{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:56Q7V6L4RNETCJYY36SSAROTAP","short_pith_number":"pith:56Q7V6L4","schema_version":"1.0","canonical_sha256":"efa1faf97c8b49312718dfa52045d303d6d963b800a17f8ce02955fd9f692d72","source":{"kind":"arxiv","id":"1702.01750","version":4},"attestation_state":"computed","paper":{"title":"Cosmological perturbation effects on gravitational-wave luminosity distance estimates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Alvise Raccanelli, Daniele Bertacca, Nicola Bartolo, Sabino Matarrese","submitted_at":"2017-02-06T19:00:01Z","abstract_excerpt":"Waveforms of gravitational waves provide information about a variety of parameters for the binary system merging. However, standard calculations have been performed assuming a FLRW universe with no perturbations. In reality this assumption should be dropped: we show that the inclusion of cosmological perturbations translates into corrections to the estimate of astrophysical parameters derived for the merging binary systems. We compute corrections to the estimate of the luminosity distance due to velocity, volume, lensing and gravitational potential effects. Our results show that the amplitude "},"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":"1702.01750","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2017-02-06T19:00:01Z","cross_cats_sorted":["astro-ph.CO"],"title_canon_sha256":"1c1d6b52baf8e54f58b2a83515246a6f1accccc7cf38d25b9551f55c25dd69a7","abstract_canon_sha256":"325fd74dc8d6de685ee915b0500e94300f75541e78658ff14f26ac863fbf5ab6"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:10:48.794441Z","signature_b64":"3qrVWDAOwCp6lwaOqYiNTleIKjbVw0f7jJe5yeMIuibxyIYIpvZmS/6F2GUyeCjCIR0aTnXRTF/9tA7LQz0FAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"efa1faf97c8b49312718dfa52045d303d6d963b800a17f8ce02955fd9f692d72","last_reissued_at":"2026-07-05T00:10:48.793949Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:10:48.793949Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmological perturbation effects on gravitational-wave luminosity distance estimates","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO"],"primary_cat":"gr-qc","authors_text":"Alvise Raccanelli, Daniele Bertacca, Nicola Bartolo, Sabino Matarrese","submitted_at":"2017-02-06T19:00:01Z","abstract_excerpt":"Waveforms of gravitational waves provide information about a variety of parameters for the binary system merging. However, standard calculations have been performed assuming a FLRW universe with no perturbations. In reality this assumption should be dropped: we show that the inclusion of cosmological perturbations translates into corrections to the estimate of astrophysical parameters derived for the merging binary systems. We compute corrections to the estimate of the luminosity distance due to velocity, volume, lensing and gravitational potential effects. Our results show that the amplitude "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1702.01750","kind":"arxiv","version":4},"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/1702.01750/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":"1702.01750","created_at":"2026-07-05T00:10:48.794007+00:00"},{"alias_kind":"arxiv_version","alias_value":"1702.01750v4","created_at":"2026-07-05T00:10:48.794007+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1702.01750","created_at":"2026-07-05T00:10:48.794007+00:00"},{"alias_kind":"pith_short_12","alias_value":"56Q7V6L4RNET","created_at":"2026-07-05T00:10:48.794007+00:00"},{"alias_kind":"pith_short_16","alias_value":"56Q7V6L4RNETCJYY","created_at":"2026-07-05T00:10:48.794007+00:00"},{"alias_kind":"pith_short_8","alias_value":"56Q7V6L4","created_at":"2026-07-05T00:10:48.794007+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.21584","citing_title":"Wave-optics gravitational wave lensing in modified gravity","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"1912.02622","citing_title":"Science Case for the Einstein Telescope","ref_index":207,"is_internal_anchor":false},{"citing_arxiv_id":"2604.15313","citing_title":"Gravitational-wave lensing beyond rays: a disordered-system approach","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP","json":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP.json","graph_json":"https://pith.science/api/pith-number/56Q7V6L4RNETCJYY36SSAROTAP/graph.json","events_json":"https://pith.science/api/pith-number/56Q7V6L4RNETCJYY36SSAROTAP/events.json","paper":"https://pith.science/paper/56Q7V6L4"},"agent_actions":{"view_html":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP","download_json":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP.json","view_paper":"https://pith.science/paper/56Q7V6L4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1702.01750&json=true","fetch_graph":"https://pith.science/api/pith-number/56Q7V6L4RNETCJYY36SSAROTAP/graph.json","fetch_events":"https://pith.science/api/pith-number/56Q7V6L4RNETCJYY36SSAROTAP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP/action/storage_attestation","attest_author":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP/action/author_attestation","sign_citation":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP/action/citation_signature","submit_replication":"https://pith.science/pith/56Q7V6L4RNETCJYY36SSAROTAP/action/replication_record"}},"created_at":"2026-07-05T00:10:48.794007+00:00","updated_at":"2026-07-05T00:10:48.794007+00:00"}