{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:TJ3FW4FXHBNJM4RUBDUG2FZDL4","short_pith_number":"pith:TJ3FW4FX","schema_version":"1.0","canonical_sha256":"9a765b70b7385a96723408e86d17235f1f76d843917a38228ee9b7485e41e519","source":{"kind":"arxiv","id":"2001.00721","version":2},"attestation_state":"computed","paper":{"title":"Phase shift of gravitational waves induced by aberration","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Alejandro Torres-Orjuela, Pau Amaro-Seoane, Xian Chen","submitted_at":"2020-01-03T04:59:05Z","abstract_excerpt":"The velocity of a gravitational wave (GW) source provides crucial information about its formation and evolution processes. Previous studies considered the Doppler effect on the phase of GWs as a potential signature of a time-dependent velocity of the source. However, the Doppler shift only accounts for the time component of the wave vector, and in principle motion also affects the spatial components. The latter effect, known as ``aberration'' for light, is analyzed in this paper for GWs and applied to the waveform modeling of an accelerating source. We show that the additional aberrational pha"},"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":"2001.00721","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2020-01-03T04:59:05Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"d241d7600847aed715a9ab1aab4f9ddc3f2a3e97ff8e922bbeef98f7c3194780","abstract_canon_sha256":"d012a3e6310429babc002ba2e4301538be184c199c052486a79a41b9042844f4"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:58:07.237063Z","signature_b64":"0FX/GoBRH6En6panjaQKrmkpcXu8W1R20Arn3QPrkQ4cEeyvjGu6Zb5KRJJjZ6b+Kb+zNAj9/UiQ89TBexCoDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9a765b70b7385a96723408e86d17235f1f76d843917a38228ee9b7485e41e519","last_reissued_at":"2026-07-05T00:58:07.236581Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:58:07.236581Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Phase shift of gravitational waves induced by aberration","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Alejandro Torres-Orjuela, Pau Amaro-Seoane, Xian Chen","submitted_at":"2020-01-03T04:59:05Z","abstract_excerpt":"The velocity of a gravitational wave (GW) source provides crucial information about its formation and evolution processes. Previous studies considered the Doppler effect on the phase of GWs as a potential signature of a time-dependent velocity of the source. However, the Doppler shift only accounts for the time component of the wave vector, and in principle motion also affects the spatial components. The latter effect, known as ``aberration'' for light, is analyzed in this paper for GWs and applied to the waveform modeling of an accelerating source. We show that the additional aberrational pha"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2001.00721","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/2001.00721/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":"2001.00721","created_at":"2026-07-05T00:58:07.236640+00:00"},{"alias_kind":"arxiv_version","alias_value":"2001.00721v2","created_at":"2026-07-05T00:58:07.236640+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2001.00721","created_at":"2026-07-05T00:58:07.236640+00:00"},{"alias_kind":"pith_short_12","alias_value":"TJ3FW4FXHBNJ","created_at":"2026-07-05T00:58:07.236640+00:00"},{"alias_kind":"pith_short_16","alias_value":"TJ3FW4FXHBNJM4RU","created_at":"2026-07-05T00:58:07.236640+00:00"},{"alias_kind":"pith_short_8","alias_value":"TJ3FW4FX","created_at":"2026-07-05T00:58:07.236640+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2311.01300","citing_title":"Waveform Modelling for the Laser Interferometer Space Antenna","ref_index":173,"is_internal_anchor":false},{"citing_arxiv_id":"2605.20320","citing_title":"Ringdown and lensing of triple systems","ref_index":62,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4","json":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4.json","graph_json":"https://pith.science/api/pith-number/TJ3FW4FXHBNJM4RUBDUG2FZDL4/graph.json","events_json":"https://pith.science/api/pith-number/TJ3FW4FXHBNJM4RUBDUG2FZDL4/events.json","paper":"https://pith.science/paper/TJ3FW4FX"},"agent_actions":{"view_html":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4","download_json":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4.json","view_paper":"https://pith.science/paper/TJ3FW4FX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2001.00721&json=true","fetch_graph":"https://pith.science/api/pith-number/TJ3FW4FXHBNJM4RUBDUG2FZDL4/graph.json","fetch_events":"https://pith.science/api/pith-number/TJ3FW4FXHBNJM4RUBDUG2FZDL4/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4/action/storage_attestation","attest_author":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4/action/author_attestation","sign_citation":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4/action/citation_signature","submit_replication":"https://pith.science/pith/TJ3FW4FXHBNJM4RUBDUG2FZDL4/action/replication_record"}},"created_at":"2026-07-05T00:58:07.236640+00:00","updated_at":"2026-07-05T00:58:07.236640+00:00"}