{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:FHXKSTKSTWRYPYGDOJZ5H24TTO","short_pith_number":"pith:FHXKSTKS","schema_version":"1.0","canonical_sha256":"29eea94d529da387e0c37273d3eb939b913430e537d76dfab409a9425296a967","source":{"kind":"arxiv","id":"2507.03082","version":1},"attestation_state":"computed","paper":{"title":"Dynamical black holes and accretion-induced backreaction","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"C. Molina, Mario C. Baldiotti, Thiago de L. Campos","submitted_at":"2025-07-03T18:00:11Z","abstract_excerpt":"We investigate the evolution of future trapping horizons through the dynamics of the Misner-Sharp mass using ingoing Eddington-Finkelstein coordinates. Our analysis shows that an integral formulation of Hayward's first law governs much of the evolution of general spherically symmetric spacetimes. To account for the accretion backreaction, we consider a near-horizon approximation, yielding first-order corrections of a Vaidya-dark energy form. We further propose a systematic perturbative scheme to study these effects for an arbitrary background. As an application, we analyze an accreting Reissne"},"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":"2507.03082","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2025-07-03T18:00:11Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"e72062624a6b3c71e99a85dab9fbd6706944ec10e7d40ca7ce11f42a8a9c5673","abstract_canon_sha256":"3446d4c8496a185b7938d7ba6cd975600135166dc488676d05326f269678ca09"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:31:52.357460Z","signature_b64":"Je39JA4MZFYxs4XGQ1nHEgIoNez85/4oBLJyS+wofCxwSsVWDpCohkipSe7mmqHh1nxi+4qi3fg0kcZaV1qYAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"29eea94d529da387e0c37273d3eb939b913430e537d76dfab409a9425296a967","last_reissued_at":"2026-07-05T11:31:52.356973Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:31:52.356973Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dynamical black holes and accretion-induced backreaction","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"C. Molina, Mario C. Baldiotti, Thiago de L. Campos","submitted_at":"2025-07-03T18:00:11Z","abstract_excerpt":"We investigate the evolution of future trapping horizons through the dynamics of the Misner-Sharp mass using ingoing Eddington-Finkelstein coordinates. Our analysis shows that an integral formulation of Hayward's first law governs much of the evolution of general spherically symmetric spacetimes. To account for the accretion backreaction, we consider a near-horizon approximation, yielding first-order corrections of a Vaidya-dark energy form. We further propose a systematic perturbative scheme to study these effects for an arbitrary background. As an application, we analyze an accreting Reissne"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2507.03082","kind":"arxiv","version":1},"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/2507.03082/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":"2507.03082","created_at":"2026-07-05T11:31:52.357028+00:00"},{"alias_kind":"arxiv_version","alias_value":"2507.03082v1","created_at":"2026-07-05T11:31:52.357028+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2507.03082","created_at":"2026-07-05T11:31:52.357028+00:00"},{"alias_kind":"pith_short_12","alias_value":"FHXKSTKSTWRY","created_at":"2026-07-05T11:31:52.357028+00:00"},{"alias_kind":"pith_short_16","alias_value":"FHXKSTKSTWRYPYGD","created_at":"2026-07-05T11:31:52.357028+00:00"},{"alias_kind":"pith_short_8","alias_value":"FHXKSTKS","created_at":"2026-07-05T11:31:52.357028+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.24091","citing_title":"Hawking atmosphere of anti-de Sitter black holes","ref_index":25,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO","json":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO.json","graph_json":"https://pith.science/api/pith-number/FHXKSTKSTWRYPYGDOJZ5H24TTO/graph.json","events_json":"https://pith.science/api/pith-number/FHXKSTKSTWRYPYGDOJZ5H24TTO/events.json","paper":"https://pith.science/paper/FHXKSTKS"},"agent_actions":{"view_html":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO","download_json":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO.json","view_paper":"https://pith.science/paper/FHXKSTKS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2507.03082&json=true","fetch_graph":"https://pith.science/api/pith-number/FHXKSTKSTWRYPYGDOJZ5H24TTO/graph.json","fetch_events":"https://pith.science/api/pith-number/FHXKSTKSTWRYPYGDOJZ5H24TTO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO/action/storage_attestation","attest_author":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO/action/author_attestation","sign_citation":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO/action/citation_signature","submit_replication":"https://pith.science/pith/FHXKSTKSTWRYPYGDOJZ5H24TTO/action/replication_record"}},"created_at":"2026-07-05T11:31:52.357028+00:00","updated_at":"2026-07-05T11:31:52.357028+00:00"}