{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:67KRP55HAPBNPZI7F3OZB6XD6S","short_pith_number":"pith:67KRP55H","schema_version":"1.0","canonical_sha256":"f7d517f7a703c2d7e51f2edd90fae3f4bb27dfcf2780c853028157a2efb3837b","source":{"kind":"arxiv","id":"2506.15886","version":4},"attestation_state":"computed","paper":{"title":"Higher-curvature corrections and the endpoint of black hole evaporation in gravitational effective field theory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Andrea Fuster, Federico Toschi, Lorens F. Niehof, Sjors Heefer","submitted_at":"2025-06-18T21:23:37Z","abstract_excerpt":"The endpoint of black hole evaporation remains uncertain once the semiclassical description approaches the Planck scale. In this work we study late-stage evaporation within four-dimensional gravitational effective field theory. We consider the leading local correction to the Schwarzschild solution arising from a cubic curvature operator, and use the corrected geometry to analyze the resulting evaporation dynamics and associated thermodynamic properties.\n  We show that the cubic correction induces a parametric slow-down of the evaporation rate at small masses, which within the truncated theory "},"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":"2506.15886","kind":"arxiv","version":4},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2025-06-18T21:23:37Z","cross_cats_sorted":[],"title_canon_sha256":"ca29dedf033120b55964f854cffffe298db750eb00a1be1a92dbc99d6517f9cc","abstract_canon_sha256":"b80784c3dc27312c2847a33c6a5e1f44af7079eb50ade3151a53ef855076eff5"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-29T01:04:54.124789Z","signature_b64":"4Tm/a48poD8jfOt7VWNsXdO0JqW3wanDG23s2TSVeFpq19ne/Y6MMzqXS6CmW0d7qpbzEJPu9KWDHTHFo9fpBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f7d517f7a703c2d7e51f2edd90fae3f4bb27dfcf2780c853028157a2efb3837b","last_reissued_at":"2026-05-29T01:04:54.124308Z","signature_status":"signed_v1","first_computed_at":"2026-05-29T01:04:54.124308Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Higher-curvature corrections and the endpoint of black hole evaporation in gravitational effective field theory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Andrea Fuster, Federico Toschi, Lorens F. Niehof, Sjors Heefer","submitted_at":"2025-06-18T21:23:37Z","abstract_excerpt":"The endpoint of black hole evaporation remains uncertain once the semiclassical description approaches the Planck scale. In this work we study late-stage evaporation within four-dimensional gravitational effective field theory. We consider the leading local correction to the Schwarzschild solution arising from a cubic curvature operator, and use the corrected geometry to analyze the resulting evaporation dynamics and associated thermodynamic properties.\n  We show that the cubic correction induces a parametric slow-down of the evaporation rate at small masses, which within the truncated theory "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.15886","kind":"arxiv","version":4},"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/2506.15886/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":"2506.15886","created_at":"2026-05-29T01:04:54.124383+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.15886v4","created_at":"2026-05-29T01:04:54.124383+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.15886","created_at":"2026-05-29T01:04:54.124383+00:00"},{"alias_kind":"pith_short_12","alias_value":"67KRP55HAPBN","created_at":"2026-05-29T01:04:54.124383+00:00"},{"alias_kind":"pith_short_16","alias_value":"67KRP55HAPBNPZI7","created_at":"2026-05-29T01:04:54.124383+00:00"},{"alias_kind":"pith_short_8","alias_value":"67KRP55H","created_at":"2026-05-29T01:04:54.124383+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S","json":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S.json","graph_json":"https://pith.science/api/pith-number/67KRP55HAPBNPZI7F3OZB6XD6S/graph.json","events_json":"https://pith.science/api/pith-number/67KRP55HAPBNPZI7F3OZB6XD6S/events.json","paper":"https://pith.science/paper/67KRP55H"},"agent_actions":{"view_html":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S","download_json":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S.json","view_paper":"https://pith.science/paper/67KRP55H","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.15886&json=true","fetch_graph":"https://pith.science/api/pith-number/67KRP55HAPBNPZI7F3OZB6XD6S/graph.json","fetch_events":"https://pith.science/api/pith-number/67KRP55HAPBNPZI7F3OZB6XD6S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S/action/storage_attestation","attest_author":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S/action/author_attestation","sign_citation":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S/action/citation_signature","submit_replication":"https://pith.science/pith/67KRP55HAPBNPZI7F3OZB6XD6S/action/replication_record"}},"created_at":"2026-05-29T01:04:54.124383+00:00","updated_at":"2026-05-29T01:04:54.124383+00:00"}