{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:ZC2P45TDOKKF6PDKJDFZ3J672K","short_pith_number":"pith:ZC2P45TD","schema_version":"1.0","canonical_sha256":"c8b4fe766372945f3c6a48cb9da7dfd29d0410597fe9c7fb433bfeb6e6d71a32","source":{"kind":"arxiv","id":"2203.09394","version":1},"attestation_state":"computed","paper":{"title":"EUP-corrected thermodynamics of BTZ black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["quant-ph"],"primary_cat":"gr-qc","authors_text":"B. C. L\\\"utf\\\"uo\\u{g}lu, B. Hamil, L. Dahbi","submitted_at":"2022-03-17T15:36:30Z","abstract_excerpt":"In this manuscript, we investigate the influence of the extended uncertainty principle (EUP) on the thermodynamics of a charged rotating Ba\\~{n}ados, Teitelboim and Zanelli (BTZ) black hole in (2+1)-dimensional anti-de Sitter (AdS) and de Sitter (dS) space-time, respectively. We find that EUP-corrected Hawking temperature, entropy, volume, Gibbs free energy, pressure, and heat capacity functions have different characteristic behaviors in (A)dS space-time. During the detailed analysis, we obtain a critical horizon in the AdS space-time where the pressure has a non-zero minimum value. However, i"},"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":"2203.09394","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2022-03-17T15:36:30Z","cross_cats_sorted":["quant-ph"],"title_canon_sha256":"bc307f1e0a460b42257cc4f1f1ca5e2eae9526f87a6f962bd3ed2c068e0a997d","abstract_canon_sha256":"35246b3714db1d41a7056b5b829b09c113a2aa6c7bf2755beb138527008fe4b6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:29:18.074232Z","signature_b64":"dIBMzGoPvbHqjB1ceiCILQCdHgBA6Tl/kh7KP18auUxK7Fkg/z3ZnUqo66L1IYdLUq8Ynz77PBCsUZjarS9BCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c8b4fe766372945f3c6a48cb9da7dfd29d0410597fe9c7fb433bfeb6e6d71a32","last_reissued_at":"2026-07-05T05:29:18.073782Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:29:18.073782Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"EUP-corrected thermodynamics of BTZ black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["quant-ph"],"primary_cat":"gr-qc","authors_text":"B. C. L\\\"utf\\\"uo\\u{g}lu, B. Hamil, L. Dahbi","submitted_at":"2022-03-17T15:36:30Z","abstract_excerpt":"In this manuscript, we investigate the influence of the extended uncertainty principle (EUP) on the thermodynamics of a charged rotating Ba\\~{n}ados, Teitelboim and Zanelli (BTZ) black hole in (2+1)-dimensional anti-de Sitter (AdS) and de Sitter (dS) space-time, respectively. We find that EUP-corrected Hawking temperature, entropy, volume, Gibbs free energy, pressure, and heat capacity functions have different characteristic behaviors in (A)dS space-time. During the detailed analysis, we obtain a critical horizon in the AdS space-time where the pressure has a non-zero minimum value. However, i"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.09394","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/2203.09394/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":"2203.09394","created_at":"2026-07-05T05:29:18.073839+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.09394v1","created_at":"2026-07-05T05:29:18.073839+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.09394","created_at":"2026-07-05T05:29:18.073839+00:00"},{"alias_kind":"pith_short_12","alias_value":"ZC2P45TDOKKF","created_at":"2026-07-05T05:29:18.073839+00:00"},{"alias_kind":"pith_short_16","alias_value":"ZC2P45TDOKKF6PDK","created_at":"2026-07-05T05:29:18.073839+00:00"},{"alias_kind":"pith_short_8","alias_value":"ZC2P45TD","created_at":"2026-07-05T05:29:18.073839+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2506.00295","citing_title":"Extended uncertainty principle inspired black hole in a G\\\"odel Universe","ref_index":19,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K","json":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K.json","graph_json":"https://pith.science/api/pith-number/ZC2P45TDOKKF6PDKJDFZ3J672K/graph.json","events_json":"https://pith.science/api/pith-number/ZC2P45TDOKKF6PDKJDFZ3J672K/events.json","paper":"https://pith.science/paper/ZC2P45TD"},"agent_actions":{"view_html":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K","download_json":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K.json","view_paper":"https://pith.science/paper/ZC2P45TD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.09394&json=true","fetch_graph":"https://pith.science/api/pith-number/ZC2P45TDOKKF6PDKJDFZ3J672K/graph.json","fetch_events":"https://pith.science/api/pith-number/ZC2P45TDOKKF6PDKJDFZ3J672K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K/action/storage_attestation","attest_author":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K/action/author_attestation","sign_citation":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K/action/citation_signature","submit_replication":"https://pith.science/pith/ZC2P45TDOKKF6PDKJDFZ3J672K/action/replication_record"}},"created_at":"2026-07-05T05:29:18.073839+00:00","updated_at":"2026-07-05T05:29:18.073839+00:00"}