{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:GVXDUD3NAYEI6YYHGDB6C42HQW","short_pith_number":"pith:GVXDUD3N","schema_version":"1.0","canonical_sha256":"356e3a0f6d06088f630730c3e1734785a0738c65e0f2b268323ecc4315d42e24","source":{"kind":"arxiv","id":"2411.06188","version":2},"attestation_state":"computed","paper":{"title":"The thermodynamic profile of AdS black holes in Lorentz-violating Bumblebee and Kalb-Ramond gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Syed Masood","submitted_at":"2024-11-09T14:01:15Z","abstract_excerpt":"Lorentz invariance violation (LIV) is a topic of significant interest in quantum gravity and in extensions of the Standard Model of particle physics. Recently, new classes of black hole solutions have been proposed, involving vector fields and rank-two antisymmetric tensor fields that acquire nontrivial vacuum expectation values, resulting in the Bumblebee and Kalb-Ramond (KR) gravity models, respectively. These models exhibit novel geometric structures and differ in notable ways from standard Einstein gravity. In this study, we examine neutral anti-de Sitter (AdS) black holes within the conte"},"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":"2411.06188","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-11-09T14:01:15Z","cross_cats_sorted":[],"title_canon_sha256":"9a442739980e41c83f40b5496ad0f55a2fa98919075f04115fc2eb6006f71f5a","abstract_canon_sha256":"dbfb3e97105b4a8af5824429e9145a9fcc0a79e0e460abd2dda1d55914d60d96"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:14:50.542809Z","signature_b64":"XwtBAlw/SpbuaTDqQz1dnaEm4rFDFcfLvQG2v+tUp3AiBIzibBflNai1gK0hilwlu4B5VK/Z9tGyb3Ojmi7XAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"356e3a0f6d06088f630730c3e1734785a0738c65e0f2b268323ecc4315d42e24","last_reissued_at":"2026-07-05T11:14:50.542336Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:14:50.542336Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The thermodynamic profile of AdS black holes in Lorentz-violating Bumblebee and Kalb-Ramond gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Syed Masood","submitted_at":"2024-11-09T14:01:15Z","abstract_excerpt":"Lorentz invariance violation (LIV) is a topic of significant interest in quantum gravity and in extensions of the Standard Model of particle physics. Recently, new classes of black hole solutions have been proposed, involving vector fields and rank-two antisymmetric tensor fields that acquire nontrivial vacuum expectation values, resulting in the Bumblebee and Kalb-Ramond (KR) gravity models, respectively. These models exhibit novel geometric structures and differ in notable ways from standard Einstein gravity. In this study, we examine neutral anti-de Sitter (AdS) black holes within the conte"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2411.06188","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/2411.06188/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":"2411.06188","created_at":"2026-07-05T11:14:50.542387+00:00"},{"alias_kind":"arxiv_version","alias_value":"2411.06188v2","created_at":"2026-07-05T11:14:50.542387+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2411.06188","created_at":"2026-07-05T11:14:50.542387+00:00"},{"alias_kind":"pith_short_12","alias_value":"GVXDUD3NAYEI","created_at":"2026-07-05T11:14:50.542387+00:00"},{"alias_kind":"pith_short_16","alias_value":"GVXDUD3NAYEI6YYH","created_at":"2026-07-05T11:14:50.542387+00:00"},{"alias_kind":"pith_short_8","alias_value":"GVXDUD3N","created_at":"2026-07-05T11:14:50.542387+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.17947","citing_title":"Charged black holes in Kalb-Ramond gravity: Weak Deflection Angle, Shadow cast, Quasinormal Modes and Neutrino annihilation","ref_index":27,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW","json":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW.json","graph_json":"https://pith.science/api/pith-number/GVXDUD3NAYEI6YYHGDB6C42HQW/graph.json","events_json":"https://pith.science/api/pith-number/GVXDUD3NAYEI6YYHGDB6C42HQW/events.json","paper":"https://pith.science/paper/GVXDUD3N"},"agent_actions":{"view_html":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW","download_json":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW.json","view_paper":"https://pith.science/paper/GVXDUD3N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2411.06188&json=true","fetch_graph":"https://pith.science/api/pith-number/GVXDUD3NAYEI6YYHGDB6C42HQW/graph.json","fetch_events":"https://pith.science/api/pith-number/GVXDUD3NAYEI6YYHGDB6C42HQW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW/action/storage_attestation","attest_author":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW/action/author_attestation","sign_citation":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW/action/citation_signature","submit_replication":"https://pith.science/pith/GVXDUD3NAYEI6YYHGDB6C42HQW/action/replication_record"}},"created_at":"2026-07-05T11:14:50.542387+00:00","updated_at":"2026-07-05T11:14:50.542387+00:00"}