{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:JEO5L555GV4NED4JVJS4EJIT5J","short_pith_number":"pith:JEO5L555","schema_version":"1.0","canonical_sha256":"491dd5f7bd3578d20f89aa65c22513ea52437b0255b4a794b0220a92fb0429d1","source":{"kind":"arxiv","id":"1906.06263","version":2},"attestation_state":"computed","paper":{"title":"Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bala R. Iyer, Chandra K. Mishra, Guillaume Faye, Michael Ebersold, Philippe Jetzer, Yannick Boetzel","submitted_at":"2019-06-14T16:00:46Z","abstract_excerpt":"We compute the non-linear memory contributions to the gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian (3PN) order in general relativity. These contributions are hereditary in nature as they are sourced by gravitational waves emitted during the binary's entire dynamical past. Combining these with already available instantaneous and tail contributions we get the complete 3PN accurate gravitational waveform."},"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":"1906.06263","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-06-14T16:00:46Z","cross_cats_sorted":[],"title_canon_sha256":"94bf55d2552af66275db16edb45306b69a15b2692d00693fd8d0daf02ee27043","abstract_canon_sha256":"44daba771ae6a7cdf32d00956f9af9c07c49f2705e0bc78d27b20a95d9558e60"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:13:29.900874Z","signature_b64":"ndAIkCpdxcM0h+K+l3k7VfgWGTX/YsSvA6RknFe1gO/IcAIcXWUGoK6h/sSCu+irWx1VSPLjvRr6KZ3i6Y9HDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"491dd5f7bd3578d20f89aa65c22513ea52437b0255b4a794b0220a92fb0429d1","last_reissued_at":"2026-07-05T00:13:29.900452Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:13:29.900452Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian order: Memory contributions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Bala R. Iyer, Chandra K. Mishra, Guillaume Faye, Michael Ebersold, Philippe Jetzer, Yannick Boetzel","submitted_at":"2019-06-14T16:00:46Z","abstract_excerpt":"We compute the non-linear memory contributions to the gravitational-wave amplitudes for compact binaries in eccentric orbits at the third post-Newtonian (3PN) order in general relativity. These contributions are hereditary in nature as they are sourced by gravitational waves emitted during the binary's entire dynamical past. Combining these with already available instantaneous and tail contributions we get the complete 3PN accurate gravitational waveform."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1906.06263","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/1906.06263/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":"1906.06263","created_at":"2026-07-05T00:13:29.900509+00:00"},{"alias_kind":"arxiv_version","alias_value":"1906.06263v2","created_at":"2026-07-05T00:13:29.900509+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1906.06263","created_at":"2026-07-05T00:13:29.900509+00:00"},{"alias_kind":"pith_short_12","alias_value":"JEO5L555GV4N","created_at":"2026-07-05T00:13:29.900509+00:00"},{"alias_kind":"pith_short_16","alias_value":"JEO5L555GV4NED4J","created_at":"2026-07-05T00:13:29.900509+00:00"},{"alias_kind":"pith_short_8","alias_value":"JEO5L555","created_at":"2026-07-05T00:13:29.900509+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30594","citing_title":"Efficient Eccentric Effective-One-Body Dynamics via Near-Identity Averaging Transformations","ref_index":137,"is_internal_anchor":false},{"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":160,"is_internal_anchor":false},{"citing_arxiv_id":"2510.04332","citing_title":"Biased parameter inference of eccentric, spin-precessing binary black holes","ref_index":103,"is_internal_anchor":false},{"citing_arxiv_id":"2511.10735","citing_title":"Constants of motion and fundamental frequencies for elliptic orbits at fourth post-Newtonian order","ref_index":96,"is_internal_anchor":false},{"citing_arxiv_id":"2601.23019","citing_title":"Toward claiming a detection of gravitational memory","ref_index":202,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J","json":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J.json","graph_json":"https://pith.science/api/pith-number/JEO5L555GV4NED4JVJS4EJIT5J/graph.json","events_json":"https://pith.science/api/pith-number/JEO5L555GV4NED4JVJS4EJIT5J/events.json","paper":"https://pith.science/paper/JEO5L555"},"agent_actions":{"view_html":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J","download_json":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J.json","view_paper":"https://pith.science/paper/JEO5L555","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1906.06263&json=true","fetch_graph":"https://pith.science/api/pith-number/JEO5L555GV4NED4JVJS4EJIT5J/graph.json","fetch_events":"https://pith.science/api/pith-number/JEO5L555GV4NED4JVJS4EJIT5J/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J/action/storage_attestation","attest_author":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J/action/author_attestation","sign_citation":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J/action/citation_signature","submit_replication":"https://pith.science/pith/JEO5L555GV4NED4JVJS4EJIT5J/action/replication_record"}},"created_at":"2026-07-05T00:13:29.900509+00:00","updated_at":"2026-07-05T00:13:29.900509+00:00"}