{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:W3HQOFB5J4DMUHTAPX2ZQOI334","short_pith_number":"pith:W3HQOFB5","schema_version":"1.0","canonical_sha256":"b6cf07143d4f06ca1e607df598391bdf102f5a1e5e875ae9bae430f1215b564c","source":{"kind":"arxiv","id":"2311.12423","version":1},"attestation_state":"computed","paper":{"title":"Constraints on Hairy Kerr black hole with quasi-periodic oscillations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Cheng Liu, Haiguang Xu, Hoongwah Siew, Qiang Wu, Tao Zhu, Yuanyuan Zhao","submitted_at":"2023-11-21T08:27:34Z","abstract_excerpt":"The Hairy Kerr black hole is a novel black hole solution that depicts a rotating space-time encompassed by an axisymmetric fluid. It has significant observational importance and is an excellent candidate for an astrophysical black hole. Our study investigates the impact of the hairy charge on the quasi-periodic oscillations (QPOs) of X-ray binaries in the Hairy Kerr black hole (HKBH) space-time. The relativistic precession model is employed to compute the three principal frequencies of the accretion disk encircling the HKBH. We compare our outcomes with the observations of five X-ray binaries "},"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":"2311.12423","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-11-21T08:27:34Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"58abb19f0921baa386487145c3834388908a1a9b04ae1af6b400083dbfb3f2c4","abstract_canon_sha256":"e350b115d4b1f6386c9d3fbff3e4d29d80c03731c93db659620f5b2dbc9bccd2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:15:05.232486Z","signature_b64":"9h3krwkGGUEEks/2C5Cw/vA/AvwrYainzct90MoiWSw5aMwF4bxeJQlzTehx2S28ul42rLCvgzyz/QaY+U/IBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b6cf07143d4f06ca1e607df598391bdf102f5a1e5e875ae9bae430f1215b564c","last_reissued_at":"2026-07-05T07:15:05.232002Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:15:05.232002Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraints on Hairy Kerr black hole with quasi-periodic oscillations","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Cheng Liu, Haiguang Xu, Hoongwah Siew, Qiang Wu, Tao Zhu, Yuanyuan Zhao","submitted_at":"2023-11-21T08:27:34Z","abstract_excerpt":"The Hairy Kerr black hole is a novel black hole solution that depicts a rotating space-time encompassed by an axisymmetric fluid. It has significant observational importance and is an excellent candidate for an astrophysical black hole. Our study investigates the impact of the hairy charge on the quasi-periodic oscillations (QPOs) of X-ray binaries in the Hairy Kerr black hole (HKBH) space-time. The relativistic precession model is employed to compute the three principal frequencies of the accretion disk encircling the HKBH. We compare our outcomes with the observations of five X-ray binaries "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.12423","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/2311.12423/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":"2311.12423","created_at":"2026-07-05T07:15:05.232059+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.12423v1","created_at":"2026-07-05T07:15:05.232059+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.12423","created_at":"2026-07-05T07:15:05.232059+00:00"},{"alias_kind":"pith_short_12","alias_value":"W3HQOFB5J4DM","created_at":"2026-07-05T07:15:05.232059+00:00"},{"alias_kind":"pith_short_16","alias_value":"W3HQOFB5J4DMUHTA","created_at":"2026-07-05T07:15:05.232059+00:00"},{"alias_kind":"pith_short_8","alias_value":"W3HQOFB5","created_at":"2026-07-05T07:15:05.232059+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2601.02904","citing_title":"Probing the nature of Einstein nonlinear Maxwell Yukawa black hole through gravitational wave forms from periodic orbits and quasiperiodic oscillations","ref_index":25,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334","json":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334.json","graph_json":"https://pith.science/api/pith-number/W3HQOFB5J4DMUHTAPX2ZQOI334/graph.json","events_json":"https://pith.science/api/pith-number/W3HQOFB5J4DMUHTAPX2ZQOI334/events.json","paper":"https://pith.science/paper/W3HQOFB5"},"agent_actions":{"view_html":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334","download_json":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334.json","view_paper":"https://pith.science/paper/W3HQOFB5","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.12423&json=true","fetch_graph":"https://pith.science/api/pith-number/W3HQOFB5J4DMUHTAPX2ZQOI334/graph.json","fetch_events":"https://pith.science/api/pith-number/W3HQOFB5J4DMUHTAPX2ZQOI334/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334/action/timestamp_anchor","attest_storage":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334/action/storage_attestation","attest_author":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334/action/author_attestation","sign_citation":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334/action/citation_signature","submit_replication":"https://pith.science/pith/W3HQOFB5J4DMUHTAPX2ZQOI334/action/replication_record"}},"created_at":"2026-07-05T07:15:05.232059+00:00","updated_at":"2026-07-05T07:15:05.232059+00:00"}