{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:K5G4CSP7HYJJFPSGKLJHHCW3QU","short_pith_number":"pith:K5G4CSP7","schema_version":"1.0","canonical_sha256":"574dc149ff3e1292be4652d2738adb851c39a6c27b2358d8c81e4575901e7fac","source":{"kind":"arxiv","id":"2312.14451","version":3},"attestation_state":"computed","paper":{"title":"Special $N$-dimensional charged anti-de-Sitter black holes in $f(\\mathbb{Q})$ gravitational theory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"G.G.L. Nashed","submitted_at":"2023-12-22T05:54:28Z","abstract_excerpt":"Due to the absence of spherically symmetric black hole solutions in $f(\\mathbb{Q})$ because of the constraint derived from its field equations, which yields either $\\mathbb{Q}=0 $ or $f_{\\mathbb{Q} \\mathbb{Q}}=0 $ \\cite{Heisenberg:2023lru,Maurya:2023muz}. We are going to introduce a tours solutions for charged anti-de-Sitter black holes in $N$-dimensions within the framework of the quadratic form of $f(\\mathbb{Q})$ gravity, where the coincident gauge condition is applied \\cite{Heisenberg:2023lru}. Here, $f(\\mathbb{Q})=\\mathbb{Q}+\\frac{1}2\\alpha \\mathbb{Q}^2-2\\Lambda$, and the condition $N \\geq"},"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":"2312.14451","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-12-22T05:54:28Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"7512f72b0adabda91d660c1961b7c4588797790935b06cea71e4a901c5a475af","abstract_canon_sha256":"61a3b2c47dd826c352708d9156becc6e4e4ee77293b78f1f4892c7a4ce10ae51"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:01:31.792722Z","signature_b64":"K/HSWAniXSsrUH108V3PxOuh9WqP4zd4yIFYOsEW+U+qGNN4iNoaSPz3gsI6fvg0zdrOiuTkEfHJH/YfM20PDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"574dc149ff3e1292be4652d2738adb851c39a6c27b2358d8c81e4575901e7fac","last_reissued_at":"2026-07-05T10:01:31.792306Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:01:31.792306Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Special $N$-dimensional charged anti-de-Sitter black holes in $f(\\mathbb{Q})$ gravitational theory","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"G.G.L. Nashed","submitted_at":"2023-12-22T05:54:28Z","abstract_excerpt":"Due to the absence of spherically symmetric black hole solutions in $f(\\mathbb{Q})$ because of the constraint derived from its field equations, which yields either $\\mathbb{Q}=0 $ or $f_{\\mathbb{Q} \\mathbb{Q}}=0 $ \\cite{Heisenberg:2023lru,Maurya:2023muz}. We are going to introduce a tours solutions for charged anti-de-Sitter black holes in $N$-dimensions within the framework of the quadratic form of $f(\\mathbb{Q})$ gravity, where the coincident gauge condition is applied \\cite{Heisenberg:2023lru}. Here, $f(\\mathbb{Q})=\\mathbb{Q}+\\frac{1}2\\alpha \\mathbb{Q}^2-2\\Lambda$, and the condition $N \\geq"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2312.14451","kind":"arxiv","version":3},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2312.14451/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"2312.14451","created_at":"2026-07-05T10:01:31.792379+00:00"},{"alias_kind":"arxiv_version","alias_value":"2312.14451v3","created_at":"2026-07-05T10:01:31.792379+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2312.14451","created_at":"2026-07-05T10:01:31.792379+00:00"},{"alias_kind":"pith_short_12","alias_value":"K5G4CSP7HYJJ","created_at":"2026-07-05T10:01:31.792379+00:00"},{"alias_kind":"pith_short_16","alias_value":"K5G4CSP7HYJJFPSG","created_at":"2026-07-05T10:01:31.792379+00:00"},{"alias_kind":"pith_short_8","alias_value":"K5G4CSP7","created_at":"2026-07-05T10:01:31.792379+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.09373","citing_title":"Maxwell-$f(Q)$ theory","ref_index":65,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU","json":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU.json","graph_json":"https://pith.science/api/pith-number/K5G4CSP7HYJJFPSGKLJHHCW3QU/graph.json","events_json":"https://pith.science/api/pith-number/K5G4CSP7HYJJFPSGKLJHHCW3QU/events.json","paper":"https://pith.science/paper/K5G4CSP7"},"agent_actions":{"view_html":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU","download_json":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU.json","view_paper":"https://pith.science/paper/K5G4CSP7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2312.14451&json=true","fetch_graph":"https://pith.science/api/pith-number/K5G4CSP7HYJJFPSGKLJHHCW3QU/graph.json","fetch_events":"https://pith.science/api/pith-number/K5G4CSP7HYJJFPSGKLJHHCW3QU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU/action/storage_attestation","attest_author":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU/action/author_attestation","sign_citation":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU/action/citation_signature","submit_replication":"https://pith.science/pith/K5G4CSP7HYJJFPSGKLJHHCW3QU/action/replication_record"}},"created_at":"2026-07-05T10:01:31.792379+00:00","updated_at":"2026-07-05T10:01:31.792379+00:00"}