{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:YSDKW3PLS63O63D7PLHPGOPTK2","short_pith_number":"pith:YSDKW3PL","schema_version":"1.0","canonical_sha256":"c486ab6deb97b6ef6c7f7acef339f356b295a88fb93991768071b368f2bf6feb","source":{"kind":"arxiv","id":"2406.17658","version":2},"attestation_state":"computed","paper":{"title":"Systematic integral evaluation for spin-resummed binary dynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Gang Chen, Jung-Wook Kim, Tianheng Wang","submitted_at":"2024-06-25T15:49:28Z","abstract_excerpt":"Computation of spin-resummed observables in post-Minkowskian dynamics typically involve evaluation of Feynman integrals deformed by an exponential factor, where the exponent is a linear sum of the momenta being integrated. Such integrals can be viewed as tensor integral generating functions, which provide alternative approaches to tensor reduction of Feynman integrals. We develop a systematic method to evaluate tensor integral generating functions using conventional multiloop integration techniques. The spin-resummed aligned-spin eikonal at second post-Minkowskian order is considered as a phen"},"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":"2406.17658","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-06-25T15:49:28Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"66a6267778fd5c49d7fe3078378404f374d106a2bb9eba8d9913217099a3df37","abstract_canon_sha256":"ca99acb98373fa7f361e8f24b39f5fdeb4edb25c02fa7d88dc60f53bb33694c6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:45:09.478338Z","signature_b64":"h//KX8AiFR4/wZhIUjDj11WqHXOO84W2/Yu+h5xAfJEeWQWVAMk3vVF6BW13uaiT40ODCA1bhkIZFaVNvc9tAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c486ab6deb97b6ef6c7f7acef339f356b295a88fb93991768071b368f2bf6feb","last_reissued_at":"2026-07-05T10:45:09.477713Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:45:09.477713Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Systematic integral evaluation for spin-resummed binary dynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Gang Chen, Jung-Wook Kim, Tianheng Wang","submitted_at":"2024-06-25T15:49:28Z","abstract_excerpt":"Computation of spin-resummed observables in post-Minkowskian dynamics typically involve evaluation of Feynman integrals deformed by an exponential factor, where the exponent is a linear sum of the momenta being integrated. Such integrals can be viewed as tensor integral generating functions, which provide alternative approaches to tensor reduction of Feynman integrals. We develop a systematic method to evaluate tensor integral generating functions using conventional multiloop integration techniques. The spin-resummed aligned-spin eikonal at second post-Minkowskian order is considered as a phen"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2406.17658","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/2406.17658/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":"2406.17658","created_at":"2026-07-05T10:45:09.477802+00:00"},{"alias_kind":"arxiv_version","alias_value":"2406.17658v2","created_at":"2026-07-05T10:45:09.477802+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2406.17658","created_at":"2026-07-05T10:45:09.477802+00:00"},{"alias_kind":"pith_short_12","alias_value":"YSDKW3PLS63O","created_at":"2026-07-05T10:45:09.477802+00:00"},{"alias_kind":"pith_short_16","alias_value":"YSDKW3PLS63O63D7","created_at":"2026-07-05T10:45:09.477802+00:00"},{"alias_kind":"pith_short_8","alias_value":"YSDKW3PL","created_at":"2026-07-05T10:45:09.477802+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2509.04425","citing_title":"Hidden simplicity in the scattering for neutron stars and black holes","ref_index":95,"is_internal_anchor":false},{"citing_arxiv_id":"2512.21210","citing_title":"Twisted Feynman Integrals: from generating functions to spin-resummed post-Minkowskian dynamics","ref_index":13,"is_internal_anchor":false},{"citing_arxiv_id":"2602.06947","citing_title":"The gravitational Compton amplitude at third post-Minkowskian order","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2","json":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2.json","graph_json":"https://pith.science/api/pith-number/YSDKW3PLS63O63D7PLHPGOPTK2/graph.json","events_json":"https://pith.science/api/pith-number/YSDKW3PLS63O63D7PLHPGOPTK2/events.json","paper":"https://pith.science/paper/YSDKW3PL"},"agent_actions":{"view_html":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2","download_json":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2.json","view_paper":"https://pith.science/paper/YSDKW3PL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2406.17658&json=true","fetch_graph":"https://pith.science/api/pith-number/YSDKW3PLS63O63D7PLHPGOPTK2/graph.json","fetch_events":"https://pith.science/api/pith-number/YSDKW3PLS63O63D7PLHPGOPTK2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2/action/storage_attestation","attest_author":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2/action/author_attestation","sign_citation":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2/action/citation_signature","submit_replication":"https://pith.science/pith/YSDKW3PLS63O63D7PLHPGOPTK2/action/replication_record"}},"created_at":"2026-07-05T10:45:09.477802+00:00","updated_at":"2026-07-05T10:45:09.477802+00:00"}