{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2001:CZ466ULT5UK2XIGWFFMKCSL6EO","short_pith_number":"pith:CZ466ULT","schema_version":"1.0","canonical_sha256":"1679ef5173ed15aba0d62958a1497e23a9c86998f0047f3fa800f48ac8e51808","source":{"kind":"arxiv","id":"astro-ph/0111066","version":2},"attestation_state":"computed","paper":{"title":"Broad-band gravitational-wave pulses from binary neutron stars in eccentric orbits","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph","authors_text":"2), A.G.Kuranov (1), A.V.Gusev (1), Garching), K.A.Postnov (1, M.E.Prokhorov (1)((1) Sternberg Astronomical Insitute, Moscow (2) MPA fuer Astrophysik, V.B.Ignatiev (1)","submitted_at":"2001-11-04T16:11:07Z","abstract_excerpt":"Maximum gravitational wave emission from binary stars in eccentric orbits occurs near the periastron passage. We show that for a stationary distribution of binary neutron stars in the Galaxy, several high-eccentricity systems with orbital periods in the range from tens of minutes to several days should exist that emit broad gravitational-wave pulses in the frequency range 1-100 mHz. The space interferometer LISA could register the pulsed signal from these system at a signal-to-noise ratio level $S/N>5\\sqrt{5}$ in the frequency range $\\sim 10^{-3}-10^{-1}$ Hz during one-year observational time."},"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/0111066","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2001-11-04T16:11:07Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"2c7a0d30d5987c26e5f85089480bdeba5cdc9b92c17b06aa7e312fe5a4d41f6e","abstract_canon_sha256":"cdf0f37d538bb5f90d312de3971e393f951ecabde553976cb95090c1a55647bd"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:24:24.559077Z","signature_b64":"3BKQl+uffUxiL00gnLCl5zgLbJbcrgzqSf/HPG/SHAE/iwocOSW3yJgMVjFQH5ZLZzIGXu7hsoDXpOIVI0zgCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1679ef5173ed15aba0d62958a1497e23a9c86998f0047f3fa800f48ac8e51808","last_reissued_at":"2026-07-04T16:24:24.558549Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:24:24.558549Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Broad-band gravitational-wave pulses from binary neutron stars in eccentric orbits","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph","authors_text":"2), A.G.Kuranov (1), A.V.Gusev (1), Garching), K.A.Postnov (1, M.E.Prokhorov (1)((1) Sternberg Astronomical Insitute, Moscow (2) MPA fuer Astrophysik, V.B.Ignatiev (1)","submitted_at":"2001-11-04T16:11:07Z","abstract_excerpt":"Maximum gravitational wave emission from binary stars in eccentric orbits occurs near the periastron passage. We show that for a stationary distribution of binary neutron stars in the Galaxy, several high-eccentricity systems with orbital periods in the range from tens of minutes to several days should exist that emit broad gravitational-wave pulses in the frequency range 1-100 mHz. The space interferometer LISA could register the pulsed signal from these system at a signal-to-noise ratio level $S/N>5\\sqrt{5}$ in the frequency range $\\sim 10^{-3}-10^{-1}$ Hz during one-year observational time."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0111066","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/astro-ph/0111066/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":"astro-ph/0111066","created_at":"2026-07-04T16:24:24.558621+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0111066v2","created_at":"2026-07-04T16:24:24.558621+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0111066","created_at":"2026-07-04T16:24:24.558621+00:00"},{"alias_kind":"pith_short_12","alias_value":"CZ466ULT5UK2","created_at":"2026-07-04T16:24:24.558621+00:00"},{"alias_kind":"pith_short_16","alias_value":"CZ466ULT5UK2XIGW","created_at":"2026-07-04T16:24:24.558621+00:00"},{"alias_kind":"pith_short_8","alias_value":"CZ466ULT","created_at":"2026-07-04T16:24:24.558621+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/CZ466ULT5UK2XIGWFFMKCSL6EO","json":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO.json","graph_json":"https://pith.science/api/pith-number/CZ466ULT5UK2XIGWFFMKCSL6EO/graph.json","events_json":"https://pith.science/api/pith-number/CZ466ULT5UK2XIGWFFMKCSL6EO/events.json","paper":"https://pith.science/paper/CZ466ULT"},"agent_actions":{"view_html":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO","download_json":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO.json","view_paper":"https://pith.science/paper/CZ466ULT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0111066&json=true","fetch_graph":"https://pith.science/api/pith-number/CZ466ULT5UK2XIGWFFMKCSL6EO/graph.json","fetch_events":"https://pith.science/api/pith-number/CZ466ULT5UK2XIGWFFMKCSL6EO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO/action/storage_attestation","attest_author":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO/action/author_attestation","sign_citation":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO/action/citation_signature","submit_replication":"https://pith.science/pith/CZ466ULT5UK2XIGWFFMKCSL6EO/action/replication_record"}},"created_at":"2026-07-04T16:24:24.558621+00:00","updated_at":"2026-07-04T16:24:24.558621+00:00"}