{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:L6FVVOG67A3TZRDDPG6AQIG4NP","short_pith_number":"pith:L6FVVOG6","schema_version":"1.0","canonical_sha256":"5f8b5ab8def8373cc46379bc0820dc6be74cfd7e36594b2dfbc7eca778bdf0f6","source":{"kind":"arxiv","id":"2501.01018","version":1},"attestation_state":"computed","paper":{"title":"Thin Accretion Disk Around Rotating Hairy Black Hole: Radiative Property and Optical Appearance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Xiao-Kan Guo, Zhen Li","submitted_at":"2025-01-02T02:39:31Z","abstract_excerpt":"The gravitational decoupling method systematically generates hairy modifications to the solutions in general relativity due to new gravitational sources. In view of the recent advances in astronomical observations, these hairy solutions are expected to be testable in the near-term observations. In this paper, we study the radiative property and optical appearance of the thin accretion disk around the rotating hairy black holes obtained by gravitational decoupling. We numerically compute the radiative flux, temperature, and differential luminosity of the thin accretion disk, and we also show it"},"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":"2501.01018","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2025-01-02T02:39:31Z","cross_cats_sorted":[],"title_canon_sha256":"050ba9bb186666511bd4b4c4ceb86feb541ccb8e6fce41cd5df1c8215bb1837b","abstract_canon_sha256":"014cd3f909caa0c5cac872c139c7b45372382e6be7118507e1433459f55090e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:52:16.870532Z","signature_b64":"BHsP8kubZE5/CfgJJXc3AVKRZhTma5XiXQo4neFvGf76TTTvyuTV1HrBD/hqVYdf+2JIFrmlrPWWYLsZQQBZAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"5f8b5ab8def8373cc46379bc0820dc6be74cfd7e36594b2dfbc7eca778bdf0f6","last_reissued_at":"2026-07-05T11:52:16.870066Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:52:16.870066Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thin Accretion Disk Around Rotating Hairy Black Hole: Radiative Property and Optical Appearance","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Xiao-Kan Guo, Zhen Li","submitted_at":"2025-01-02T02:39:31Z","abstract_excerpt":"The gravitational decoupling method systematically generates hairy modifications to the solutions in general relativity due to new gravitational sources. In view of the recent advances in astronomical observations, these hairy solutions are expected to be testable in the near-term observations. In this paper, we study the radiative property and optical appearance of the thin accretion disk around the rotating hairy black holes obtained by gravitational decoupling. We numerically compute the radiative flux, temperature, and differential luminosity of the thin accretion disk, and we also show it"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2501.01018","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/2501.01018/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":"2501.01018","created_at":"2026-07-05T11:52:16.870123+00:00"},{"alias_kind":"arxiv_version","alias_value":"2501.01018v1","created_at":"2026-07-05T11:52:16.870123+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2501.01018","created_at":"2026-07-05T11:52:16.870123+00:00"},{"alias_kind":"pith_short_12","alias_value":"L6FVVOG67A3T","created_at":"2026-07-05T11:52:16.870123+00:00"},{"alias_kind":"pith_short_16","alias_value":"L6FVVOG67A3TZRDD","created_at":"2026-07-05T11:52:16.870123+00:00"},{"alias_kind":"pith_short_8","alias_value":"L6FVVOG6","created_at":"2026-07-05T11:52:16.870123+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP","json":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP.json","graph_json":"https://pith.science/api/pith-number/L6FVVOG67A3TZRDDPG6AQIG4NP/graph.json","events_json":"https://pith.science/api/pith-number/L6FVVOG67A3TZRDDPG6AQIG4NP/events.json","paper":"https://pith.science/paper/L6FVVOG6"},"agent_actions":{"view_html":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP","download_json":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP.json","view_paper":"https://pith.science/paper/L6FVVOG6","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2501.01018&json=true","fetch_graph":"https://pith.science/api/pith-number/L6FVVOG67A3TZRDDPG6AQIG4NP/graph.json","fetch_events":"https://pith.science/api/pith-number/L6FVVOG67A3TZRDDPG6AQIG4NP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP/action/storage_attestation","attest_author":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP/action/author_attestation","sign_citation":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP/action/citation_signature","submit_replication":"https://pith.science/pith/L6FVVOG67A3TZRDDPG6AQIG4NP/action/replication_record"}},"created_at":"2026-07-05T11:52:16.870123+00:00","updated_at":"2026-07-05T11:52:16.870123+00:00"}