{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:LSSSCGPHJO26K6NTCQA6GCNJJR","short_pith_number":"pith:LSSSCGPH","schema_version":"1.0","canonical_sha256":"5ca52119e74bb5e579b31401e309a94c4797d660b9b6a7c426f04a42d1d0849a","source":{"kind":"arxiv","id":"2101.11033","version":2},"attestation_state":"computed","paper":{"title":"Adding eccentricity to quasicircular binary-black-hole waveform models","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Frank Ohme, Yoshinta Setyawati","submitted_at":"2021-01-26T19:04:07Z","abstract_excerpt":"The detection of gravitational-wave signals from coalescing eccentric binary black holes would yield unprecedented information about the formation and evolution of compact binaries in specific scenarios, such as dynamical formation in dense stellar clusters and three-body interactions. The gravitational-wave searches by the ground-based interferometers, LIGO and Virgo, rely on analytical waveform models for binaries on quasicircular orbits. Eccentric merger waveform models are less developed, and only few numerical simulations of eccentric mergers are publicly available, but several eccentric "},"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":"2101.11033","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2021-01-26T19:04:07Z","cross_cats_sorted":[],"title_canon_sha256":"fc059c8ac43a3fd4897cf7539a42cc8b3d4adfbde4019daa3ab5677c80fbd269","abstract_canon_sha256":"0b6e33cc1bc543ba241823c73aec9ddfca332233ef2ab3e81a62d8b90b317607"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:47:30.699641Z","signature_b64":"XZX8Tcm7zdSFfqImrIP0oYjzf9QIr2S+4BgkwKO8dWuizZ1JGukEywKENXrvuZIsFF8ObLHLm8j6ksvmf83oDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5ca52119e74bb5e579b31401e309a94c4797d660b9b6a7c426f04a42d1d0849a","last_reissued_at":"2026-07-05T02:47:30.699162Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:47:30.699162Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Adding eccentricity to quasicircular binary-black-hole waveform models","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Frank Ohme, Yoshinta Setyawati","submitted_at":"2021-01-26T19:04:07Z","abstract_excerpt":"The detection of gravitational-wave signals from coalescing eccentric binary black holes would yield unprecedented information about the formation and evolution of compact binaries in specific scenarios, such as dynamical formation in dense stellar clusters and three-body interactions. The gravitational-wave searches by the ground-based interferometers, LIGO and Virgo, rely on analytical waveform models for binaries on quasicircular orbits. Eccentric merger waveform models are less developed, and only few numerical simulations of eccentric mergers are publicly available, but several eccentric "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2101.11033","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/2101.11033/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":"2101.11033","created_at":"2026-07-05T02:47:30.699222+00:00"},{"alias_kind":"arxiv_version","alias_value":"2101.11033v2","created_at":"2026-07-05T02:47:30.699222+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2101.11033","created_at":"2026-07-05T02:47:30.699222+00:00"},{"alias_kind":"pith_short_12","alias_value":"LSSSCGPHJO26","created_at":"2026-07-05T02:47:30.699222+00:00"},{"alias_kind":"pith_short_16","alias_value":"LSSSCGPHJO26K6NT","created_at":"2026-07-05T02:47:30.699222+00:00"},{"alias_kind":"pith_short_8","alias_value":"LSSSCGPH","created_at":"2026-07-05T02:47:30.699222+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.28715","citing_title":"Accurate waveforms for generic planar-orbit binary black holes: The multipolar effective-one-body model SEOBNRv6EHM","ref_index":190,"is_internal_anchor":false},{"citing_arxiv_id":"2404.14286","citing_title":"Evidence for eccentricity in the population of binary black holes observed by LIGO-Virgo-KAGRA","ref_index":170,"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":71,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR","json":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR.json","graph_json":"https://pith.science/api/pith-number/LSSSCGPHJO26K6NTCQA6GCNJJR/graph.json","events_json":"https://pith.science/api/pith-number/LSSSCGPHJO26K6NTCQA6GCNJJR/events.json","paper":"https://pith.science/paper/LSSSCGPH"},"agent_actions":{"view_html":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR","download_json":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR.json","view_paper":"https://pith.science/paper/LSSSCGPH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2101.11033&json=true","fetch_graph":"https://pith.science/api/pith-number/LSSSCGPHJO26K6NTCQA6GCNJJR/graph.json","fetch_events":"https://pith.science/api/pith-number/LSSSCGPHJO26K6NTCQA6GCNJJR/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR/action/timestamp_anchor","attest_storage":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR/action/storage_attestation","attest_author":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR/action/author_attestation","sign_citation":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR/action/citation_signature","submit_replication":"https://pith.science/pith/LSSSCGPHJO26K6NTCQA6GCNJJR/action/replication_record"}},"created_at":"2026-07-05T02:47:30.699222+00:00","updated_at":"2026-07-05T02:47:30.699222+00:00"}