{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:FBHYO6ZSXYZPFEYFXGPOC7FLPI","short_pith_number":"pith:FBHYO6ZS","schema_version":"1.0","canonical_sha256":"284f877b32be32f29305b99ee17cab7a24708eeede16cb7a92db284ab50b1988","source":{"kind":"arxiv","id":"1808.00987","version":2},"attestation_state":"computed","paper":{"title":"An unknown branch of the total-transmission modes for the Kerr-geometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Daniel J. Vickers, Gregory B. Cook, Luke S. Annichiarico","submitted_at":"2018-08-02T18:57:17Z","abstract_excerpt":"The gravitational modes of the Kerr geometry include both quasinormal modes and total-transmission modes. Sequences of these modes are parameterized by the angular momentum of the black hole. The quasinormal and total-transmission modes are usually distinct, having mode frequencies that are different at any given value of the angular momentum. But a discrete and countably infinite subset of the left-total-transmission modes are simultaneously quasinormal modes. Most of these special modes exist along previously unknown branches of the gravitational total-transmission modes. In this paper, we g"},"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":"1808.00987","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-08-02T18:57:17Z","cross_cats_sorted":[],"title_canon_sha256":"ee9435eaf2af252ddaca2da3602bf943d48e382639bf576d9b57a61a98665206","abstract_canon_sha256":"8980afdeb22596aecc68ebf9cce95bba2e0ef3a335c4ef1565a5c92548f88ed9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:56:38.518927Z","signature_b64":"J3gm+G/oHJYSKnTajZDKBiHBbxQ1r71SiDlPWmNJC3wgwaYgAeiCUMgr2lmA/h+W7YDlF/sUBdpQxjuAUCbVDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"284f877b32be32f29305b99ee17cab7a24708eeede16cb7a92db284ab50b1988","last_reissued_at":"2026-05-17T23:56:38.518205Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:56:38.518205Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"An unknown branch of the total-transmission modes for the Kerr-geometry","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Daniel J. Vickers, Gregory B. Cook, Luke S. Annichiarico","submitted_at":"2018-08-02T18:57:17Z","abstract_excerpt":"The gravitational modes of the Kerr geometry include both quasinormal modes and total-transmission modes. Sequences of these modes are parameterized by the angular momentum of the black hole. The quasinormal and total-transmission modes are usually distinct, having mode frequencies that are different at any given value of the angular momentum. But a discrete and countably infinite subset of the left-total-transmission modes are simultaneously quasinormal modes. Most of these special modes exist along previously unknown branches of the gravitational total-transmission modes. In this paper, we g"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1808.00987","kind":"arxiv","version":2},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"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":"1808.00987","created_at":"2026-05-17T23:56:38.518339+00:00"},{"alias_kind":"arxiv_version","alias_value":"1808.00987v2","created_at":"2026-05-17T23:56:38.518339+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1808.00987","created_at":"2026-05-17T23:56:38.518339+00:00"},{"alias_kind":"pith_short_12","alias_value":"FBHYO6ZSXYZP","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_16","alias_value":"FBHYO6ZSXYZPFEYF","created_at":"2026-05-18T12:32:22.470017+00:00"},{"alias_kind":"pith_short_8","alias_value":"FBHYO6ZS","created_at":"2026-05-18T12:32:22.470017+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2605.17840","citing_title":"Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2605.17840","citing_title":"Pole Skipping, Avoided Crossing, and Resonant Excitation in Kerr Quasinormal Modes near Algebraically Special Frequencies","ref_index":16,"is_internal_anchor":true},{"citing_arxiv_id":"2505.23895","citing_title":"Black hole spectroscopy: from theory to experiment","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03730","citing_title":"Total transmission modes in draining bathtub model with vorticity","ref_index":16,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI","json":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI.json","graph_json":"https://pith.science/api/pith-number/FBHYO6ZSXYZPFEYFXGPOC7FLPI/graph.json","events_json":"https://pith.science/api/pith-number/FBHYO6ZSXYZPFEYFXGPOC7FLPI/events.json","paper":"https://pith.science/paper/FBHYO6ZS"},"agent_actions":{"view_html":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI","download_json":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI.json","view_paper":"https://pith.science/paper/FBHYO6ZS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1808.00987&json=true","fetch_graph":"https://pith.science/api/pith-number/FBHYO6ZSXYZPFEYFXGPOC7FLPI/graph.json","fetch_events":"https://pith.science/api/pith-number/FBHYO6ZSXYZPFEYFXGPOC7FLPI/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI/action/storage_attestation","attest_author":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI/action/author_attestation","sign_citation":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI/action/citation_signature","submit_replication":"https://pith.science/pith/FBHYO6ZSXYZPFEYFXGPOC7FLPI/action/replication_record"}},"created_at":"2026-05-17T23:56:38.518339+00:00","updated_at":"2026-05-17T23:56:38.518339+00:00"}