{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:HNUIKTZ5LMDB2FNC5HAQHL554Y","short_pith_number":"pith:HNUIKTZ5","schema_version":"1.0","canonical_sha256":"3b68854f3d5b061d15a2e9c103afbde61f566d2cccb165b925fc2db5e39bb2ec","source":{"kind":"arxiv","id":"2411.11846","version":2},"attestation_state":"computed","paper":{"title":"Emergence of Calabi-Yau manifolds in high-precision black hole scattering","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","math.AG"],"primary_cat":"hep-th","authors_text":"Albrecht Klemm, Benjamin Sauer, Christoph Nega, Gustav Mogull, Gustav Uhre Jakobsen, Jan Plefka, Johann Usovitsch, Mathias Driesse","submitted_at":"2024-11-18T18:59:58Z","abstract_excerpt":"Using the worldline quantum field theory formalism, we compute the radiation-reacted impulse, scattering angle, radiated energy and recoil of a classical black hole (or neutron star) scattering event at fifth post-Minkowskian and sub-leading self-force orders (5PM-1SF). This state-of-the-art four-loop computation employs advanced integration-by-parts and differential equation technology, and is considerably more challenging than the conservative 5PM-1SF counterpart. As compared with the conservative 5PM-1SF, in the radiation sector Calabi-Yau three-fold periods appear and contribute to the rad"},"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":"2411.11846","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-11-18T18:59:58Z","cross_cats_sorted":["gr-qc","hep-ph","math.AG"],"title_canon_sha256":"c2b2dbc5204378ed1469bd86b83dad4076d5fca6619c961b875646919a18de26","abstract_canon_sha256":"8055d5a12036557a9c0457d1f8ed7309c3c72abed59bf8060d9c0ed8107262ef"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-21T18:25:30.066238Z","signature_b64":"kUll1DKlMaePLpmUp0vS9KbrFbJXcyN0yldQRQ9T0E7RshRWOum2d9RBugcFTFNlONhXUIi1/aZPQTabAP3jDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3b68854f3d5b061d15a2e9c103afbde61f566d2cccb165b925fc2db5e39bb2ec","last_reissued_at":"2026-05-21T18:25:30.063802Z","signature_status":"signed_v1","first_computed_at":"2026-05-21T18:25:30.063802Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Emergence of Calabi-Yau manifolds in high-precision black hole scattering","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph","math.AG"],"primary_cat":"hep-th","authors_text":"Albrecht Klemm, Benjamin Sauer, Christoph Nega, Gustav Mogull, Gustav Uhre Jakobsen, Jan Plefka, Johann Usovitsch, Mathias Driesse","submitted_at":"2024-11-18T18:59:58Z","abstract_excerpt":"Using the worldline quantum field theory formalism, we compute the radiation-reacted impulse, scattering angle, radiated energy and recoil of a classical black hole (or neutron star) scattering event at fifth post-Minkowskian and sub-leading self-force orders (5PM-1SF). This state-of-the-art four-loop computation employs advanced integration-by-parts and differential equation technology, and is considerably more challenging than the conservative 5PM-1SF counterpart. As compared with the conservative 5PM-1SF, in the radiation sector Calabi-Yau three-fold periods appear and contribute to the rad"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.11846","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/2411.11846/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":"2411.11846","created_at":"2026-05-21T18:25:30.063906+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.11846v2","created_at":"2026-05-21T18:25:30.063906+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.11846","created_at":"2026-05-21T18:25:30.063906+00:00"},{"alias_kind":"pith_short_12","alias_value":"HNUIKTZ5LMDB","created_at":"2026-05-21T18:25:30.063906+00:00"},{"alias_kind":"pith_short_16","alias_value":"HNUIKTZ5LMDB2FNC","created_at":"2026-05-21T18:25:30.063906+00:00"},{"alias_kind":"pith_short_8","alias_value":"HNUIKTZ5","created_at":"2026-05-21T18:25:30.063906+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":22,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.22037","citing_title":"Classical Renormalization Group Equations for General Relativity","ref_index":19,"is_internal_anchor":true},{"citing_arxiv_id":"2511.15240","citing_title":"A construction of single-valued elliptic polylogarithms","ref_index":12,"is_internal_anchor":true},{"citing_arxiv_id":"2511.11457","citing_title":"Analytic structure of the