{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:JY3UG2LE6PZ6WRASFHL3LSJGWW","short_pith_number":"pith:JY3UG2LE","schema_version":"1.0","canonical_sha256":"4e37436964f3f3eb441229d7b5c926b58f9370dcfd541c625e5b6772cb1c53d4","source":{"kind":"arxiv","id":"2411.03382","version":2},"attestation_state":"computed","paper":{"title":"Absorptive Effects in Black Hole Scattering","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jung-Wook Kim, Yilber Fabian Bautista, Yu-tin Huang","submitted_at":"2024-11-05T18:11:00Z","abstract_excerpt":"In this paper we define absorptive Compton amplitudes, which captures the absorption factor for waves of spin-weight-$s$ scattering in black hole perturbation theory. At the leading order, in the $G M \\omega$ expansion, such amplitudes are purely imaginary and expressible as contact terms. Equipped with these amplitudes we compute the mass change in black hole scattering events via Kosower-Maybee-O'Connell formalism, where the rest mass of Schwarzschild/Kerr black hole is modified due to absorption of gravitational, electromagnetic, or scalar fields sourced by other compact object. We reproduc"},"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":"2411.03382","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-11-05T18:11:00Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"b30c839b5ed83a17ff62cf4ad8cf3773eeda21ff9027b47a319b282399ca419a","abstract_canon_sha256":"2013374b7cee6e7b0cbe18ab91c835e27222b14113771eeb0de774da99e769dd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:03:47.683646Z","signature_b64":"d8G/Jtzv2x+1qRNSPqtFR+tBMXug4xWDFD8XBBZschfO6z5NNREUjca2Q7NwHnftot/wkx/rCqCGFc5jRCjWCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4e37436964f3f3eb441229d7b5c926b58f9370dcfd541c625e5b6772cb1c53d4","last_reissued_at":"2026-07-05T10:03:47.683113Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:03:47.683113Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Absorptive Effects in Black Hole Scattering","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Jung-Wook Kim, Yilber Fabian Bautista, Yu-tin Huang","submitted_at":"2024-11-05T18:11:00Z","abstract_excerpt":"In this paper we define absorptive Compton amplitudes, which captures the absorption factor for waves of spin-weight-$s$ scattering in black hole perturbation theory. At the leading order, in the $G M \\omega$ expansion, such amplitudes are purely imaginary and expressible as contact terms. Equipped with these amplitudes we compute the mass change in black hole scattering events via Kosower-Maybee-O'Connell formalism, where the rest mass of Schwarzschild/Kerr black hole is modified due to absorption of gravitational, electromagnetic, or scalar fields sourced by other compact object. We reproduc"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.03382","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/2411.03382/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":"2411.03382","created_at":"2026-07-05T10:03:47.683172+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.03382v2","created_at":"2026-07-05T10:03:47.683172+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.03382","created_at":"2026-07-05T10:03:47.683172+00:00"},{"alias_kind":"pith_short_12","alias_value":"JY3UG2LE6PZ6","created_at":"2026-07-05T10:03:47.683172+00:00"},{"alias_kind":"pith_short_16","alias_value":"JY3UG2LE6PZ6WRAS","created_at":"2026-07-05T10:03:47.683172+00:00"},{"alias_kind":"pith_short_8","alias_value":"JY3UG2LE","created_at":"2026-07-05T10:03:47.683172+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.13599","citing_title":"Black Hole Thermodynamics Meets On-Shell Amplitudes: Local Detailed Balance and Thermal Spectrum from Spin Universality and Unitarity","ref_index":32,"is_internal_anchor":false},{"citing_arxiv_id":"2606.11705","citing_title":"Horizon absorption in eccentric precessing binary black hole inspirals and its importance for gravitational wave data analysis","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2601.08252","citing_title":"Resumming Scattering Amplitudes for Waveforms","ref_index":94,"is_internal_anchor":false},{"citing_arxiv_id":"2602.06947","citing_title":"The gravitational Compton amplitude at third post-Minkowskian order","ref_index":100,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW","json":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW.json","graph_json":"https://pith.science/api/pith-number/JY3UG2LE6PZ6WRASFHL3LSJGWW/graph.json","events_json":"https://pith.science/api/pith-number/JY3UG2LE6PZ6WRASFHL3LSJGWW/events.json","paper":"https://pith.science/paper/JY3UG2LE"},"agent_actions":{"view_html":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW","download_json":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW.json","view_paper":"https://pith.science/paper/JY3UG2LE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.03382&json=true","fetch_graph":"https://pith.science/api/pith-number/JY3UG2LE6PZ6WRASFHL3LSJGWW/graph.json","fetch_events":"https://pith.science/api/pith-number/JY3UG2LE6PZ6WRASFHL3LSJGWW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW/action/storage_attestation","attest_author":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW/action/author_attestation","sign_citation":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW/action/citation_signature","submit_replication":"https://pith.science/pith/JY3UG2LE6PZ6WRASFHL3LSJGWW/action/replication_record"}},"created_at":"2026-07-05T10:03:47.683172+00:00","updated_at":"2026-07-05T10:03:47.683172+00:00"}