{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:43YFDO3NDFX2ZJ6EPJIC6RAHF4","short_pith_number":"pith:43YFDO3N","schema_version":"1.0","canonical_sha256":"e6f051bb6d196faca7c47a502f44072f2876958da10e1d31c35e089ca1904b50","source":{"kind":"arxiv","id":"2504.06907","version":3},"attestation_state":"computed","paper":{"title":"Thermodynamic phase transition and Joule-Thomson expansion of a quantum corrected black hole in AdS spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Jian-Bo Deng, Lei You, Rui-bo Wang, Shi-Jie Ma, Xian-Ru Hu","submitted_at":"2025-04-09T14:09:26Z","abstract_excerpt":"The thermodynamics in the extended phase space of a quantum corrected black hole (BH) proposed recently is presented in this work. Our study shows that the phase transition behavior of the BH is analogous to that of conventional Schwarzschild BH in anti-de Sitter (AdS) space; however, a critical temperature exists such that when the BH temperature exceeds this critical value, the small BH phase and the large BH phase become separated, and no phase transition occurs. Due to the introduction of the quantum parameter $\\xi$, the BH equation of state splits into two branches. One branch reduces to "},"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":"2504.06907","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-04-09T14:09:26Z","cross_cats_sorted":[],"title_canon_sha256":"b248814581ee0111808fb6297e85b6118ce52c57e9e85334ca9dbd0aaf73f454","abstract_canon_sha256":"dc9ee8299ec5c92adf544c85b694a79b53723e2c3810dbd5f436ec98dd215785"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:57:35.674776Z","signature_b64":"Mh5k8WkS6KjcUXhg0nzlFN/ooFwtkyLdh/HscH60ttWWmbSLyg46wJw1Gg1d6jr9E6raOxjZ7GkgUtFBdhc5CQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e6f051bb6d196faca7c47a502f44072f2876958da10e1d31c35e089ca1904b50","last_reissued_at":"2026-07-05T11:57:35.674341Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:57:35.674341Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermodynamic phase transition and Joule-Thomson expansion of a quantum corrected black hole in AdS spacetime","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Jian-Bo Deng, Lei You, Rui-bo Wang, Shi-Jie Ma, Xian-Ru Hu","submitted_at":"2025-04-09T14:09:26Z","abstract_excerpt":"The thermodynamics in the extended phase space of a quantum corrected black hole (BH) proposed recently is presented in this work. Our study shows that the phase transition behavior of the BH is analogous to that of conventional Schwarzschild BH in anti-de Sitter (AdS) space; however, a critical temperature exists such that when the BH temperature exceeds this critical value, the small BH phase and the large BH phase become separated, and no phase transition occurs. Due to the introduction of the quantum parameter $\\xi$, the BH equation of state splits into two branches. One branch reduces to "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.06907","kind":"arxiv","version":3},"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/2504.06907/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":"2504.06907","created_at":"2026-07-05T11:57:35.674400+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.06907v3","created_at":"2026-07-05T11:57:35.674400+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.06907","created_at":"2026-07-05T11:57:35.674400+00:00"},{"alias_kind":"pith_short_12","alias_value":"43YFDO3NDFX2","created_at":"2026-07-05T11:57:35.674400+00:00"},{"alias_kind":"pith_short_16","alias_value":"43YFDO3NDFX2ZJ6E","created_at":"2026-07-05T11:57:35.674400+00:00"},{"alias_kind":"pith_short_8","alias_value":"43YFDO3N","created_at":"2026-07-05T11:57:35.674400+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.17476","citing_title":"Joule-Thomson effect and Efficiency of deformed AdS-Schwarzschild black hole in presence of quintessence","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4","json":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4.json","graph_json":"https://pith.science/api/pith-number/43YFDO3NDFX2ZJ6EPJIC6RAHF4/graph.json","events_json":"https://pith.science/api/pith-number/43YFDO3NDFX2ZJ6EPJIC6RAHF4/events.json","paper":"https://pith.science/paper/43YFDO3N"},"agent_actions":{"view_html":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4","download_json":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4.json","view_paper":"https://pith.science/paper/43YFDO3N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.06907&json=true","fetch_graph":"https://pith.science/api/pith-number/43YFDO3NDFX2ZJ6EPJIC6RAHF4/graph.json","fetch_events":"https://pith.science/api/pith-number/43YFDO3NDFX2ZJ6EPJIC6RAHF4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4/action/storage_attestation","attest_author":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4/action/author_attestation","sign_citation":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4/action/citation_signature","submit_replication":"https://pith.science/pith/43YFDO3NDFX2ZJ6EPJIC6RAHF4/action/replication_record"}},"created_at":"2026-07-05T11:57:35.674400+00:00","updated_at":"2026-07-05T11:57:35.674400+00:00"}