{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:YZXPP3KVB67FIFJQHXGVJKABWX","short_pith_number":"pith:YZXPP3KV","schema_version":"1.0","canonical_sha256":"c66ef7ed550fbe5415303dcd54a801b5fb811fd812c769b0582629b368333d18","source":{"kind":"arxiv","id":"2310.06033","version":1},"attestation_state":"computed","paper":{"title":"Isospectrality breaking in the Teukolsky formalism","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Aaron Zimmerman, Asad Hussain, Dongjun Li, Nicol\\'as Yunes, Pratik Wagle, Yanbei Chen","submitted_at":"2023-10-09T18:00:04Z","abstract_excerpt":"General relativity, though the most successful theory of gravity, has been continuously modified to resolve its incompatibility with quantum mechanics and explain the origin of dark energy or dark matter. One way to test these modified gravity theories is to study the gravitational waves emitted during the ringdown of binary mergers, which consist of quasinormal modes. In several modified gravity theories, the even- and odd-parity gravitational perturbations of non-rotating and slowly rotating black holes have different quasinormal mode frequencies, breaking the isospectrality of general relat"},"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":"2310.06033","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-10-09T18:00:04Z","cross_cats_sorted":[],"title_canon_sha256":"fadc73d6a129c44f57a720f8300bdc2f4464a96eef1271cd2dea657234d05da9","abstract_canon_sha256":"2d3c01b5fa68cd1852eec03a8d32203c4f8ad6954a86efa2dcbed37fe7dbe452"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:59:03.335607Z","signature_b64":"J4oQkkvVwZiDoXiW+kX+4kQA1Q7ujHY/QejbQ3r51Dr1CdFwUxXlCc8N/GwYLGsIGlHePzhmlm5XKArzhc+dBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c66ef7ed550fbe5415303dcd54a801b5fb811fd812c769b0582629b368333d18","last_reissued_at":"2026-07-05T06:59:03.335176Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:59:03.335176Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Isospectrality breaking in the Teukolsky formalism","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Aaron Zimmerman, Asad Hussain, Dongjun Li, Nicol\\'as Yunes, Pratik Wagle, Yanbei Chen","submitted_at":"2023-10-09T18:00:04Z","abstract_excerpt":"General relativity, though the most successful theory of gravity, has been continuously modified to resolve its incompatibility with quantum mechanics and explain the origin of dark energy or dark matter. One way to test these modified gravity theories is to study the gravitational waves emitted during the ringdown of binary mergers, which consist of quasinormal modes. In several modified gravity theories, the even- and odd-parity gravitational perturbations of non-rotating and slowly rotating black holes have different quasinormal mode frequencies, breaking the isospectrality of general relat"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2310.06033","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/2310.06033/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":"2310.06033","created_at":"2026-07-05T06:59:03.335241+00:00"},{"alias_kind":"arxiv_version","alias_value":"2310.06033v1","created_at":"2026-07-05T06:59:03.335241+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2310.06033","created_at":"2026-07-05T06:59:03.335241+00:00"},{"alias_kind":"pith_short_12","alias_value":"YZXPP3KVB67F","created_at":"2026-07-05T06:59:03.335241+00:00"},{"alias_kind":"pith_short_16","alias_value":"YZXPP3KVB67FIFJQ","created_at":"2026-07-05T06:59:03.335241+00:00"},{"alias_kind":"pith_short_8","alias_value":"YZXPP3KV","created_at":"2026-07-05T06:59:03.335241+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09766","citing_title":"Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity","ref_index":66,"is_internal_anchor":false},{"citing_arxiv_id":"2606.07070","citing_title":"Gravitational waveforms from binaries in higher-derivative gravity: a Love story","ref_index":17,"is_internal_anchor":false},{"citing_arxiv_id":"2605.03018","citing_title":"Gravitational electric-magnetic duality at the light ring and quasinormal mode isospectrality in effective field theories","ref_index":77,"is_internal_anchor":false},{"citing_arxiv_id":"2604.13182","citing_title":"Bilinear products and the orthogonality of quasinormal modes on hyperboloidal foliations","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02820","citing_title":"Gravitational-Bumblebee perturbations: Exact decoupling and isospectrality","ref_index":62,"is_internal_anchor":false},{"citing_arxiv_id":"2605.04147","citing_title":"Unifying the Regge-Wheeler-Zerilli and Bardeen-Press-Teukolsky formalisms on spherical backgrounds","ref_index":60,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX","json":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX.json","graph_json":"https://pith.science/api/pith-number/YZXPP3KVB67FIFJQHXGVJKABWX/graph.json","events_json":"https://pith.science/api/pith-number/YZXPP3KVB67FIFJQHXGVJKABWX/events.json","paper":"https://pith.science/paper/YZXPP3KV"},"agent_actions":{"view_html":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX","download_json":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX.json","view_paper":"https://pith.science/paper/YZXPP3KV","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2310.06033&json=true","fetch_graph":"https://pith.science/api/pith-number/YZXPP3KVB67FIFJQHXGVJKABWX/graph.json","fetch_events":"https://pith.science/api/pith-number/YZXPP3KVB67FIFJQHXGVJKABWX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX/action/storage_attestation","attest_author":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX/action/author_attestation","sign_citation":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX/action/citation_signature","submit_replication":"https://pith.science/pith/YZXPP3KVB67FIFJQHXGVJKABWX/action/replication_record"}},"created_at":"2026-07-05T06:59:03.335241+00:00","updated_at":"2026-07-05T06:59:03.335241+00:00"}