{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:Q7Z5WHDTCMUF5QYYHEFBRUHWAC","short_pith_number":"pith:Q7Z5WHDT","schema_version":"1.0","canonical_sha256":"87f3db1c7313285ec318390a18d0f600b51abcfd4119f390827979a457d359b7","source":{"kind":"arxiv","id":"2005.04236","version":3},"attestation_state":"computed","paper":{"title":"Extremal black hole scattering at O(G^3): graviton dominance, eikonal exponentiation, and differential equations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Julio Parra-Martinez, Mao Zeng, Michael S. Ruf","submitted_at":"2020-05-08T18:00:00Z","abstract_excerpt":"We use $\\mathcal N=8$ supergravity as a toy model for understanding the dynamics of black hole binary systems via the scattering amplitudes approach. We compute the conservative part of the classical scattering angle of two extremal (half-BPS) black holes with minimal charge misalignment at $\\mathcal O(G^3)$ using the eikonal approximation and effective field theory, finding agreement between both methods. We construct the massive loop integrands by Kaluza-Klein reduction of the known $D$-dimensional massless integrands. To carry out integration we formulate a novel method for calculating the "},"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":"2005.04236","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2020-05-08T18:00:00Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"c086ccac7b7bf49ccf53d849fa30f7a25271b6fe0faabe7cdf9f424a0f4d039e","abstract_canon_sha256":"a1ba3a6392ba0562a45540a880b243b0b2ca65aa5284a945d0a32caa86c92036"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T02:06:08.407224Z","signature_b64":"AzBPSXJJTqUClFJy1PZlR7Lg/0pvca5LIQYzRONdeohxkqzMgHBITUyy5TO9MWEDUHRTD4JjRmDh+nweK637BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"87f3db1c7313285ec318390a18d0f600b51abcfd4119f390827979a457d359b7","last_reissued_at":"2026-07-05T02:06:08.406798Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T02:06:08.406798Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Extremal black hole scattering at O(G^3): graviton dominance, eikonal exponentiation, and differential equations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Julio Parra-Martinez, Mao Zeng, Michael S. Ruf","submitted_at":"2020-05-08T18:00:00Z","abstract_excerpt":"We use $\\mathcal N=8$ supergravity as a toy model for understanding the dynamics of black hole binary systems via the scattering amplitudes approach. We compute the conservative part of the classical scattering angle of two extremal (half-BPS) black holes with minimal charge misalignment at $\\mathcal O(G^3)$ using the eikonal approximation and effective field theory, finding agreement between both methods. We construct the massive loop integrands by Kaluza-Klein reduction of the known $D$-dimensional massless integrands. To carry out integration we formulate a novel method for calculating the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2005.04236","kind":"arxiv","version":3},"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/2005.04236/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":"2005.04236","created_at":"2026-07-05T02:06:08.406856+00:00"},{"alias_kind":"arxiv_version","alias_value":"2005.04236v3","created_at":"2026-07-05T02:06:08.406856+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2005.04236","created_at":"2026-07-05T02:06:08.406856+00:00"},{"alias_kind":"pith_short_12","alias_value":"Q7Z5WHDTCMUF","created_at":"2026-07-05T02:06:08.406856+00:00"},{"alias_kind":"pith_short_16","alias_value":"Q7Z5WHDTCMUF5QYY","created_at":"2026-07-05T02:06:08.406856+00:00"},{"alias_kind":"pith_short_8","alias_value":"Q7Z5WHDT","created_at":"2026-07-05T02:06:08.406856+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"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":24,"is_internal_anchor":false},{"citing_arxiv_id":"2606.11423","citing_title":"Weak-field waveforms for generic relativistic orbits","ref_index":53,"is_internal_anchor":false},{"citing_arxiv_id":"2606.28239","citing_title":"Gravitational Compton scattering at the fourth post-Minkowskian order","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2511.11457","citing_title":"Analytic structure of the high-energy gravitational amplitude: multi-H diagrams and classical 5PM logarithms","ref_index":61,"is_internal_anchor":false},{"citing_arxiv_id":"2510.07390","citing_title":"Heterotic Footprints in Classical Gravity: PM dynamics from On-Shell soft amplitudes at one loop","ref_index":139,"is_internal_anchor":false},{"citing_arxiv_id":"2602.06947","citing_title":"The gravitational Compton amplitude at third post-Minkowskian order","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18004","citing_title":"Eikonal, nonlocality and regular black holes","ref_index":9,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC","json":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC.json","graph_json":"https://pith.science/api/pith-number/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/graph.json","events_json":"https://pith.science/api/pith-number/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/events.json","paper":"https://pith.science/paper/Q7Z5WHDT"},"agent_actions":{"view_html":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC","download_json":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC.json","view_paper":"https://pith.science/paper/Q7Z5WHDT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2005.04236&json=true","fetch_graph":"https://pith.science/api/pith-number/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/graph.json","fetch_events":"https://pith.science/api/pith-number/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/action/storage_attestation","attest_author":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/action/author_attestation","sign_citation":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/action/citation_signature","submit_replication":"https://pith.science/pith/Q7Z5WHDTCMUF5QYYHEFBRUHWAC/action/replication_record"}},"created_at":"2026-07-05T02:06:08.406856+00:00","updated_at":"2026-07-05T02:06:08.406856+00:00"}