{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2005:CWPPYSTWWOYL6CSVA5DYWWDVRN","short_pith_number":"pith:CWPPYSTW","schema_version":"1.0","canonical_sha256":"159efc4a76b3b0bf0a5507478b58758b524597a160dfca80f0c1f4ba4097e024","source":{"kind":"arxiv","id":"astro-ph/0510602","version":1},"attestation_state":"computed","paper":{"title":"The Kepler equation for inspiralling compact binaries","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph","authors_text":"Bal\\'azs Mik\\'oczi, L\\'aszl\\'o \\'A. Gergely, Zolt\\'an Keresztes","submitted_at":"2005-10-20T10:38:03Z","abstract_excerpt":"Compact binaries consisting of neutron stars / black holes on eccentric orbit undergo a perturbed Keplerian motion. The perturbations are either of relativistic origin or are related to the spin, mass quadrupole and magnetic dipole moments of the binary components. The post-Newtonian motion of such systems decouples into radial and angular parts. We present here for the first time the radial motion of such a binary encoded in a generalized Kepler equation, with the inclusion of all above-mentioned contributions, up to linear order in the perturbations. Together with suitably introduced paramet"},"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":"astro-ph/0510602","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2005-10-20T10:38:03Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"ee79c9d43f8669aba95f525824d482c77144cd30eee931e52876b414a6763d7d","abstract_canon_sha256":"a3ae4a55389c9997f5eca966072cb5be8dc7cc0412fdd60fca8c930fb03a03e3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:08:58.852576Z","signature_b64":"NJiMbK3J3BATJ8BEVsg2+jXYfqHI0PTp7pZRgkYbCWZ7D3LI0SnggCV96fqRbqctwxGumZdRrK7WwA5ip0UXDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"159efc4a76b3b0bf0a5507478b58758b524597a160dfca80f0c1f4ba4097e024","last_reissued_at":"2026-05-18T01:08:58.851703Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:08:58.851703Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"The Kepler equation for inspiralling compact binaries","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph","authors_text":"Bal\\'azs Mik\\'oczi, L\\'aszl\\'o \\'A. Gergely, Zolt\\'an Keresztes","submitted_at":"2005-10-20T10:38:03Z","abstract_excerpt":"Compact binaries consisting of neutron stars / black holes on eccentric orbit undergo a perturbed Keplerian motion. The perturbations are either of relativistic origin or are related to the spin, mass quadrupole and magnetic dipole moments of the binary components. The post-Newtonian motion of such systems decouples into radial and angular parts. We present here for the first time the radial motion of such a binary encoded in a generalized Kepler equation, with the inclusion of all above-mentioned contributions, up to linear order in the perturbations. Together with suitably introduced paramet"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0510602","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":"astro-ph/0510602","created_at":"2026-05-18T01:08:58.851860+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0510602v1","created_at":"2026-05-18T01:08:58.851860+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0510602","created_at":"2026-05-18T01:08:58.851860+00:00"},{"alias_kind":"pith_short_12","alias_value":"CWPPYSTWWOYL","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_16","alias_value":"CWPPYSTWWOYL6CSV","created_at":"2026-05-18T12:25:53.335082+00:00"},{"alias_kind":"pith_short_8","alias_value":"CWPPYSTW","created_at":"2026-05-18T12:25:53.335082+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/CWPPYSTWWOYL6CSVA5DYWWDVRN","json":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN.json","graph_json":"https://pith.science/api/pith-number/CWPPYSTWWOYL6CSVA5DYWWDVRN/graph.json","events_json":"https://pith.science/api/pith-number/CWPPYSTWWOYL6CSVA5DYWWDVRN/events.json","paper":"https://pith.science/paper/CWPPYSTW"},"agent_actions":{"view_html":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN","download_json":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN.json","view_paper":"https://pith.science/paper/CWPPYSTW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0510602&json=true","fetch_graph":"https://pith.science/api/pith-number/CWPPYSTWWOYL6CSVA5DYWWDVRN/graph.json","fetch_events":"https://pith.science/api/pith-number/CWPPYSTWWOYL6CSVA5DYWWDVRN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN/action/storage_attestation","attest_author":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN/action/author_attestation","sign_citation":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN/action/citation_signature","submit_replication":"https://pith.science/pith/CWPPYSTWWOYL6CSVA5DYWWDVRN/action/replication_record"}},"created_at":"2026-05-18T01:08:58.851860+00:00","updated_at":"2026-05-18T01:08:58.851860+00:00"}