{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:UVEZU2I27LV2INGYYBUD5OSHVV","short_pith_number":"pith:UVEZU2I2","schema_version":"1.0","canonical_sha256":"a5499a691afaeba434d8c0683eba47ad512f8c2ea929f380f1f5bed12aa905a2","source":{"kind":"arxiv","id":"2412.15332","version":1},"attestation_state":"computed","paper":{"title":"Non-equatorial scalar rings supported by rapidly spinning Gauss-Bonnet black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Shahar Hod","submitted_at":"2024-12-19T19:00:07Z","abstract_excerpt":"Black-hole spacetimes that possess stationary equatorial matter rings are known to exist in general relativity. We here reveal the existence of black-hole spacetimes that support {\\it non}-equatorial matter rings. In particular, it is proved that rapidly-rotating Kerr black holes in the dimensionless large-spin regime ${\\bar a}>{\\bar a}_{\\text{crit}}= \\sqrt{\\big\\{{{7+\\sqrt{7}\\cos\\big[{1\\over3}\\arctan\\big(3\\sqrt{3}\\big)\\big]- \\sqrt{21}\\sin\\big[{1\\over3}\\arctan\\big(3\\sqrt{3}\\big)\\big]}\\big\\}/12}}\\simeq0.78$ can support a pair of non-equatorial massive scalar rings which are negatively coupled to"},"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":"2412.15332","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"gr-qc","submitted_at":"2024-12-19T19:00:07Z","cross_cats_sorted":["astro-ph.HE","hep-th"],"title_canon_sha256":"4ab45c657697c28054384226caa8c3e679f61ae832158f5278746c66609a9a0a","abstract_canon_sha256":"570658946f2dfd40dec52b0ccfef6886d25a55813008c82eb2f50c39a3a4a188"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:52:21.448243Z","signature_b64":"8YuiRLNHCEzZJr38IUcDd2m+C3BAKLHlkmgRhshDXeT2AViQ/ip60YHn7vxmFJ6xEgOqF9s9sv8sU8B6Y9sgAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a5499a691afaeba434d8c0683eba47ad512f8c2ea929f380f1f5bed12aa905a2","last_reissued_at":"2026-07-05T09:52:21.447772Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:52:21.447772Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-equatorial scalar rings supported by rapidly spinning Gauss-Bonnet black holes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","hep-th"],"primary_cat":"gr-qc","authors_text":"Shahar Hod","submitted_at":"2024-12-19T19:00:07Z","abstract_excerpt":"Black-hole spacetimes that possess stationary equatorial matter rings are known to exist in general relativity. We here reveal the existence of black-hole spacetimes that support {\\it non}-equatorial matter rings. In particular, it is proved that rapidly-rotating Kerr black holes in the dimensionless large-spin regime ${\\bar a}>{\\bar a}_{\\text{crit}}= \\sqrt{\\big\\{{{7+\\sqrt{7}\\cos\\big[{1\\over3}\\arctan\\big(3\\sqrt{3}\\big)\\big]- \\sqrt{21}\\sin\\big[{1\\over3}\\arctan\\big(3\\sqrt{3}\\big)\\big]}\\big\\}/12}}\\simeq0.78$ can support a pair of non-equatorial massive scalar rings which are negatively coupled to"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.15332","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/2412.15332/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":"2412.15332","created_at":"2026-07-05T09:52:21.447831+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.15332v1","created_at":"2026-07-05T09:52:21.447831+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.15332","created_at":"2026-07-05T09:52:21.447831+00:00"},{"alias_kind":"pith_short_12","alias_value":"UVEZU2I27LV2","created_at":"2026-07-05T09:52:21.447831+00:00"},{"alias_kind":"pith_short_16","alias_value":"UVEZU2I27LV2INGY","created_at":"2026-07-05T09:52:21.447831+00:00"},{"alias_kind":"pith_short_8","alias_value":"UVEZU2I2","created_at":"2026-07-05T09:52:21.447831+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/UVEZU2I27LV2INGYYBUD5OSHVV","json":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV.json","graph_json":"https://pith.science/api/pith-number/UVEZU2I27LV2INGYYBUD5OSHVV/graph.json","events_json":"https://pith.science/api/pith-number/UVEZU2I27LV2INGYYBUD5OSHVV/events.json","paper":"https://pith.science/paper/UVEZU2I2"},"agent_actions":{"view_html":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV","download_json":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV.json","view_paper":"https://pith.science/paper/UVEZU2I2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.15332&json=true","fetch_graph":"https://pith.science/api/pith-number/UVEZU2I27LV2INGYYBUD5OSHVV/graph.json","fetch_events":"https://pith.science/api/pith-number/UVEZU2I27LV2INGYYBUD5OSHVV/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV/action/timestamp_anchor","attest_storage":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV/action/storage_attestation","attest_author":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV/action/author_attestation","sign_citation":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV/action/citation_signature","submit_replication":"https://pith.science/pith/UVEZU2I27LV2INGYYBUD5OSHVV/action/replication_record"}},"created_at":"2026-07-05T09:52:21.447831+00:00","updated_at":"2026-07-05T09:52:21.447831+00:00"}