{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:FFETD5KVOTANQ56RBZVM3IZ633","short_pith_number":"pith:FFETD5KV","schema_version":"1.0","canonical_sha256":"294931f55574c0d877d10e6acda33eded03b355fae27a6f09290b45bff7bb77c","source":{"kind":"arxiv","id":"2405.09151","version":2},"attestation_state":"computed","paper":{"title":"Thermodynamics and kinetics of state switching for the asymptotically flat black hole in a cavity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.stat-mech","hep-th"],"primary_cat":"gr-qc","authors_text":"Jin Wang, Ran Li","submitted_at":"2024-05-15T07:31:15Z","abstract_excerpt":"We propose that the thermodynamics and the kinetics of state switching for the asymptotically flat black hole enclosed by a cavity can be studied in terms of the free energy landscape formalism. The generalized free energy for the black hole enclosed by a cavity in the canonical ensemble is derived by using the York's approach, where the temperature on the cavity and the charges inside the cavity are kept as the fixed parameters. By quantifying the corresponding free energy landscape, we obtain the phase diagrams for the black hole in cavity, which reveal a Hawking-Page type transition for the"},"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":"2405.09151","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-05-15T07:31:15Z","cross_cats_sorted":["cond-mat.stat-mech","hep-th"],"title_canon_sha256":"f579fc7cf0839c981887ae3d85bf39275fed3b18e617b4cc2e7271a9a1962c13","abstract_canon_sha256":"ed96fdb2eb53390f8d54319c425eeb02a1eff5856e5e5c70d6fce6b446c166ac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:09:22.430915Z","signature_b64":"6kIuJ5nTXulsa2aPkaqfESamI9kq5PoXWRi29V0Aujc5DMLLHvbdEq3EfvY2/SSxDDL3ipslD4kPku6ArZAjBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"294931f55574c0d877d10e6acda33eded03b355fae27a6f09290b45bff7bb77c","last_reissued_at":"2026-07-05T09:09:22.430421Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:09:22.430421Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermodynamics and kinetics of state switching for the asymptotically flat black hole in a cavity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.stat-mech","hep-th"],"primary_cat":"gr-qc","authors_text":"Jin Wang, Ran Li","submitted_at":"2024-05-15T07:31:15Z","abstract_excerpt":"We propose that the thermodynamics and the kinetics of state switching for the asymptotically flat black hole enclosed by a cavity can be studied in terms of the free energy landscape formalism. The generalized free energy for the black hole enclosed by a cavity in the canonical ensemble is derived by using the York's approach, where the temperature on the cavity and the charges inside the cavity are kept as the fixed parameters. By quantifying the corresponding free energy landscape, we obtain the phase diagrams for the black hole in cavity, which reveal a Hawking-Page type transition for the"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2405.09151","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/2405.09151/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":"2405.09151","created_at":"2026-07-05T09:09:22.430482+00:00"},{"alias_kind":"arxiv_version","alias_value":"2405.09151v2","created_at":"2026-07-05T09:09:22.430482+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2405.09151","created_at":"2026-07-05T09:09:22.430482+00:00"},{"alias_kind":"pith_short_12","alias_value":"FFETD5KVOTAN","created_at":"2026-07-05T09:09:22.430482+00:00"},{"alias_kind":"pith_short_16","alias_value":"FFETD5KVOTANQ56R","created_at":"2026-07-05T09:09:22.430482+00:00"},{"alias_kind":"pith_short_8","alias_value":"FFETD5KV","created_at":"2026-07-05T09:09:22.430482+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.00037","citing_title":"Topology of black hole thermodynamics: A brief review","ref_index":156,"is_internal_anchor":false},{"citing_arxiv_id":"2604.05785","citing_title":"Probabilistic Evolution of Black Hole Thermodynamic States via Fokker-Planck Equation","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633","json":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633.json","graph_json":"https://pith.science/api/pith-number/FFETD5KVOTANQ56RBZVM3IZ633/graph.json","events_json":"https://pith.science/api/pith-number/FFETD5KVOTANQ56RBZVM3IZ633/events.json","paper":"https://pith.science/paper/FFETD5KV"},"agent_actions":{"view_html":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633","download_json":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633.json","view_paper":"https://pith.science/paper/FFETD5KV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2405.09151&json=true","fetch_graph":"https://pith.science/api/pith-number/FFETD5KVOTANQ56RBZVM3IZ633/graph.json","fetch_events":"https://pith.science/api/pith-number/FFETD5KVOTANQ56RBZVM3IZ633/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633/action/storage_attestation","attest_author":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633/action/author_attestation","sign_citation":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633/action/citation_signature","submit_replication":"https://pith.science/pith/FFETD5KVOTANQ56RBZVM3IZ633/action/replication_record"}},"created_at":"2026-07-05T09:09:22.430482+00:00","updated_at":"2026-07-05T09:09:22.430482+00:00"}