{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:KYVFIOMOHABLSBER7ZYQJX76CL","short_pith_number":"pith:KYVFIOMO","schema_version":"1.0","canonical_sha256":"562a54398e3802b90491fe7104dffe12ebae448ff12947ed895309585262c7da","source":{"kind":"arxiv","id":"1804.04002","version":2},"attestation_state":"computed","paper":{"title":"The exact dynamical Chern Simons metric for a spinning black hole possesses a fourth constant of motion: A Dynamical-Systems-Based Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","math.DS"],"primary_cat":"gr-qc","authors_text":"Alejandro Cardenas-Avendano, Andres F. Gutierrez, Leonardo A. Pachon, Nicolas Yunes","submitted_at":"2018-04-09T16:36:49Z","abstract_excerpt":"The recent gravitational wave observations by the LIGO/Virgo collaboration have allowed the first tests of General Relativity in the extreme gravity regime, when comparable-mass black holes and neutron stars collide. Future space-based detectors, such as the Laser Interferometer Space Antenna, will allow tests of Einstein's theory with gravitational waves emitted when a small black hole falls into a supermassive one in an extreme mass-ratio inspiral. One particular test that is tailor-made for such inspirals is the search for chaos in extreme gravity. We here study whether chaos is present in "},"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":"1804.04002","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-04-09T16:36:49Z","cross_cats_sorted":["hep-th","math.DS"],"title_canon_sha256":"7001000e6be907ca26d036895bc83a28ed018ccb60a30f59d0f15648bd2453be","abstract_canon_sha256":"821a9b616e0a5d09f849483931072f0daaff45714d84569efdf3df35242e5108"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:11:57.006727Z","signature_b64":"MiqRj8BFnD/IGUIaWyJhOWfozZtDOwMiNNUc8vfe2+2yOVrrIF2xuF3LFwr1tjY5eZuCLxuZgGmbydjaSA1jCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"562a54398e3802b90491fe7104dffe12ebae448ff12947ed895309585262c7da","last_reissued_at":"2026-05-18T00:11:57.006112Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:11:57.006112Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The exact dynamical Chern Simons metric for a spinning black hole possesses a fourth constant of motion: A Dynamical-Systems-Based Conjecture","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th","math.DS"],"primary_cat":"gr-qc","authors_text":"Alejandro Cardenas-Avendano, Andres F. Gutierrez, Leonardo A. Pachon, Nicolas Yunes","submitted_at":"2018-04-09T16:36:49Z","abstract_excerpt":"The recent gravitational wave observations by the LIGO/Virgo collaboration have allowed the first tests of General Relativity in the extreme gravity regime, when comparable-mass black holes and neutron stars collide. Future space-based detectors, such as the Laser Interferometer Space Antenna, will allow tests of Einstein's theory with gravitational waves emitted when a small black hole falls into a supermassive one in an extreme mass-ratio inspiral. One particular test that is tailor-made for such inspirals is the search for chaos in extreme gravity. We here study whether chaos is present in "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1804.04002","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":"1804.04002","created_at":"2026-05-18T00:11:57.006197+00:00"},{"alias_kind":"arxiv_version","alias_value":"1804.04002v2","created_at":"2026-05-18T00:11:57.006197+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1804.04002","created_at":"2026-05-18T00:11:57.006197+00:00"},{"alias_kind":"pith_short_12","alias_value":"KYVFIOMOHABL","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_16","alias_value":"KYVFIOMOHABLSBER","created_at":"2026-05-18T12:32:33.847187+00:00"},{"alias_kind":"pith_short_8","alias_value":"KYVFIOMO","created_at":"2026-05-18T12:32:33.847187+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/KYVFIOMOHABLSBER7ZYQJX76CL","json":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL.json","graph_json":"https://pith.science/api/pith-number/KYVFIOMOHABLSBER7ZYQJX76CL/graph.json","events_json":"https://pith.science/api/pith-number/KYVFIOMOHABLSBER7ZYQJX76CL/events.json","paper":"https://pith.science/paper/KYVFIOMO"},"agent_actions":{"view_html":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL","download_json":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL.json","view_paper":"https://pith.science/paper/KYVFIOMO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1804.04002&json=true","fetch_graph":"https://pith.science/api/pith-number/KYVFIOMOHABLSBER7ZYQJX76CL/graph.json","fetch_events":"https://pith.science/api/pith-number/KYVFIOMOHABLSBER7ZYQJX76CL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL/action/storage_attestation","attest_author":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL/action/author_attestation","sign_citation":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL/action/citation_signature","submit_replication":"https://pith.science/pith/KYVFIOMOHABLSBER7ZYQJX76CL/action/replication_record"}},"created_at":"2026-05-18T00:11:57.006197+00:00","updated_at":"2026-05-18T00:11:57.006197+00:00"}