{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:25RDJHPKUYVIASV4HNKL5SJLWV","short_pith_number":"pith:25RDJHPK","schema_version":"1.0","canonical_sha256":"d762349deaa62a804abc3b54bec92bb556c1c61cafd9c27267640a275adc3ebf","source":{"kind":"arxiv","id":"1501.07856","version":1},"attestation_state":"computed","paper":{"title":"Busting Up Binaries: Encounters Between Compact Binaries and a Supermassive Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Eric Addison, Pablo Laguna, Shane Larson","submitted_at":"2015-01-26T12:10:46Z","abstract_excerpt":"Given the stellar density near the galactic center, close encounters between compact object binaries and the supermassive black hole are a plausible occurrence. We present results from a numerical study of close to 13 million such encounters. Consistent with previous studies, we corroborate that, for binary systems tidally disrupted by the black hole, the component of the binary remaining bound to the hole has eccentricity ~ 0.97 and circularizes dramatically by the time it enters the classical LISA band. Our results also show that the population of surviving binaries merits attention. These b"},"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":"1501.07856","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2015-01-26T12:10:46Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"44be89ea08eb8e9d4b12e957780bded10a079d57f478153dde91e0b836c0da93","abstract_canon_sha256":"509095a56b0274a2996f1f0e16466a756c35ba73cb7e16256e97429bde9b2ac5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:28:04.725954Z","signature_b64":"rkozIbY4ccmu7XlHese3DsmnmU4acbkc0WGO+2I2rC0GEx5DofGgfYHt1fiUdpID/j9gIkiaPwAup+oqTpSXDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d762349deaa62a804abc3b54bec92bb556c1c61cafd9c27267640a275adc3ebf","last_reissued_at":"2026-05-18T02:28:04.725554Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:28:04.725554Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Busting Up Binaries: Encounters Between Compact Binaries and a Supermassive Black Hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Eric Addison, Pablo Laguna, Shane Larson","submitted_at":"2015-01-26T12:10:46Z","abstract_excerpt":"Given the stellar density near the galactic center, close encounters between compact object binaries and the supermassive black hole are a plausible occurrence. We present results from a numerical study of close to 13 million such encounters. Consistent with previous studies, we corroborate that, for binary systems tidally disrupted by the black hole, the component of the binary remaining bound to the hole has eccentricity ~ 0.97 and circularizes dramatically by the time it enters the classical LISA band. Our results also show that the population of surviving binaries merits attention. These b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1501.07856","kind":"arxiv","version":1},"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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1501.07856","created_at":"2026-05-18T02:28:04.725618+00:00"},{"alias_kind":"arxiv_version","alias_value":"1501.07856v1","created_at":"2026-05-18T02:28:04.725618+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1501.07856","created_at":"2026-05-18T02:28:04.725618+00:00"},{"alias_kind":"pith_short_12","alias_value":"25RDJHPKUYVI","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_16","alias_value":"25RDJHPKUYVIASV4","created_at":"2026-05-18T12:28:59.999130+00:00"},{"alias_kind":"pith_short_8","alias_value":"25RDJHPK","created_at":"2026-05-18T12:28:59.999130+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.11375","citing_title":"The Missing Link in Gravitational-Wave Astronomy: Discoveries waiting in the decihertz range","ref_index":264,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV","json":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV.json","graph_json":"https://pith.science/api/pith-number/25RDJHPKUYVIASV4HNKL5SJLWV/graph.json","events_json":"https://pith.science/api/pith-number/25RDJHPKUYVIASV4HNKL5SJLWV/events.json","paper":"https://pith.science/paper/25RDJHPK"},"agent_actions":{"view_html":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV","download_json":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV.json","view_paper":"https://pith.science/paper/25RDJHPK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1501.07856&json=true","fetch_graph":"https://pith.science/api/pith-number/25RDJHPKUYVIASV4HNKL5SJLWV/graph.json","fetch_events":"https://pith.science/api/pith-number/25RDJHPKUYVIASV4HNKL5SJLWV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV/action/storage_attestation","attest_author":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV/action/author_attestation","sign_citation":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV/action/citation_signature","submit_replication":"https://pith.science/pith/25RDJHPKUYVIASV4HNKL5SJLWV/action/replication_record"}},"created_at":"2026-05-18T02:28:04.725618+00:00","updated_at":"2026-05-18T02:28:04.725618+00:00"}