{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:MFEODZLCM6NFG42ND656NL5R4F","short_pith_number":"pith:MFEODZLC","schema_version":"1.0","canonical_sha256":"6148e1e562679a53734d1fbbe6afb1e152a44cd8da9a5838a0cbf6dde45e9aa7","source":{"kind":"arxiv","id":"2506.15261","version":2},"attestation_state":"computed","paper":{"title":"Quantum-corrected black hole thermodynamics from the gravitational path integral","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Hao-Wei Yu, Peng Cheng, Yu-Qi Liu","submitted_at":"2025-06-18T08:39:28Z","abstract_excerpt":"Exploring quantum effects from black hole thermodynamics has always been a pivotal topic. In recent years, the free energy landscape and ensemble-averaged theory based on the Euclidean path integral approach have provided further understanding of the statistical aspects of the black hole system. We investigate the quantum-corrected thermodynamics of the Reissner-Nordstrom AdS black hole by including off-shell geometries in a reduced gravitational path integral. Within this collective-variable approximation, we derive an effective action by considering the subleading-order terms in the ensemble"},"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":"2506.15261","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2025-06-18T08:39:28Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"ff1cecbac60663fe6d659757c04aae3ac273bc6693f6c0257e7251b18db61247","abstract_canon_sha256":"87ef4fdcdb22200e51fc5f090f3d54ec7dd1a82a54883cb6ae1c50f26a8eeb8a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-08T01:03:45.860842Z","signature_b64":"Sim0eG91k1/fu4IeQ/9p+rqxlZPV4NrrhZkxb9aG6cyDQwp6NGe+jBi29Ai4XoT07NYo2vN+431F0Lf8J9KuCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6148e1e562679a53734d1fbbe6afb1e152a44cd8da9a5838a0cbf6dde45e9aa7","last_reissued_at":"2026-06-08T01:03:45.859966Z","signature_status":"signed_v1","first_computed_at":"2026-06-08T01:03:45.859966Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quantum-corrected black hole thermodynamics from the gravitational path integral","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Hao-Wei Yu, Peng Cheng, Yu-Qi Liu","submitted_at":"2025-06-18T08:39:28Z","abstract_excerpt":"Exploring quantum effects from black hole thermodynamics has always been a pivotal topic. In recent years, the free energy landscape and ensemble-averaged theory based on the Euclidean path integral approach have provided further understanding of the statistical aspects of the black hole system. We investigate the quantum-corrected thermodynamics of the Reissner-Nordstrom AdS black hole by including off-shell geometries in a reduced gravitational path integral. Within this collective-variable approximation, we derive an effective action by considering the subleading-order terms in the ensemble"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.15261","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/2506.15261/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":"2506.15261","created_at":"2026-06-08T01:03:45.860079+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.15261v2","created_at":"2026-06-08T01:03:45.860079+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.15261","created_at":"2026-06-08T01:03:45.860079+00:00"},{"alias_kind":"pith_short_12","alias_value":"MFEODZLCM6NF","created_at":"2026-06-08T01:03:45.860079+00:00"},{"alias_kind":"pith_short_16","alias_value":"MFEODZLCM6NFG42N","created_at":"2026-06-08T01:03:45.860079+00:00"},{"alias_kind":"pith_short_8","alias_value":"MFEODZLC","created_at":"2026-06-08T01:03:45.860079+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2509.03656","citing_title":"Loops Outside a Black Hole","ref_index":81,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F","json":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F.json","graph_json":"https://pith.science/api/pith-number/MFEODZLCM6NFG42ND656NL5R4F/graph.json","events_json":"https://pith.science/api/pith-number/MFEODZLCM6NFG42ND656NL5R4F/events.json","paper":"https://pith.science/paper/MFEODZLC"},"agent_actions":{"view_html":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F","download_json":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F.json","view_paper":"https://pith.science/paper/MFEODZLC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.15261&json=true","fetch_graph":"https://pith.science/api/pith-number/MFEODZLCM6NFG42ND656NL5R4F/graph.json","fetch_events":"https://pith.science/api/pith-number/MFEODZLCM6NFG42ND656NL5R4F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F/action/storage_attestation","attest_author":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F/action/author_attestation","sign_citation":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F/action/citation_signature","submit_replication":"https://pith.science/pith/MFEODZLCM6NFG42ND656NL5R4F/action/replication_record"}},"created_at":"2026-06-08T01:03:45.860079+00:00","updated_at":"2026-06-08T01:03:45.860079+00:00"}