{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:OX337OGXM75Y4JUFBBSB5M43HS","short_pith_number":"pith:OX337OGX","schema_version":"1.0","canonical_sha256":"75f7bfb8d767fb8e268508641eb39b3c8f77ed96f49905d272e06b963e83a6a9","source":{"kind":"arxiv","id":"2310.00069","version":2},"attestation_state":"computed","paper":{"title":"Absorptive Effects and Classical Black Hole Scattering","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Callum R. T. Jones, Michael S. Ruf","submitted_at":"2023-09-29T18:19:44Z","abstract_excerpt":"We describe an approach to incorporating the physical effects of the absorption of energy by the event horizon of black holes in the scattering amplitudes based post-Minkowskian, point-particle effective description. Absorptive dynamics are incorporated in a model-independent way by coupling the usual point-particle description to an invisible sector of gapless internal degrees-of-freedom. The leading order dynamics of this sector are encoded in the low-energy expansion of a spectral density function obtained by matching an absorption cross section in the ultraviolet description. This informat"},"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":"2310.00069","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2023-09-29T18:19:44Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"112cf3b50d7ff6fb35647985b2bac2a8e5122b76b94751fe9319462dd896c322","abstract_canon_sha256":"aa97635c0adf686d0c1f69a1e82e92e6a919b15533ccb739b11a8debb9dba0bb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:51:32.962839Z","signature_b64":"dn/Ydxk1sU+VPV2VsGfuXkEiqj6zo4rT5XXndIoSVyPLg1H7FHnJxdTFf7lWRqG2Mb6aI+OZd2tKTqWycRF2AQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"75f7bfb8d767fb8e268508641eb39b3c8f77ed96f49905d272e06b963e83a6a9","last_reissued_at":"2026-07-05T07:51:32.962359Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:51:32.962359Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Absorptive Effects and Classical Black Hole Scattering","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Callum R. T. Jones, Michael S. Ruf","submitted_at":"2023-09-29T18:19:44Z","abstract_excerpt":"We describe an approach to incorporating the physical effects of the absorption of energy by the event horizon of black holes in the scattering amplitudes based post-Minkowskian, point-particle effective description. Absorptive dynamics are incorporated in a model-independent way by coupling the usual point-particle description to an invisible sector of gapless internal degrees-of-freedom. The leading order dynamics of this sector are encoded in the low-energy expansion of a spectral density function obtained by matching an absorption cross section in the ultraviolet description. This informat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.00069","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/2310.00069/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":"2310.00069","created_at":"2026-07-05T07:51:32.962415+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.00069v2","created_at":"2026-07-05T07:51:32.962415+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.00069","created_at":"2026-07-05T07:51:32.962415+00:00"},{"alias_kind":"pith_short_12","alias_value":"OX337OGXM75Y","created_at":"2026-07-05T07:51:32.962415+00:00"},{"alias_kind":"pith_short_16","alias_value":"OX337OGXM75Y4JUF","created_at":"2026-07-05T07:51:32.962415+00:00"},{"alias_kind":"pith_short_8","alias_value":"OX337OGX","created_at":"2026-07-05T07:51:32.962415+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"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":29,"is_internal_anchor":false},{"citing_arxiv_id":"2606.12528","citing_title":"How traversable is a traversable wormhole?","ref_index":70,"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":70,"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":46,"is_internal_anchor":false},{"citing_arxiv_id":"2601.08252","citing_title":"Resumming Scattering Amplitudes for Waveforms","ref_index":91,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS","json":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS.json","graph_json":"https://pith.science/api/pith-number/OX337OGXM75Y4JUFBBSB5M43HS/graph.json","events_json":"https://pith.science/api/pith-number/OX337OGXM75Y4JUFBBSB5M43HS/events.json","paper":"https://pith.science/paper/OX337OGX"},"agent_actions":{"view_html":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS","download_json":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS.json","view_paper":"https://pith.science/paper/OX337OGX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.00069&json=true","fetch_graph":"https://pith.science/api/pith-number/OX337OGXM75Y4JUFBBSB5M43HS/graph.json","fetch_events":"https://pith.science/api/pith-number/OX337OGXM75Y4JUFBBSB5M43HS/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS/action/storage_attestation","attest_author":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS/action/author_attestation","sign_citation":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS/action/citation_signature","submit_replication":"https://pith.science/pith/OX337OGXM75Y4JUFBBSB5M43HS/action/replication_record"}},"created_at":"2026-07-05T07:51:32.962415+00:00","updated_at":"2026-07-05T07:51:32.962415+00:00"}