{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:TRE7YJYZCTMWSDO76YKTB5NEU5","short_pith_number":"pith:TRE7YJYZ","schema_version":"1.0","canonical_sha256":"9c49fc271914d9690ddff61530f5a4a746e1e163757125d3cf31efc2bc89c94c","source":{"kind":"arxiv","id":"gr-qc/0505015","version":2},"attestation_state":"computed","paper":{"title":"On Hawking Radiation as Tunneling with Logarithmic Corrections","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"A.J.M. Medved, Elias C. Vagenas","submitted_at":"2005-05-03T19:29:39Z","abstract_excerpt":"There has been recent speculation that the tunneling paradigm for Hawking radiation could -- after quantum-gravitational effects have suitably been incorporated -- provide a means for resolving the (black hole) information loss paradox. A prospective quantum-gravitational effect is the logarithmic-order correction to the Bekenstein-Hawking entropy/area law. In this letter, it is demonstrated that, even with the inclusion of the logarithmic correction (or, indeed, the quantum correction up to any perturbative order), the tunneling formalism is still unable to resolve the stated paradox. Moreove"},"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":"gr-qc/0505015","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"gr-qc","submitted_at":"2005-05-03T19:29:39Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"9e5bb64d02060510f1e59058dd45390cea20b471815f730b4c735460d7c46fab","abstract_canon_sha256":"1bd7d2f0a2be5c3cbe0b74502fc8d7d039b3a0d75d1d7870057b4a0732ba69f4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:55:13.594690Z","signature_b64":"/e2Rw69T9q+POL2mzg+rMm1DzSVUMcMBRObExWAbOb4RTbgWdQWxUiS9oJ14RFs9d/Ee7ZsV0iiDnDkPQIGmBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c49fc271914d9690ddff61530f5a4a746e1e163757125d3cf31efc2bc89c94c","last_reissued_at":"2026-07-04T16:55:13.594298Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:55:13.594298Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On Hawking Radiation as Tunneling with Logarithmic Corrections","license":"","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"A.J.M. Medved, Elias C. Vagenas","submitted_at":"2005-05-03T19:29:39Z","abstract_excerpt":"There has been recent speculation that the tunneling paradigm for Hawking radiation could -- after quantum-gravitational effects have suitably been incorporated -- provide a means for resolving the (black hole) information loss paradox. A prospective quantum-gravitational effect is the logarithmic-order correction to the Bekenstein-Hawking entropy/area law. In this letter, it is demonstrated that, even with the inclusion of the logarithmic correction (or, indeed, the quantum correction up to any perturbative order), the tunneling formalism is still unable to resolve the stated paradox. Moreove"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"gr-qc/0505015","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/gr-qc/0505015/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":"gr-qc/0505015","created_at":"2026-07-04T16:55:13.594372+00:00"},{"alias_kind":"arxiv_version","alias_value":"gr-qc/0505015v2","created_at":"2026-07-04T16:55:13.594372+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.gr-qc/0505015","created_at":"2026-07-04T16:55:13.594372+00:00"},{"alias_kind":"pith_short_12","alias_value":"TRE7YJYZCTMW","created_at":"2026-07-04T16:55:13.594372+00:00"},{"alias_kind":"pith_short_16","alias_value":"TRE7YJYZCTMWSDO7","created_at":"2026-07-04T16:55:13.594372+00:00"},{"alias_kind":"pith_short_8","alias_value":"TRE7YJYZ","created_at":"2026-07-04T16:55:13.594372+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2508.01559","citing_title":"Statistical Entropy Based on the Generalized-Uncertainty-Principle-Induced Effective Metric","ref_index":57,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5","json":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5.json","graph_json":"https://pith.science/api/pith-number/TRE7YJYZCTMWSDO76YKTB5NEU5/graph.json","events_json":"https://pith.science/api/pith-number/TRE7YJYZCTMWSDO76YKTB5NEU5/events.json","paper":"https://pith.science/paper/TRE7YJYZ"},"agent_actions":{"view_html":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5","download_json":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5.json","view_paper":"https://pith.science/paper/TRE7YJYZ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=gr-qc/0505015&json=true","fetch_graph":"https://pith.science/api/pith-number/TRE7YJYZCTMWSDO76YKTB5NEU5/graph.json","fetch_events":"https://pith.science/api/pith-number/TRE7YJYZCTMWSDO76YKTB5NEU5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5/action/storage_attestation","attest_author":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5/action/author_attestation","sign_citation":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5/action/citation_signature","submit_replication":"https://pith.science/pith/TRE7YJYZCTMWSDO76YKTB5NEU5/action/replication_record"}},"created_at":"2026-07-04T16:55:13.594372+00:00","updated_at":"2026-07-04T16:55:13.594372+00:00"}