{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:U7DHDS6RBMRAYMLPFNRMDLM4P5","short_pith_number":"pith:U7DHDS6R","schema_version":"1.0","canonical_sha256":"a7c671cbd10b220c316f2b62c1ad9c7f480154e0755aa4af69bf776a04120869","source":{"kind":"arxiv","id":"2306.02881","version":1},"attestation_state":"computed","paper":{"title":"Joule-Thomson expansion and Optical behaviour of Reissner-Nordstr\\\"om-Anti-de Sitter black holes in Rastall gravity surrounded by a Quintessence field","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dhruba Jyoti Gogoi, Digbijay Kalita, Jyatsnasree Bora, Naba Jyoti Gogoi, Yassine Sekhmani","submitted_at":"2023-06-05T13:52:05Z","abstract_excerpt":"This paper deals with the thermodynamics, Joule-Thomson expansion and optical behaviour of a Reissner-Nordstr\\\"om-anti-de Sitter black hole in Rastall gravity surrounded by a quintessence field. The black hole solution obtained in this framework is different from a corresponding black hole in General Relativity. The black hole metric function, as well as the Hawking temperature, is affected by the presence of energy-momentum conservation violation. The presence of energy-momentum conservation violation also affects the isenthalpic and inversion temperature curves, and with an increase in the R"},"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":"2306.02881","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2023-06-05T13:52:05Z","cross_cats_sorted":[],"title_canon_sha256":"f8f34f4097d3a7b997c047f546eccc6fb7b949f4d9a7b3e0523c506b70be5f20","abstract_canon_sha256":"1ec5e31908e780e3894dd84b554926ce804ea4e0d19ae201af7d59a530a11196"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:17:32.421958Z","signature_b64":"kghh1Dqw+32NkjJr0R9Kc37AaNnKDhFCRnXvtKUjqngdR979VA7Juxd47KOnIxDXazyH6Mk97dTWWVpMK9+mCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a7c671cbd10b220c316f2b62c1ad9c7f480154e0755aa4af69bf776a04120869","last_reissued_at":"2026-07-05T06:17:32.421576Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:17:32.421576Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Joule-Thomson expansion and Optical behaviour of Reissner-Nordstr\\\"om-Anti-de Sitter black holes in Rastall gravity surrounded by a Quintessence field","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Dhruba Jyoti Gogoi, Digbijay Kalita, Jyatsnasree Bora, Naba Jyoti Gogoi, Yassine Sekhmani","submitted_at":"2023-06-05T13:52:05Z","abstract_excerpt":"This paper deals with the thermodynamics, Joule-Thomson expansion and optical behaviour of a Reissner-Nordstr\\\"om-anti-de Sitter black hole in Rastall gravity surrounded by a quintessence field. The black hole solution obtained in this framework is different from a corresponding black hole in General Relativity. The black hole metric function, as well as the Hawking temperature, is affected by the presence of energy-momentum conservation violation. The presence of energy-momentum conservation violation also affects the isenthalpic and inversion temperature curves, and with an increase in the R"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.02881","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/2306.02881/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":"2306.02881","created_at":"2026-07-05T06:17:32.421632+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.02881v1","created_at":"2026-07-05T06:17:32.421632+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.02881","created_at":"2026-07-05T06:17:32.421632+00:00"},{"alias_kind":"pith_short_12","alias_value":"U7DHDS6RBMRA","created_at":"2026-07-05T06:17:32.421632+00:00"},{"alias_kind":"pith_short_16","alias_value":"U7DHDS6RBMRAYMLP","created_at":"2026-07-05T06:17:32.421632+00:00"},{"alias_kind":"pith_short_8","alias_value":"U7DHDS6R","created_at":"2026-07-05T06:17:32.421632+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06704","citing_title":"Joule-Thomson Effect and Geodesic Structure of Charged AdS Black Holes in f(R,T) Coupled with Nonlinear Electrodynamics","ref_index":63,"is_internal_anchor":true},{"citing_arxiv_id":"2606.26210","citing_title":"Extended Thermodynamics and Throttling Process of Charged AdS Black Holes in ModMax-dRGT Massive Gravity with Sharma-Mittal Entropy","ref_index":15,"is_internal_anchor":false},{"citing_arxiv_id":"2605.17476","citing_title":"Joule-Thomson effect and Efficiency of deformed AdS-Schwarzschild black hole in presence of quintessence","ref_index":47,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5","json":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5.json","graph_json":"https://pith.science/api/pith-number/U7DHDS6RBMRAYMLPFNRMDLM4P5/graph.json","events_json":"https://pith.science/api/pith-number/U7DHDS6RBMRAYMLPFNRMDLM4P5/events.json","paper":"https://pith.science/paper/U7DHDS6R"},"agent_actions":{"view_html":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5","download_json":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5.json","view_paper":"https://pith.science/paper/U7DHDS6R","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.02881&json=true","fetch_graph":"https://pith.science/api/pith-number/U7DHDS6RBMRAYMLPFNRMDLM4P5/graph.json","fetch_events":"https://pith.science/api/pith-number/U7DHDS6RBMRAYMLPFNRMDLM4P5/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5/action/storage_attestation","attest_author":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5/action/author_attestation","sign_citation":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5/action/citation_signature","submit_replication":"https://pith.science/pith/U7DHDS6RBMRAYMLPFNRMDLM4P5/action/replication_record"}},"created_at":"2026-07-05T06:17:32.421632+00:00","updated_at":"2026-07-05T06:17:32.421632+00:00"}