{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:MWBX4WTCN4DCBRPR3XTPLQ4TTK","short_pith_number":"pith:MWBX4WTC","schema_version":"1.0","canonical_sha256":"65837e5a626f0620c5f1dde6f5c3939ab3ee9ef2f5d9b29015a0d841ccad4d95","source":{"kind":"arxiv","id":"2311.04672","version":2},"attestation_state":"computed","paper":{"title":"Parametrized multipolar gravitational waveforms for testing general relativity: Amplitude corrections up to 2PN order","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Parthapratim Mahapatra, Shilpa Kastha","submitted_at":"2023-11-08T13:27:23Z","abstract_excerpt":"A parametrized multipolar gravitational wave phasing within multipolar post-Minkowskian and post-Newtonian formalism was developed in earlier works [S. Kastha et al., PRD 98, 124033 (2018) and PRD 100, 044007 (2019)]. This facilitates the model-agnostic tests for the multipolar structure of compact binaries using gravitational wave observations. In this paper, we derive a parametrized multipolar amplitude of the gravitational wave signal in terms of mass and current-type radiative multipole moments within the post-Newtonian approximation to general relativity. We assume the compact binary to b"},"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":"2311.04672","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-11-08T13:27:23Z","cross_cats_sorted":[],"title_canon_sha256":"e82bea9fb796357726941b4eb419ceb036ced38011ce391ce89d28abbb013efc","abstract_canon_sha256":"affc2ab18d518e8367998331c1979153810db50708ed015db7f424cf3caa9171"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:19:06.719755Z","signature_b64":"syguXfwSiluUl79lMqNDCdO1NMx8w/ucuqPLDbGdEaBJBrwuS9TW6WYqKcnDvanSqW0H4yVbOB5rJuluyxIqCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"65837e5a626f0620c5f1dde6f5c3939ab3ee9ef2f5d9b29015a0d841ccad4d95","last_reissued_at":"2026-07-05T09:19:06.719282Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:19:06.719282Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Parametrized multipolar gravitational waveforms for testing general relativity: Amplitude corrections up to 2PN order","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"Parthapratim Mahapatra, Shilpa Kastha","submitted_at":"2023-11-08T13:27:23Z","abstract_excerpt":"A parametrized multipolar gravitational wave phasing within multipolar post-Minkowskian and post-Newtonian formalism was developed in earlier works [S. Kastha et al., PRD 98, 124033 (2018) and PRD 100, 044007 (2019)]. This facilitates the model-agnostic tests for the multipolar structure of compact binaries using gravitational wave observations. In this paper, we derive a parametrized multipolar amplitude of the gravitational wave signal in terms of mass and current-type radiative multipole moments within the post-Newtonian approximation to general relativity. We assume the compact binary to b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2311.04672","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/2311.04672/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":"2311.04672","created_at":"2026-07-05T09:19:06.719349+00:00"},{"alias_kind":"arxiv_version","alias_value":"2311.04672v2","created_at":"2026-07-05T09:19:06.719349+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2311.04672","created_at":"2026-07-05T09:19:06.719349+00:00"},{"alias_kind":"pith_short_12","alias_value":"MWBX4WTCN4DC","created_at":"2026-07-05T09:19:06.719349+00:00"},{"alias_kind":"pith_short_16","alias_value":"MWBX4WTCN4DCBRPR","created_at":"2026-07-05T09:19:06.719349+00:00"},{"alias_kind":"pith_short_8","alias_value":"MWBX4WTC","created_at":"2026-07-05T09:19:06.719349+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2507.21566","citing_title":"Probing missing physics from inspiralling compact binaries via time-frequency tracks","ref_index":27,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK","json":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK.json","graph_json":"https://pith.science/api/pith-number/MWBX4WTCN4DCBRPR3XTPLQ4TTK/graph.json","events_json":"https://pith.science/api/pith-number/MWBX4WTCN4DCBRPR3XTPLQ4TTK/events.json","paper":"https://pith.science/paper/MWBX4WTC"},"agent_actions":{"view_html":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK","download_json":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK.json","view_paper":"https://pith.science/paper/MWBX4WTC","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2311.04672&json=true","fetch_graph":"https://pith.science/api/pith-number/MWBX4WTCN4DCBRPR3XTPLQ4TTK/graph.json","fetch_events":"https://pith.science/api/pith-number/MWBX4WTCN4DCBRPR3XTPLQ4TTK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK/action/storage_attestation","attest_author":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK/action/author_attestation","sign_citation":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK/action/citation_signature","submit_replication":"https://pith.science/pith/MWBX4WTCN4DCBRPR3XTPLQ4TTK/action/replication_record"}},"created_at":"2026-07-05T09:19:06.719349+00:00","updated_at":"2026-07-05T09:19:06.719349+00:00"}