high-energy gravitational amplitude: multi-H diagrams and classical 5PM logarithms","ref_index":33,"is_internal_anchor":false},{"citing_arxiv_id":"2512.10518","citing_title":"Fano and Reflexive Polytopes from Feynman Integrals","ref_index":16,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18544","citing_title":"The Classical Gravitational Impulse at High Energies","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2508.02800","citing_title":"Towards Motivic Coactions at Genus One from Zeta Generators","ref_index":97,"is_internal_anchor":false},{"citing_arxiv_id":"2508.10761","citing_title":"Unexpected Symmetries of Kerr Black Hole Scattering","ref_index":33,"is_internal_anchor":false},{"citing_arxiv_id":"2509.04425","citing_title":"Hidden simplicity in the scattering for neutron stars and black holes","ref_index":43,"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":131,"is_internal_anchor":false},{"citing_arxiv_id":"2512.02274","citing_title":"Gravitational radiation from hyperbolic orbits: comparison between self-force, post-Minkowskian, post-Newtonian, and numerical relativity results","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2512.13794","citing_title":"The spectrum of Feynman-integral geometries at two loops","ref_index":67,"is_internal_anchor":false},{"citing_arxiv_id":"2601.08252","citing_title":"Resumming Scattering Amplitudes for Waveforms","ref_index":28,"is_internal_anchor":false},{"citing_arxiv_id":"2601.22697","citing_title":"A complex-linear reformulation of Hamilton-Jacobi theory and emergent quantum structure","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2602.06947","citing_title":"The gravitational Compton amplitude at third post-Minkowskian order","ref_index":52,"is_internal_anchor":false},{"citing_arxiv_id":"2605.12214","citing_title":"A Runway to Dissipation of Angular Momentum via Worldline Quantum Field Theory","ref_index":47,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25916","citing_title":"Nonlocal-in-time tail effects in gravitational scattering to fifth Post-Minkowskian and tenth self-force orders","ref_index":67,"is_internal_anchor":false},{"citing_arxiv_id":"2604.25270","citing_title":"Integrand Analysis, Leading Singularities and Canonical Bases beyond Polylogarithms","ref_index":49,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22009","citing_title":"Black Hole Response Theory and its Exact Shockwave Limit","ref_index":87,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14134","citing_title":"All-order structure of static gravitational interactions and the seventh post-Newtonian potential","ref_index":59,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09545","citing_title":"Black Hole Dynamics at Fifth Post-Newtonian Order","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2604.09129","citing_title":"Picard-Fuchs Equations of Twisted Differential forms associated to Feynman Integrals","ref_index":24,"is_internal_anchor":false},{"citing_arxiv_id":"2503.12263","citing_title":"The Science of the Einstein Telescope","ref_index":236,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y","json":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y.json","graph_json":"https://pith.science/api/pith-number/HNUIKTZ5LMDB2FNC5HAQHL554Y/graph.json","events_json":"https://pith.science/api/pith-number/HNUIKTZ5LMDB2FNC5HAQHL554Y/events.json","paper":"https://pith.science/paper/HNUIKTZ5"},"agent_actions":{"view_html":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y","download_json":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y.json","view_paper":"https://pith.science/paper/HNUIKTZ5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.11846&json=true","fetch_graph":"https://pith.science/api/pith-number/HNUIKTZ5LMDB2FNC5HAQHL554Y/graph.json","fetch_events":"https://pith.science/api/pith-number/HNUIKTZ5LMDB2FNC5HAQHL554Y/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y/action/storage_attestation","attest_author":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y/action/author_attestation","sign_citation":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y/action/citation_signature","submit_replication":"https://pith.science/pith/HNUIKTZ5LMDB2FNC5HAQHL554Y/action/replication_record"}},"created_at":"2026-05-21T18:25:30.063906+00:00","updated_at":"2026-05-21T18:25:30.063906+00:00"}