp1T3RMEaqn1eSIaHVJIQYAitY72wNhV1dkvBj3rqc2FS2FRBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cebb92320c106c75ff86daf3e817e1687d5329e0279a2d2c38d24d27e6357456","last_reissued_at":"2026-07-04T16:37:40.890984Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:37:40.890984Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational waves from intermediate-mass-ratio inspirals for ground-based detectors","license":"","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Chao Li, Duncan A. Brown, Geoffrey Lovelace, Hua Fang, Ilya Mandel, Jeandrew Brink, Jonathan R. Gair, Kip S. Thorne","submitted_at":"2006-12-11T20:14:56Z","abstract_excerpt":"We explore the prospects for Advanced LIGO to detect gravitational waves from neutron stars and stellar mass black holes spiraling into intermediate-mass ($M\\sim 50 M_\\odot$ to $350 M_\\odot$) black holes. We estimate an event rate for such \\emph{intermediate-mass-ratio inspirals} (IMRIs) of up to $\\sim 10$--$30 \\mathrm{yr}^{-1}$. Our numerical simulations show that if the central body is not a black hole but its metric is stationary, axisymmetric, reflection symmetric and asymptotically flat then the waves will likely be tri-periodic, as for a black hole. We report generalizations of a theorem"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0612060","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/gr-qc/0612060/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"gr-qc/0612060","created_at":"2026-07-04T16:37:40.891044+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0612060v2","created_at":"2026-07-04T16:37:40.891044+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0612060","created_at":"2026-07-04T16:37:40.891044+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z25ZEMQMCBWH","created_at":"2026-07-04T16:37:40.891044+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z25ZEMQMCBWHL74G","created_at":"2026-07-04T16:37:40.891044+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z25ZEMQM","created_at":"2026-07-04T16:37:40.891044+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.22210","citing_title":"Constraints on Schwarzschild Black Hole in a Generalized Dehnen-Type $(1,4,\\gamma)$ Dark Matter Halo via the S2 Star Orbit around Sgr A$^\\star$","ref_index":26,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB","json":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB.json","graph_json":"https://pith.science/api/pith-number/Z25ZEMQMCBWHL74G3LZ6QF7BNB/graph.json","events_json":"https://pith.science/api/pith-number/Z25ZEMQMCBWHL74G3LZ6QF7BNB/events.json","paper":"https://pith.science/paper/Z25ZEMQM"},"agent_actions":{"view_html":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB","download_json":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB.json","view_paper":"https://pith.science/paper/Z25ZEMQM","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0612060&json=true","fetch_graph":"https://pith.science/api/pith-number/Z25ZEMQMCBWHL74G3LZ6QF7BNB/graph.json","fetch_events":"https://pith.science/api/pith-number/Z25ZEMQMCBWHL74G3LZ6QF7BNB/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB/action/storage_attestation","attest_author":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB/action/author_attestation","sign_citation":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB/action/citation_signature","submit_replication":"https://pith.science/pith/Z25ZEMQMCBWHL74G3LZ6QF7BNB/action/replication_record"}},"created_at":"2026-07-04T16:37:40.891044+00:00","updated_at":"2026-07-04T16:37:40.891044+00:00"}