{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:UVTFAM3OIRLTM6REGEJNB2MKKX","short_pith_number":"pith:UVTFAM3O","schema_version":"1.0","canonical_sha256":"a56650336e4457367a243112d0e98a55f7e7979304e576f02356b39511c4ded8","source":{"kind":"arxiv","id":"2311.13839","version":1},"attestation_state":"computed","paper":{"title":"Circular orbits and accretion disk around AdS black holes surrounded by dark fluid with Chaplygin-like equation of state","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. Ditta, Farruh Atamurotov, G. Mustafa, Saibal Ray, S. K. Maurya","submitted_at":"2023-11-23T07:53:35Z","abstract_excerpt":"In the present work we study the geodesic motion and accretion process of a test particle near an Anti-de Sitter (ADS) BH surrounded by a dark fluid with a Chaplygin-like equation. Within the defined paradigm, we investigate on the equatorial plane and examine circular geodesics along with their features related to stabilities, radiation energy flux, oscillations and orbits. The general form of the fluid accretion onto the AdS BH through dynamical analysis and mass expansion also has discussed in a depth. Additionally, a few more interesting topics, e.g. the effective potential, angular moment"},"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":"2311.13839","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-11-23T07:53:35Z","cross_cats_sorted":[],"title_canon_sha256":"b7c89f8fc6d148bccc7c373ffe36ab30dc57b0d5fb6a4f47bb169904b55bfd23","abstract_canon_sha256":"8c9670051741e8eb89260671d11a414e68cd46b4f7a8133be6b5724bb65e063c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:16:08.757179Z","signature_b64":"d5XHVzYmvX7V4uC9LqAh2gaiaVpT6vuR+aVl1dnTMXKz6Gb3FvTzDe0ilx4orXOhsCV8NUQxNPb90JNE63SSBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a56650336e4457367a243112d0e98a55f7e7979304e576f02356b39511c4ded8","last_reissued_at":"2026-07-05T07:16:08.756746Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:16:08.756746Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Circular orbits and accretion disk around AdS black holes surrounded by dark fluid with Chaplygin-like equation of state","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. Ditta, Farruh Atamurotov, G. Mustafa, Saibal Ray, S. K. Maurya","submitted_at":"2023-11-23T07:53:35Z","abstract_excerpt":"In the present work we study the geodesic motion and accretion process of a test particle near an Anti-de Sitter (ADS) BH surrounded by a dark fluid with a Chaplygin-like equation. Within the defined paradigm, we investigate on the equatorial plane and examine circular geodesics along with their features related to stabilities, radiation energy flux, oscillations and orbits. The general form of the fluid accretion onto the AdS BH through dynamical analysis and mass expansion also has discussed in a depth. Additionally, a few more interesting topics, e.g. the effective potential, angular moment"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.13839","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/2311.13839/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":"2311.13839","created_at":"2026-07-05T07:16:08.756812+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.13839v1","created_at":"2026-07-05T07:16:08.756812+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.13839","created_at":"2026-07-05T07:16:08.756812+00:00"},{"alias_kind":"pith_short_12","alias_value":"UVTFAM3OIRLT","created_at":"2026-07-05T07:16:08.756812+00:00"},{"alias_kind":"pith_short_16","alias_value":"UVTFAM3OIRLTM6RE","created_at":"2026-07-05T07:16:08.756812+00:00"},{"alias_kind":"pith_short_8","alias_value":"UVTFAM3O","created_at":"2026-07-05T07:16:08.756812+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.27242","citing_title":"Strong-lensing degeneracies of black holes embedded in self-interacting scalar field dark matter halos","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX","json":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX.json","graph_json":"https://pith.science/api/pith-number/UVTFAM3OIRLTM6REGEJNB2MKKX/graph.json","events_json":"https://pith.science/api/pith-number/UVTFAM3OIRLTM6REGEJNB2MKKX/events.json","paper":"https://pith.science/paper/UVTFAM3O"},"agent_actions":{"view_html":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX","download_json":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX.json","view_paper":"https://pith.science/paper/UVTFAM3O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.13839&json=true","fetch_graph":"https://pith.science/api/pith-number/UVTFAM3OIRLTM6REGEJNB2MKKX/graph.json","fetch_events":"https://pith.science/api/pith-number/UVTFAM3OIRLTM6REGEJNB2MKKX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX/action/storage_attestation","attest_author":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX/action/author_attestation","sign_citation":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX/action/citation_signature","submit_replication":"https://pith.science/pith/UVTFAM3OIRLTM6REGEJNB2MKKX/action/replication_record"}},"created_at":"2026-07-05T07:16:08.756812+00:00","updated_at":"2026-07-05T07:16:08.756812+00:00"}