{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:MAO4S4XPDWWEWYLENCU6MB724W","short_pith_number":"pith:MAO4S4XP","schema_version":"1.0","canonical_sha256":"601dc972ef1dac4b616468a9e607fae590918cea6b4f191230307ceb670efe8e","source":{"kind":"arxiv","id":"2307.11611","version":1},"attestation_state":"computed","paper":{"title":"Rotating Kiselev Black Holes in $f(R,T)$ Gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Shafqat Ul Islam, Sunil D. Maharaj, Sushant G. Ghosh","submitted_at":"2023-07-21T14:31:33Z","abstract_excerpt":"Exact solutions describing rotating black holes can provide significant opportunities for testing modified theories of gravity, which are motivated by the challenges posed by dark energy and dark matter. Starting with a spherical Kiselev black hole as a seed metric, we construct rotating Kiselev black holes within the $f(R,T)$ gravity framework using the revised Newman-Janis algorithm - the $f(R,T)$ gravity-motivated rotating Kiselev black holes (FRKBH), which encompasses, as exceptional cases, Kerr ($K=0$) and Kerr-Newman ($K=Q^2$) black holes. These solutions give rise to distinct classes of"},"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":"2307.11611","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-07-21T14:31:33Z","cross_cats_sorted":[],"title_canon_sha256":"631bc9744bca8094fff663f775ed525846d75336c5c33044c4a002bdd2b9cc86","abstract_canon_sha256":"5318500bfe4e4a54fb0e16c05d75cb730d495c7b9c2efd052e9245235a456d82"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:33:30.005923Z","signature_b64":"XsW1xNZeu9GQeUO44hjM5gxEM0U+RTUs+4ChnFZvow9Z8c4YlaY1IxVPko+5APLADTz0osyCFcL5b50DGfvkCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"601dc972ef1dac4b616468a9e607fae590918cea6b4f191230307ceb670efe8e","last_reissued_at":"2026-07-05T06:33:30.005483Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:33:30.005483Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Rotating Kiselev Black Holes in $f(R,T)$ Gravity","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Shafqat Ul Islam, Sunil D. Maharaj, Sushant G. Ghosh","submitted_at":"2023-07-21T14:31:33Z","abstract_excerpt":"Exact solutions describing rotating black holes can provide significant opportunities for testing modified theories of gravity, which are motivated by the challenges posed by dark energy and dark matter. Starting with a spherical Kiselev black hole as a seed metric, we construct rotating Kiselev black holes within the $f(R,T)$ gravity framework using the revised Newman-Janis algorithm - the $f(R,T)$ gravity-motivated rotating Kiselev black holes (FRKBH), which encompasses, as exceptional cases, Kerr ($K=0$) and Kerr-Newman ($K=Q^2$) black holes. These solutions give rise to distinct classes of"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.11611","kind":"arxiv","version":1},"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/2307.11611/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":"2307.11611","created_at":"2026-07-05T06:33:30.005550+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.11611v1","created_at":"2026-07-05T06:33:30.005550+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.11611","created_at":"2026-07-05T06:33:30.005550+00:00"},{"alias_kind":"pith_short_12","alias_value":"MAO4S4XPDWWE","created_at":"2026-07-05T06:33:30.005550+00:00"},{"alias_kind":"pith_short_16","alias_value":"MAO4S4XPDWWEWYLE","created_at":"2026-07-05T06:33:30.005550+00:00"},{"alias_kind":"pith_short_8","alias_value":"MAO4S4XP","created_at":"2026-07-05T06:33:30.005550+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2505.07028","citing_title":"Traversable wormholes from a smoothed string fluid in 4D Einstein-Gauss-Bonnet gravity","ref_index":50,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W","json":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W.json","graph_json":"https://pith.science/api/pith-number/MAO4S4XPDWWEWYLENCU6MB724W/graph.json","events_json":"https://pith.science/api/pith-number/MAO4S4XPDWWEWYLENCU6MB724W/events.json","paper":"https://pith.science/paper/MAO4S4XP"},"agent_actions":{"view_html":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W","download_json":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W.json","view_paper":"https://pith.science/paper/MAO4S4XP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.11611&json=true","fetch_graph":"https://pith.science/api/pith-number/MAO4S4XPDWWEWYLENCU6MB724W/graph.json","fetch_events":"https://pith.science/api/pith-number/MAO4S4XPDWWEWYLENCU6MB724W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W/action/storage_attestation","attest_author":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W/action/author_attestation","sign_citation":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W/action/citation_signature","submit_replication":"https://pith.science/pith/MAO4S4XPDWWEWYLENCU6MB724W/action/replication_record"}},"created_at":"2026-07-05T06:33:30.005550+00:00","updated_at":"2026-07-05T06:33:30.005550+00:00"}