{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:G6APJRZ63D2OMYHFKDKXJYMHMH","short_pith_number":"pith:G6APJRZ6","schema_version":"1.0","canonical_sha256":"3780f4c73ed8f4e660e550d574e18761c29d4e0172e4bccc32483cb3a887cf6f","source":{"kind":"arxiv","id":"1711.09989","version":2},"attestation_state":"computed","paper":{"title":"Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Bence Kocsis, L\\'aszl\\'o Gond\\'an, P\\'eter Raffai, Zsolt Frei","submitted_at":"2017-11-27T20:53:04Z","abstract_excerpt":"Mergers of binary black holes on eccentric orbits are among the targets for second-generation ground-based gravitational-wave detectors. These sources may commonly form in galactic nuclei due to gravitational-wave emission during close flyby events of single objects. We determine the distributions of initial orbital parameters for a population of these gravitational-wave sources. Our results show that the initial dimensionless pericenter distance systematically decreases with the binary component masses and the mass of the central supermassive black hole, and its distribution depends sensitive"},"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":"1711.09989","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-11-27T20:53:04Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"391b646ad318b3ec41123accf3e835338aebdcda65e55c4014592dc1302a2588","abstract_canon_sha256":"ed28c5161aadfadc76d992519c39da2b4179ade353aa5f9fb7bce9acc0378f40"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:01:38.831805Z","signature_b64":"VhwrX3yYcGK++bwBUyc5Z6NBGnh1gB2M2OvdFqMOC1st4xe5uzQMgdg50Mk1uKh0pc9OfR92K1UQoqcPyTe6Cg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3780f4c73ed8f4e660e550d574e18761c29d4e0172e4bccc32483cb3a887cf6f","last_reissued_at":"2026-05-18T00:01:38.831305Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:01:38.831305Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Eccentric Black Hole Gravitational-Wave Capture Sources in Galactic Nuclei: Distribution of Binary Parameters","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Bence Kocsis, L\\'aszl\\'o Gond\\'an, P\\'eter Raffai, Zsolt Frei","submitted_at":"2017-11-27T20:53:04Z","abstract_excerpt":"Mergers of binary black holes on eccentric orbits are among the targets for second-generation ground-based gravitational-wave detectors. These sources may commonly form in galactic nuclei due to gravitational-wave emission during close flyby events of single objects. We determine the distributions of initial orbital parameters for a population of these gravitational-wave sources. Our results show that the initial dimensionless pericenter distance systematically decreases with the binary component masses and the mass of the central supermassive black hole, and its distribution depends sensitive"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1711.09989","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"},"aliases":[{"alias_kind":"arxiv","alias_value":"1711.09989","created_at":"2026-05-18T00:01:38.831406+00:00"},{"alias_kind":"arxiv_version","alias_value":"1711.09989v2","created_at":"2026-05-18T00:01:38.831406+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1711.09989","created_at":"2026-05-18T00:01:38.831406+00:00"},{"alias_kind":"pith_short_12","alias_value":"G6APJRZ63D2O","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_16","alias_value":"G6APJRZ63D2OMYHF","created_at":"2026-05-18T12:31:15.632608+00:00"},{"alias_kind":"pith_short_8","alias_value":"G6APJRZ6","created_at":"2026-05-18T12:31:15.632608+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2404.14286","citing_title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","ref_index":77,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH","json":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH.json","graph_json":"https://pith.science/api/pith-number/G6APJRZ63D2OMYHFKDKXJYMHMH/graph.json","events_json":"https://pith.science/api/pith-number/G6APJRZ63D2OMYHFKDKXJYMHMH/events.json","paper":"https://pith.science/paper/G6APJRZ6"},"agent_actions":{"view_html":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH","download_json":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH.json","view_paper":"https://pith.science/paper/G6APJRZ6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1711.09989&json=true","fetch_graph":"https://pith.science/api/pith-number/G6APJRZ63D2OMYHFKDKXJYMHMH/graph.json","fetch_events":"https://pith.science/api/pith-number/G6APJRZ63D2OMYHFKDKXJYMHMH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH/action/storage_attestation","attest_author":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH/action/author_attestation","sign_citation":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH/action/citation_signature","submit_replication":"https://pith.science/pith/G6APJRZ63D2OMYHFKDKXJYMHMH/action/replication_record"}},"created_at":"2026-05-18T00:01:38.831406+00:00","updated_at":"2026-05-18T00:01:38.831406+00:00"}