{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:YDUUZ7YHHCIBXQFGN5KAQOCOQ3","short_pith_number":"pith:YDUUZ7YH","schema_version":"1.0","canonical_sha256":"c0e94cff0738901bc0a66f5408384e86e47cf6b625123362c3705c7dfb8ab1b5","source":{"kind":"arxiv","id":"1908.04410","version":2},"attestation_state":"computed","paper":{"title":"Gravitational Radiation from Binaries: A Pedagogical Introduction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Amir Jafari","submitted_at":"2019-08-07T04:50:00Z","abstract_excerpt":"This short note serves as an introduction to gravitational radiation through reviewing the inspiral-plunge transition phase in extreme mass ratio binaries. We study the relativistic motion of a compact object (CO) of mass $m$ around a massive black hole of mass $M\\gg m$. The Kerr-Newman metric, effective potential for the general case of elliptical orbits, gravitational radiation, orbital energy and angular momentum of a coalescing CO in Kerr spacetime and gravitational wave frequency and signal to noise ratio are briefly reviewed. The main focus is on the transition from inspiral to plunge fo"},"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":"1908.04410","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2019-08-07T04:50:00Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"5913dbaecd09f61eb1193bca3fb6247be85d94f998c6a88ccffa84b1b3eb9e0e","abstract_canon_sha256":"c34acdc64ee503c93da12126c6f40dad737f505eec748c689a92d8724443f6a8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T23:58:10.951140Z","signature_b64":"FSQ4CZJKN9KmhKizEAU+2OUay1VCr/JtLXCMc0L2Kb8eIX1laj3Wzynj33Tc0i7dVCtzrtSZpbf9spFzJibUCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"c0e94cff0738901bc0a66f5408384e86e47cf6b625123362c3705c7dfb8ab1b5","last_reissued_at":"2026-07-04T23:58:10.950785Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T23:58:10.950785Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Gravitational Radiation from Binaries: A Pedagogical Introduction","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"gr-qc","authors_text":"Amir Jafari","submitted_at":"2019-08-07T04:50:00Z","abstract_excerpt":"This short note serves as an introduction to gravitational radiation through reviewing the inspiral-plunge transition phase in extreme mass ratio binaries. We study the relativistic motion of a compact object (CO) of mass $m$ around a massive black hole of mass $M\\gg m$. The Kerr-Newman metric, effective potential for the general case of elliptical orbits, gravitational radiation, orbital energy and angular momentum of a coalescing CO in Kerr spacetime and gravitational wave frequency and signal to noise ratio are briefly reviewed. The main focus is on the transition from inspiral to plunge fo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1908.04410","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/1908.04410/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":"1908.04410","created_at":"2026-07-04T23:58:10.950841+00:00"},{"alias_kind":"arxiv_version","alias_value":"1908.04410v2","created_at":"2026-07-04T23:58:10.950841+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1908.04410","created_at":"2026-07-04T23:58:10.950841+00:00"},{"alias_kind":"pith_short_12","alias_value":"YDUUZ7YHHCIB","created_at":"2026-07-04T23:58:10.950841+00:00"},{"alias_kind":"pith_short_16","alias_value":"YDUUZ7YHHCIBXQFG","created_at":"2026-07-04T23:58:10.950841+00:00"},{"alias_kind":"pith_short_8","alias_value":"YDUUZ7YH","created_at":"2026-07-04T23:58:10.950841+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/YDUUZ7YHHCIBXQFGN5KAQOCOQ3","json":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3.json","graph_json":"https://pith.science/api/pith-number/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/graph.json","events_json":"https://pith.science/api/pith-number/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/events.json","paper":"https://pith.science/paper/YDUUZ7YH"},"agent_actions":{"view_html":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3","download_json":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3.json","view_paper":"https://pith.science/paper/YDUUZ7YH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1908.04410&json=true","fetch_graph":"https://pith.science/api/pith-number/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/graph.json","fetch_events":"https://pith.science/api/pith-number/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/action/storage_attestation","attest_author":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/action/author_attestation","sign_citation":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/action/citation_signature","submit_replication":"https://pith.science/pith/YDUUZ7YHHCIBXQFGN5KAQOCOQ3/action/replication_record"}},"created_at":"2026-07-04T23:58:10.950841+00:00","updated_at":"2026-07-04T23:58:10.950841+00:00"}