{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:CLEA3FLHEE4VE7U24FOBBRWCWU","short_pith_number":"pith:CLEA3FLH","schema_version":"1.0","canonical_sha256":"12c80d95672139527e9ae15c10c6c2b533c619a1bdd12b2a3946027ec0d48542","source":{"kind":"arxiv","id":"2111.13639","version":4},"attestation_state":"computed","paper":{"title":"The 2PM Hamiltonian for binary Kerr to quartic in spin","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jung-Wook Kim, Ming-Zhi Chung, Wei-Ming Chen, Yu-tin Huang","submitted_at":"2021-11-26T18:07:30Z","abstract_excerpt":"From the S-matrix of spinning particles, we extract the 2 PM conservative potential for binary spinning black holes up to quartic order in spin operators. An important ingredient is the exponentiated gravitational Compton amplitude in the classical spin-limit for all graviton helicity sectors. The validity of the resulting Hamiltonian is verified by matching to known lower spin order results, as well as direct computation of the 2PM impulse and spin kicks from the eikonal phase and that from the test black hole scattering based on Mathisson-Papapetrou-Dixon equations."},"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":"2111.13639","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2021-11-26T18:07:30Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"d14923a2fdb87e38ce629ccc32ccc708c132bd3eba281173c996e038e6d87dce","abstract_canon_sha256":"e96e92eaa6554865002741f00f574f1cd3e8240f690288513e4fbd49b7ee6255"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:44:39.423476Z","signature_b64":"ZrTr62usJCQLUWju1FJ6lm6v7bm9I11m/V64BSvg43rMsc2CYFMMUjMGEiFhkxBT/vlaL6/uAc/oR+cHMnEsDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"12c80d95672139527e9ae15c10c6c2b533c619a1bdd12b2a3946027ec0d48542","last_reissued_at":"2026-07-05T07:44:39.423044Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:44:39.423044Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The 2PM Hamiltonian for binary Kerr to quartic in spin","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jung-Wook Kim, Ming-Zhi Chung, Wei-Ming Chen, Yu-tin Huang","submitted_at":"2021-11-26T18:07:30Z","abstract_excerpt":"From the S-matrix of spinning particles, we extract the 2 PM conservative potential for binary spinning black holes up to quartic order in spin operators. An important ingredient is the exponentiated gravitational Compton amplitude in the classical spin-limit for all graviton helicity sectors. The validity of the resulting Hamiltonian is verified by matching to known lower spin order results, as well as direct computation of the 2PM impulse and spin kicks from the eikonal phase and that from the test black hole scattering based on Mathisson-Papapetrou-Dixon equations."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2111.13639","kind":"arxiv","version":4},"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/2111.13639/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":"2111.13639","created_at":"2026-07-05T07:44:39.423103+00:00"},{"alias_kind":"arxiv_version","alias_value":"2111.13639v4","created_at":"2026-07-05T07:44:39.423103+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2111.13639","created_at":"2026-07-05T07:44:39.423103+00:00"},{"alias_kind":"pith_short_12","alias_value":"CLEA3FLHEE4V","created_at":"2026-07-05T07:44:39.423103+00:00"},{"alias_kind":"pith_short_16","alias_value":"CLEA3FLHEE4VE7U2","created_at":"2026-07-05T07:44:39.423103+00:00"},{"alias_kind":"pith_short_8","alias_value":"CLEA3FLH","created_at":"2026-07-05T07:44:39.423103+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.23450","citing_title":"NLO Angular Impulse and Leading Singularities to all orders in spin for Kerr Black Holes","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2508.10761","citing_title":"Unexpected Symmetries of Kerr Black Hole Scattering","ref_index":51,"is_internal_anchor":false},{"citing_arxiv_id":"2509.04425","citing_title":"Hidden simplicity in the scattering for neutron stars and black holes","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2602.06947","citing_title":"The gravitational Compton amplitude at third post-Minkowskian order","ref_index":88,"is_internal_anchor":false},{"citing_arxiv_id":"2602.18790","citing_title":"Generalized Carter & R\\\"udiger Constants of $\\sqrt{\\text{Kerr}}$","ref_index":83,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05067","citing_title":"Gravitational multipoles from scattering amplitudes in higher dimensions","ref_index":25,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU","json":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU.json","graph_json":"https://pith.science/api/pith-number/CLEA3FLHEE4VE7U24FOBBRWCWU/graph.json","events_json":"https://pith.science/api/pith-number/CLEA3FLHEE4VE7U24FOBBRWCWU/events.json","paper":"https://pith.science/paper/CLEA3FLH"},"agent_actions":{"view_html":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU","download_json":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU.json","view_paper":"https://pith.science/paper/CLEA3FLH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2111.13639&json=true","fetch_graph":"https://pith.science/api/pith-number/CLEA3FLHEE4VE7U24FOBBRWCWU/graph.json","fetch_events":"https://pith.science/api/pith-number/CLEA3FLHEE4VE7U24FOBBRWCWU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU/action/storage_attestation","attest_author":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU/action/author_attestation","sign_citation":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU/action/citation_signature","submit_replication":"https://pith.science/pith/CLEA3FLHEE4VE7U24FOBBRWCWU/action/replication_record"}},"created_at":"2026-07-05T07:44:39.423103+00:00","updated_at":"2026-07-05T07:44:39.423103+00:00"}