{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:6D5W7WRJQLXFCQCCAPVSW346YU","short_pith_number":"pith:6D5W7WRJ","schema_version":"1.0","canonical_sha256":"f0fb6fda2982ee51404203eb2b6f9ec519c81e40fecf39122889b9678785e68f","source":{"kind":"arxiv","id":"1201.5715","version":1},"attestation_state":"computed","paper":{"title":"Approximate Waveforms for Extreme-Mass-Ratio Inspirals: The Chimera Scheme","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Carlos F. Sopuerta, Nicolas Yunes","submitted_at":"2012-01-27T08:08:05Z","abstract_excerpt":"We describe a new kludge scheme to model the dynamics of generic extreme-mass-ratio inspirals (EMRIs; stellar compact objects spiraling into a spinning supermassive black hole) and their gravitational-wave emission. The Chimera scheme is a hybrid method that combines tools from different approximation techniques in General Relativity: (i) A multipolar, post-Minkowskian expansion for the far-zone metric perturbation (the gravitational waveforms) and for the local prescription of the self-force; (ii) a post-Newtonian expansion for the computation of the multipole moments in terms of the trajecto"},"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":"1201.5715","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-01-27T08:08:05Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"dca2a01a99f430b6e2838a2746d2ae09a9adc029e6c73193c84b1c2a4e50c740","abstract_canon_sha256":"c12d0b1d4ac517cedf7ebe5fbcb05c5c1a1e34fafb2a2480a0246bd196d02841"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:40.996805Z","signature_b64":"QxXBM3a7Hx4uG2fp6GDkpx8+zndSaKO0p8KWRhyv3WoOHenJnUN7NSQQQ8rRGv4vjgpZOx9OIOG9SuD8S2xQBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f0fb6fda2982ee51404203eb2b6f9ec519c81e40fecf39122889b9678785e68f","last_reissued_at":"2026-05-18T01:58:40.996159Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:40.996159Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Approximate Waveforms for Extreme-Mass-Ratio Inspirals: The Chimera Scheme","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Carlos F. Sopuerta, Nicolas Yunes","submitted_at":"2012-01-27T08:08:05Z","abstract_excerpt":"We describe a new kludge scheme to model the dynamics of generic extreme-mass-ratio inspirals (EMRIs; stellar compact objects spiraling into a spinning supermassive black hole) and their gravitational-wave emission. The Chimera scheme is a hybrid method that combines tools from different approximation techniques in General Relativity: (i) A multipolar, post-Minkowskian expansion for the far-zone metric perturbation (the gravitational waveforms) and for the local prescription of the self-force; (ii) a post-Newtonian expansion for the computation of the multipole moments in terms of the trajecto"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.5715","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":""},"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":"1201.5715","created_at":"2026-05-18T01:58:40.996258+00:00"},{"alias_kind":"arxiv_version","alias_value":"1201.5715v1","created_at":"2026-05-18T01:58:40.996258+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.5715","created_at":"2026-05-18T01:58:40.996258+00:00"},{"alias_kind":"pith_short_12","alias_value":"6D5W7WRJQLXF","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"6D5W7WRJQLXFCQCC","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"6D5W7WRJ","created_at":"2026-05-18T12:26:56.085431+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.06053","citing_title":"Probing Kerr Symmetry Breaking with LISA Extreme-Mass-Ratio Inspirals","ref_index":134,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU","json":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU.json","graph_json":"https://pith.science/api/pith-number/6D5W7WRJQLXFCQCCAPVSW346YU/graph.json","events_json":"https://pith.science/api/pith-number/6D5W7WRJQLXFCQCCAPVSW346YU/events.json","paper":"https://pith.science/paper/6D5W7WRJ"},"agent_actions":{"view_html":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU","download_json":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU.json","view_paper":"https://pith.science/paper/6D5W7WRJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1201.5715&json=true","fetch_graph":"https://pith.science/api/pith-number/6D5W7WRJQLXFCQCCAPVSW346YU/graph.json","fetch_events":"https://pith.science/api/pith-number/6D5W7WRJQLXFCQCCAPVSW346YU/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU/action/storage_attestation","attest_author":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU/action/author_attestation","sign_citation":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU/action/citation_signature","submit_replication":"https://pith.science/pith/6D5W7WRJQLXFCQCCAPVSW346YU/action/replication_record"}},"created_at":"2026-05-18T01:58:40.996258+00:00","updated_at":"2026-05-18T01:58:40.996258+00:00"}