{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:WKFPNWUGZEVNTZOTEZAKXZJKED","short_pith_number":"pith:WKFPNWUG","schema_version":"1.0","canonical_sha256":"b28af6da86c92ad9e5d32640abe52a20ec7e3845850c1f3f8983b11138ceb44c","source":{"kind":"arxiv","id":"1203.2962","version":2},"attestation_state":"computed","paper":{"title":"Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Andreas Ross, Ira Z. Rothstein, Rafael A. Porto","submitted_at":"2012-03-13T21:55:10Z","abstract_excerpt":"Using the NRGR effective field theory formalism we calculate the remaining source multipole moments necessary to obtain the spin contributions to the gravitational wave amplitude to 2.5 Post-Newtonian (PN) order. We also reproduce the tail contribution to the waveform linear in spin at 2.5PN arising from the nonlinear interaction between the current quadrupole and the mass monopole."},"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":"1203.2962","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2012-03-13T21:55:10Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE","hep-ph","hep-th"],"title_canon_sha256":"f3262e1f4ac75cda9392a16dad5699ea510a2c4b2c99de16ac7fcafb35b7f307","abstract_canon_sha256":"dc1bdf93e62c76feb835f8c3530e5e73bdb6aaf30aaef00023afa9e61b535edf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:09.083795Z","signature_b64":"0WlTVti3G8NXjN3rRknEN/fJ2xFan5h1KQElkIz0VUG0C/22yCxdzUFqOC+ZMV1u/wBBpRT2aglL+XyInPH0Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b28af6da86c92ad9e5d32640abe52a20ec7e3845850c1f3f8983b11138ceb44c","last_reissued_at":"2026-05-18T01:58:09.083383Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:09.083383Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spin induced multipole moments for the gravitational wave amplitude from binary inspirals to 2.5 Post-Newtonian order","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE","hep-ph","hep-th"],"primary_cat":"gr-qc","authors_text":"Andreas Ross, Ira Z. Rothstein, Rafael A. Porto","submitted_at":"2012-03-13T21:55:10Z","abstract_excerpt":"Using the NRGR effective field theory formalism we calculate the remaining source multipole moments necessary to obtain the spin contributions to the gravitational wave amplitude to 2.5 Post-Newtonian (PN) order. We also reproduce the tail contribution to the waveform linear in spin at 2.5PN arising from the nonlinear interaction between the current quadrupole and the mass monopole."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1203.2962","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":""},"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":"1203.2962","created_at":"2026-05-18T01:58:09.083446+00:00"},{"alias_kind":"arxiv_version","alias_value":"1203.2962v2","created_at":"2026-05-18T01:58:09.083446+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1203.2962","created_at":"2026-05-18T01:58:09.083446+00:00"},{"alias_kind":"pith_short_12","alias_value":"WKFPNWUGZEVN","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_16","alias_value":"WKFPNWUGZEVNTZOT","created_at":"2026-05-18T12:27:25.539911+00:00"},{"alias_kind":"pith_short_8","alias_value":"WKFPNWUG","created_at":"2026-05-18T12:27:25.539911+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2305.15473","citing_title":"Worldline effective field theory of inspiralling black hole binaries in presence of dark photon and axionic dark matter","ref_index":35,"is_internal_anchor":true},{"citing_arxiv_id":"2602.18790","citing_title":"Generalized Carter & R\\\"udiger Constants of $\\sqrt{\\text{Kerr}}$","ref_index":30,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED","json":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED.json","graph_json":"https://pith.science/api/pith-number/WKFPNWUGZEVNTZOTEZAKXZJKED/graph.json","events_json":"https://pith.science/api/pith-number/WKFPNWUGZEVNTZOTEZAKXZJKED/events.json","paper":"https://pith.science/paper/WKFPNWUG"},"agent_actions":{"view_html":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED","download_json":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED.json","view_paper":"https://pith.science/paper/WKFPNWUG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1203.2962&json=true","fetch_graph":"https://pith.science/api/pith-number/WKFPNWUGZEVNTZOTEZAKXZJKED/graph.json","fetch_events":"https://pith.science/api/pith-number/WKFPNWUGZEVNTZOTEZAKXZJKED/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED/action/storage_attestation","attest_author":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED/action/author_attestation","sign_citation":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED/action/citation_signature","submit_replication":"https://pith.science/pith/WKFPNWUGZEVNTZOTEZAKXZJKED/action/replication_record"}},"created_at":"2026-05-18T01:58:09.083446+00:00","updated_at":"2026-05-18T01:58:09.083446+00:00"}