{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:56HBQISHDUYAQYNOSE3APBLVAL","short_pith_number":"pith:56HBQISH","schema_version":"1.0","canonical_sha256":"ef8e1822471d300861ae913607857502dead6eb26573421b8f33557ff5469a38","source":{"kind":"arxiv","id":"2506.14626","version":2},"attestation_state":"computed","paper":{"title":"Spinning the Probe in Kerr with WQFT","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Gustav Uhre Jakobsen, Jan Plefka, Jitze Hoogeveen","submitted_at":"2025-06-17T15:22:30Z","abstract_excerpt":"We investigate the gravitational scattering of a spinning probe mass in a Kerr background using the worldline quantum field theory (WQFT) approach. This corresponds to the leading term (0SF) in the gravitational self-force expansion for the spinning two-body problem with large mass hierarchy. By reformulating the geodesic and Mathisson-Papapetrou-Dixon equations as a recursive Berends-Giele type equation known from multi-gluon scattering, we develop a novel integration-by-parts formalism on the worldline that enables systematic computation of scattering observables - specifically the impulse a"},"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":"2506.14626","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2025-06-17T15:22:30Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"26bfbe8368c968092170c2cd7eb94be2d6c5364332506a9d07b53b4a905db51c","abstract_canon_sha256":"a341f197d6c89159572e6b3d8aa47e5a253e91e130228d3e318ac8abbcbfb3f1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:35:35.526303Z","signature_b64":"+4a2hEystww6gLvRL7nU8bKV3gnEjgtLTIV8iXf3uCvk+ORaRRcb8DrEGjPo4rNPKllaP6XNmKuYOS3sHCoBAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"ef8e1822471d300861ae913607857502dead6eb26573421b8f33557ff5469a38","last_reissued_at":"2026-07-05T11:35:35.525813Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:35:35.525813Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spinning the Probe in Kerr with WQFT","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Gustav Uhre Jakobsen, Jan Plefka, Jitze Hoogeveen","submitted_at":"2025-06-17T15:22:30Z","abstract_excerpt":"We investigate the gravitational scattering of a spinning probe mass in a Kerr background using the worldline quantum field theory (WQFT) approach. This corresponds to the leading term (0SF) in the gravitational self-force expansion for the spinning two-body problem with large mass hierarchy. By reformulating the geodesic and Mathisson-Papapetrou-Dixon equations as a recursive Berends-Giele type equation known from multi-gluon scattering, we develop a novel integration-by-parts formalism on the worldline that enables systematic computation of scattering observables - specifically the impulse a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.14626","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/2506.14626/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":"2506.14626","created_at":"2026-07-05T11:35:35.525878+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.14626v2","created_at":"2026-07-05T11:35:35.525878+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.14626","created_at":"2026-07-05T11:35:35.525878+00:00"},{"alias_kind":"pith_short_12","alias_value":"56HBQISHDUYA","created_at":"2026-07-05T11:35:35.525878+00:00"},{"alias_kind":"pith_short_16","alias_value":"56HBQISHDUYAQYNO","created_at":"2026-07-05T11:35:35.525878+00:00"},{"alias_kind":"pith_short_8","alias_value":"56HBQISH","created_at":"2026-07-05T11:35:35.525878+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.29831","citing_title":"Five-dimensional Geometry from Spinning Amplitudes","ref_index":81,"is_internal_anchor":false},{"citing_arxiv_id":"2508.10761","citing_title":"Unexpected Symmetries of Kerr Black Hole Scattering","ref_index":116,"is_internal_anchor":false},{"citing_arxiv_id":"2509.04425","citing_title":"Hidden simplicity in the scattering for neutron stars and black holes","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2603.27353","citing_title":"Universality in Relativistic Spinning Particle Models","ref_index":171,"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":53,"is_internal_anchor":false},{"citing_arxiv_id":"2604.22009","citing_title":"Black Hole Response Theory and its Exact Shockwave Limit","ref_index":149,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL","json":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL.json","graph_json":"https://pith.science/api/pith-number/56HBQISHDUYAQYNOSE3APBLVAL/graph.json","events_json":"https://pith.science/api/pith-number/56HBQISHDUYAQYNOSE3APBLVAL/events.json","paper":"https://pith.science/paper/56HBQISH"},"agent_actions":{"view_html":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL","download_json":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL.json","view_paper":"https://pith.science/paper/56HBQISH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.14626&json=true","fetch_graph":"https://pith.science/api/pith-number/56HBQISHDUYAQYNOSE3APBLVAL/graph.json","fetch_events":"https://pith.science/api/pith-number/56HBQISHDUYAQYNOSE3APBLVAL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL/action/storage_attestation","attest_author":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL/action/author_attestation","sign_citation":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL/action/citation_signature","submit_replication":"https://pith.science/pith/56HBQISHDUYAQYNOSE3APBLVAL/action/replication_record"}},"created_at":"2026-07-05T11:35:35.525878+00:00","updated_at":"2026-07-05T11:35:35.525878+00:00"}