{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:EO37W5GYFZZL6O3G355CRCID2K","short_pith_number":"pith:EO37W5GY","schema_version":"1.0","canonical_sha256":"23b7fb74d82e72bf3b66df7a288903d2b204d585b0ded5c4bafd6967f68eb2d2","source":{"kind":"arxiv","id":"2307.02030","version":3},"attestation_state":"computed","paper":{"title":"Topological classes of thermodynamics of the four-dimensional static accelerating black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Di Wu","submitted_at":"2023-07-05T05:27:53Z","abstract_excerpt":"In this paper, utilizing the generalized off shell Helmholtz free energy, we explore the topological numbers of the four-dimensional static accelerating black hole and its AdS extension, as well as the static charged accelerating black hole and its AdS extension. Our analysis reveals a profound and significant impact of the acceleration parameter on the topological numbers associated with the static black holes; and different values (nonzero) of the acceleration parameter do not affect the topological numbers of the corresponding four-dimensional static accelerating black holes. In addition, w"},"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":"2307.02030","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2023-07-05T05:27:53Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"e4f6931cb3b7ac3e99953e44c2a15f9d7637704d597dcf5f1b7712aaada7ac56","abstract_canon_sha256":"d971b2976e2418f73cbeca52300a185f352997a27e7eb329b11eb812d8f55954"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:03:28.819460Z","signature_b64":"Eu5g/CLOF81JUgxGs/y36Gy3do1M/ilcXyg4jcBRiyUixZ9LY57/wQIy3yi28Flq+76jW3TH66wKeqTZ3E6VDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"23b7fb74d82e72bf3b66df7a288903d2b204d585b0ded5c4bafd6967f68eb2d2","last_reissued_at":"2026-07-05T07:03:28.818944Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:03:28.818944Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Topological classes of thermodynamics of the four-dimensional static accelerating black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Di Wu","submitted_at":"2023-07-05T05:27:53Z","abstract_excerpt":"In this paper, utilizing the generalized off shell Helmholtz free energy, we explore the topological numbers of the four-dimensional static accelerating black hole and its AdS extension, as well as the static charged accelerating black hole and its AdS extension. Our analysis reveals a profound and significant impact of the acceleration parameter on the topological numbers associated with the static black holes; and different values (nonzero) of the acceleration parameter do not affect the topological numbers of the corresponding four-dimensional static accelerating black holes. In addition, w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.02030","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/2307.02030/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":"2307.02030","created_at":"2026-07-05T07:03:28.819003+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.02030v3","created_at":"2026-07-05T07:03:28.819003+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.02030","created_at":"2026-07-05T07:03:28.819003+00:00"},{"alias_kind":"pith_short_12","alias_value":"EO37W5GYFZZL","created_at":"2026-07-05T07:03:28.819003+00:00"},{"alias_kind":"pith_short_16","alias_value":"EO37W5GYFZZL6O3G","created_at":"2026-07-05T07:03:28.819003+00:00"},{"alias_kind":"pith_short_8","alias_value":"EO37W5GY","created_at":"2026-07-05T07:03:28.819003+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.03958","citing_title":"Multihair thermodynamics of Kerr-Newman-NUT-AdS$_4$ spacetimes","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00037","citing_title":"Topology of black hole thermodynamics: A brief review","ref_index":63,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K","json":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K.json","graph_json":"https://pith.science/api/pith-number/EO37W5GYFZZL6O3G355CRCID2K/graph.json","events_json":"https://pith.science/api/pith-number/EO37W5GYFZZL6O3G355CRCID2K/events.json","paper":"https://pith.science/paper/EO37W5GY"},"agent_actions":{"view_html":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K","download_json":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K.json","view_paper":"https://pith.science/paper/EO37W5GY","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.02030&json=true","fetch_graph":"https://pith.science/api/pith-number/EO37W5GYFZZL6O3G355CRCID2K/graph.json","fetch_events":"https://pith.science/api/pith-number/EO37W5GYFZZL6O3G355CRCID2K/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K/action/storage_attestation","attest_author":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K/action/author_attestation","sign_citation":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K/action/citation_signature","submit_replication":"https://pith.science/pith/EO37W5GYFZZL6O3G355CRCID2K/action/replication_record"}},"created_at":"2026-07-05T07:03:28.819003+00:00","updated_at":"2026-07-05T07:03:28.819003+00:00"}