{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:O5TU4AYQRJC2CF22I54U3U2U37","short_pith_number":"pith:O5TU4AYQ","schema_version":"1.0","canonical_sha256":"77674e03108a45a1175a47794dd354dff888857d1837b0db94153d85f62fa6ac","source":{"kind":"arxiv","id":"1603.01286","version":1},"attestation_state":"computed","paper":{"title":"Measurability of the tidal deformability by gravitational waves from coalescing binary neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Kenta Hotokezaka, Koutarou Kyutoku, Masaru Shibata, Yu-ichiro Sekiguchi","submitted_at":"2016-03-03T21:26:03Z","abstract_excerpt":"Combining new gravitational waveforms derived by long-term (14--16 orbits) numerical-relativity simulations with waveforms by an effective-one-body (EOB) formalism for coalescing binary neutron stars, we construct hybrid waveforms and estimate the measurability for the dimensionless tidal deformability of the neutron stars, $\\Lambda$, by advanced gravitational-wave detectors. We focus on the equal-mass case with the total mass $2.7M_\\odot$. We find that for an event at a hypothetical effective distance of $D_{\\rm eff}=200$ Mpc, the distinguishable difference in the dimensionless tidal deformab"},"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":"1603.01286","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2016-03-03T21:26:03Z","cross_cats_sorted":[],"title_canon_sha256":"cdab628de017aec5f626d32082d720012e5ff8edc511698a6c3d9957f084b2a2","abstract_canon_sha256":"ebf4cc265484b98c81cfc8a6771b6014d17a6fb33574f736d0528e048d5257d6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:16:40.064475Z","signature_b64":"9gLwaz9ot2CXfvUgrJTsB63aJbqdzdgw3BOn2bap0wHeck3CQ747wfodWCWvFVH/3oKQGBTaHAJzXDJ6vpwjCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"77674e03108a45a1175a47794dd354dff888857d1837b0db94153d85f62fa6ac","last_reissued_at":"2026-05-18T01:16:40.063754Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:16:40.063754Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measurability of the tidal deformability by gravitational waves from coalescing binary neutron stars","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Kenta Hotokezaka, Koutarou Kyutoku, Masaru Shibata, Yu-ichiro Sekiguchi","submitted_at":"2016-03-03T21:26:03Z","abstract_excerpt":"Combining new gravitational waveforms derived by long-term (14--16 orbits) numerical-relativity simulations with waveforms by an effective-one-body (EOB) formalism for coalescing binary neutron stars, we construct hybrid waveforms and estimate the measurability for the dimensionless tidal deformability of the neutron stars, $\\Lambda$, by advanced gravitational-wave detectors. We focus on the equal-mass case with the total mass $2.7M_\\odot$. We find that for an event at a hypothetical effective distance of $D_{\\rm eff}=200$ Mpc, the distinguishable difference in the dimensionless tidal deformab"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.01286","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":"1603.01286","created_at":"2026-05-18T01:16:40.063876+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.01286v1","created_at":"2026-05-18T01:16:40.063876+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.01286","created_at":"2026-05-18T01:16:40.063876+00:00"},{"alias_kind":"pith_short_12","alias_value":"O5TU4AYQRJC2","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_16","alias_value":"O5TU4AYQRJC2CF22","created_at":"2026-05-18T12:30:36.002864+00:00"},{"alias_kind":"pith_short_8","alias_value":"O5TU4AYQ","created_at":"2026-05-18T12:30:36.002864+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/O5TU4AYQRJC2CF22I54U3U2U37","json":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37.json","graph_json":"https://pith.science/api/pith-number/O5TU4AYQRJC2CF22I54U3U2U37/graph.json","events_json":"https://pith.science/api/pith-number/O5TU4AYQRJC2CF22I54U3U2U37/events.json","paper":"https://pith.science/paper/O5TU4AYQ"},"agent_actions":{"view_html":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37","download_json":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37.json","view_paper":"https://pith.science/paper/O5TU4AYQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.01286&json=true","fetch_graph":"https://pith.science/api/pith-number/O5TU4AYQRJC2CF22I54U3U2U37/graph.json","fetch_events":"https://pith.science/api/pith-number/O5TU4AYQRJC2CF22I54U3U2U37/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37/action/timestamp_anchor","attest_storage":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37/action/storage_attestation","attest_author":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37/action/author_attestation","sign_citation":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37/action/citation_signature","submit_replication":"https://pith.science/pith/O5TU4AYQRJC2CF22I54U3U2U37/action/replication_record"}},"created_at":"2026-05-18T01:16:40.063876+00:00","updated_at":"2026-05-18T01:16:40.063876+00:00"}