{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:FNXDFP5QQPRHEYK3P3AWGMUDTG","short_pith_number":"pith:FNXDFP5Q","schema_version":"1.0","canonical_sha256":"2b6e32bfb083e272615b7ec163328399bb27e5155f10bb9a6dd80d7db9fb60c8","source":{"kind":"arxiv","id":"2506.22272","version":3},"attestation_state":"computed","paper":{"title":"A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Aditya Vijaykumar, Alex B. Nielsen, Avinash Tiwari, Shasvath J. Kapadia, Shrobana Ghosh","submitted_at":"2025-06-27T14:43:14Z","abstract_excerpt":"Compact binary coalescences (CBCs), such as merging binary black holes (BBHs), binary neutron stars (BNSs), or neutron star black holes (NSBHs), hosted by dense stellar environments, could produce gravitational waves (GWs) that contain signatures of line-of-sight acceleration (LOSA) imparted by the environment's gravitational potential. We calculate the Post-Newtonian (PN) corrections to the $(2,\\,2)$ mode GW phase due to a finite LOSA, starting from the leading order at -4 PN below the quadrupole order, up to 3.5 PN above the leading order correction. We do so for binaries whose component spi"},"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":"2506.22272","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-06-27T14:43:14Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"bdeedb56e8c120069167fc401f8fef20475fa25bbf0edfc84c459a52b63652f4","abstract_canon_sha256":"34f20773aeb8aafb4a77e37b87ba81640973f4df9e60e526ee75bd806074ffdb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-06-26T01:15:44.721198Z","signature_b64":"BCWbrLaBMKx0iS6fRStjkPVEIRxOdwPC5mI0qdK1Ay9XEJw0d7QI4dSWPO09dEzPguhTqd5aL/Fl0NG5oDFzDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2b6e32bfb083e272615b7ec163328399bb27e5155f10bb9a6dd80d7db9fb60c8","last_reissued_at":"2026-06-26T01:15:44.720679Z","signature_status":"signed_v1","first_computed_at":"2026-06-26T01:15:44.720679Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A pipeline to search for signatures of line-of-sight acceleration in gravitational wave signals produced by compact binary coalescences","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"astro-ph.HE","authors_text":"Aditya Vijaykumar, Alex B. Nielsen, Avinash Tiwari, Shasvath J. Kapadia, Shrobana Ghosh","submitted_at":"2025-06-27T14:43:14Z","abstract_excerpt":"Compact binary coalescences (CBCs), such as merging binary black holes (BBHs), binary neutron stars (BNSs), or neutron star black holes (NSBHs), hosted by dense stellar environments, could produce gravitational waves (GWs) that contain signatures of line-of-sight acceleration (LOSA) imparted by the environment's gravitational potential. We calculate the Post-Newtonian (PN) corrections to the $(2,\\,2)$ mode GW phase due to a finite LOSA, starting from the leading order at -4 PN below the quadrupole order, up to 3.5 PN above the leading order correction. We do so for binaries whose component spi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2506.22272","kind":"arxiv","version":3},"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/2506.22272/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":"2506.22272","created_at":"2026-06-26T01:15:44.720741+00:00"},{"alias_kind":"arxiv_version","alias_value":"2506.22272v3","created_at":"2026-06-26T01:15:44.720741+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2506.22272","created_at":"2026-06-26T01:15:44.720741+00:00"},{"alias_kind":"pith_short_12","alias_value":"FNXDFP5QQPRH","created_at":"2026-06-26T01:15:44.720741+00:00"},{"alias_kind":"pith_short_16","alias_value":"FNXDFP5QQPRHEYK3","created_at":"2026-06-26T01:15:44.720741+00:00"},{"alias_kind":"pith_short_8","alias_value":"FNXDFP5Q","created_at":"2026-06-26T01:15:44.720741+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2605.21955","citing_title":"On the Presence of a Tertiary Compact Object in GW190814","ref_index":102,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG","json":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG.json","graph_json":"https://pith.science/api/pith-number/FNXDFP5QQPRHEYK3P3AWGMUDTG/graph.json","events_json":"https://pith.science/api/pith-number/FNXDFP5QQPRHEYK3P3AWGMUDTG/events.json","paper":"https://pith.science/paper/FNXDFP5Q"},"agent_actions":{"view_html":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG","download_json":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG.json","view_paper":"https://pith.science/paper/FNXDFP5Q","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2506.22272&json=true","fetch_graph":"https://pith.science/api/pith-number/FNXDFP5QQPRHEYK3P3AWGMUDTG/graph.json","fetch_events":"https://pith.science/api/pith-number/FNXDFP5QQPRHEYK3P3AWGMUDTG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG/action/storage_attestation","attest_author":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG/action/author_attestation","sign_citation":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG/action/citation_signature","submit_replication":"https://pith.science/pith/FNXDFP5QQPRHEYK3P3AWGMUDTG/action/replication_record"}},"created_at":"2026-06-26T01:15:44.720741+00:00","updated_at":"2026-06-26T01:15:44.720741+00:00"}