{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:NGLWIW2AT7VG2PYWPHBP5BJ7SR","short_pith_number":"pith:NGLWIW2A","schema_version":"1.0","canonical_sha256":"6997645b409fea6d3f1679c2fe853f9451631f80b111b1a088fdd1e74657d5c4","source":{"kind":"arxiv","id":"1811.04926","version":2},"attestation_state":"computed","paper":{"title":"Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carl L. Rodriguez, Claire S. Ye, Frederic A. Rasio, Johan Samsing, Kyle Kremer, Michael Zevin, Pau Amaro-Seoane, Sourav Chatterjee","submitted_at":"2018-11-12T19:00:00Z","abstract_excerpt":"Using state-of-the-art dynamical simulations of globular clusters, including radiation reaction during black hole encounters and a cosmological model of star cluster formation, we create a realistic population of dynamically-formed binary black hole mergers across cosmic space and time. We show that in the local universe, 10% of these binaries form as the result of gravitational-wave emission between unbound black holes during chaotic resonant encounters, with roughly half of those events having eccentricities detectable by current ground-based gravitational-wave detectors. The mergers that oc"},"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":"1811.04926","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-11-12T19:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"9d697e824397cf54b812296476546a61f2e3f495f6f8b1dbceb83981f4bff3df","abstract_canon_sha256":"de9846df38efc96dbfca2a0152e66cdf6b55fc1be6433bc86b3e62dfbf343c6a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:57:37.483138Z","signature_b64":"0DD4Qx7j+7iHdETYYVsb3H1r/hLE6lt7wEMypyKN4+Yor2aCxTrspX96vSB7/Zquv87wq52/bCTZ5XfpJFvkBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6997645b409fea6d3f1679c2fe853f9451631f80b111b1a088fdd1e74657d5c4","last_reissued_at":"2026-05-17T23:57:37.482751Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:57:37.482751Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Post-Newtonian Dynamics in Dense Star Clusters: Formation, Masses, and Merger Rates of Highly-Eccentric Black Hole Binaries","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"Carl L. Rodriguez, Claire S. Ye, Frederic A. Rasio, Johan Samsing, Kyle Kremer, Michael Zevin, Pau Amaro-Seoane, Sourav Chatterjee","submitted_at":"2018-11-12T19:00:00Z","abstract_excerpt":"Using state-of-the-art dynamical simulations of globular clusters, including radiation reaction during black hole encounters and a cosmological model of star cluster formation, we create a realistic population of dynamically-formed binary black hole mergers across cosmic space and time. We show that in the local universe, 10% of these binaries form as the result of gravitational-wave emission between unbound black holes during chaotic resonant encounters, with roughly half of those events having eccentricities detectable by current ground-based gravitational-wave detectors. The mergers that oc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1811.04926","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":"1811.04926","created_at":"2026-05-17T23:57:37.482809+00:00"},{"alias_kind":"arxiv_version","alias_value":"1811.04926v2","created_at":"2026-05-17T23:57:37.482809+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1811.04926","created_at":"2026-05-17T23:57:37.482809+00:00"},{"alias_kind":"pith_short_12","alias_value":"NGLWIW2AT7VG","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_16","alias_value":"NGLWIW2AT7VG2PYW","created_at":"2026-05-18T12:32:40.477152+00:00"},{"alias_kind":"pith_short_8","alias_value":"NGLWIW2A","created_at":"2026-05-18T12:32:40.477152+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":9,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"1907.02283","citing_title":"Eccentricity Without Measuring Eccentricity: Discriminating Among Stellar Mass Black Hole Binary Formation Channels","ref_index":8,"is_internal_anchor":true},{"citing_arxiv_id":"2404.14286","citing_title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","ref_index":87,"is_internal_anchor":true},{"citing_arxiv_id":"2605.18742","citing_title":"A universal framework to identify eccentric binary mergers: GW200105 case study","ref_index":10,"is_internal_anchor":true},{"citing_arxiv_id":"2601.18835","citing_title":"Beyond FINDCHIRP: Breaking the memory wall and optimal FFTs for Gravitational-Wave Matched-Filter Searches with Ratio-Filter Dechirping","ref_index":31,"is_internal_anchor":true},{"citing_arxiv_id":"1903.04467","citing_title":"Tests of General Relativity with the Binary Black Hole Signals from the LIGO-Virgo Catalog GWTC-1","ref_index":67,"is_internal_anchor":true},{"citing_arxiv_id":"2604.04546","citing_title":"Inference of recoil kicks from binary black hole mergers up to GWTC--4 and their astrophysical implications","ref_index":93,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11903","citing_title":"Post-Newtonian inspiral waveform model for eccentric precessing binaries with higher-order modes and matter effects","ref_index":154,"is_internal_anchor":false},{"citing_arxiv_id":"2604.17868","citing_title":"Including higher-order modes in a quadrupolar eccentric numerical relativity surrogate using universal eccentric modulation functions","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15431","citing_title":"Highly eccentric non-spinning binary black hole mergers: quadrupolar post-merger waveforms","ref_index":49,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR","json":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR.json","graph_json":"https://pith.science/api/pith-number/NGLWIW2AT7VG2PYWPHBP5BJ7SR/graph.json","events_json":"https://pith.science/api/pith-number/NGLWIW2AT7VG2PYWPHBP5BJ7SR/events.json","paper":"https://pith.science/paper/NGLWIW2A"},"agent_actions":{"view_html":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR","download_json":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR.json","view_paper":"https://pith.science/paper/NGLWIW2A","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1811.04926&json=true","fetch_graph":"https://pith.science/api/pith-number/NGLWIW2AT7VG2PYWPHBP5BJ7SR/graph.json","fetch_events":"https://pith.science/api/pith-number/NGLWIW2AT7VG2PYWPHBP5BJ7SR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR/action/storage_attestation","attest_author":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR/action/author_attestation","sign_citation":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR/action/citation_signature","submit_replication":"https://pith.science/pith/NGLWIW2AT7VG2PYWPHBP5BJ7SR/action/replication_record"}},"created_at":"2026-05-17T23:57:37.482809+00:00","updated_at":"2026-05-17T23:57:37.482809+00:00"}