{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:IF2CPVLHGDXUTWQRBLBH5V2AQF","short_pith_number":"pith:IF2CPVLH","schema_version":"1.0","canonical_sha256":"417427d56730ef49da110ac27ed740815dddcd870f0e14e26a2f1098e297eb64","source":{"kind":"arxiv","id":"2407.16457","version":3},"attestation_state":"computed","paper":{"title":"Spinning waveforms of scalar radiation in quadratic modified gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Adam Falkowski, Panagiotis Marinellis","submitted_at":"2024-07-23T13:14:05Z","abstract_excerpt":"We study scalar-tensor gravitational theories using on-shell amplitude methods. We focus on theories with gravity coupled to a massless scalar via the Gauss-Bonnet and Chern-Simons terms. In this framework, we calculate the waveforms for classical scalar radiation emitted in scattering of macroscopic objects, including spin effects. To this end, we use the Kosower-Maybee-O'Connell formalism, with the 5-particle amplitude for scalar emission in matter scattering calculated at tree level using the unitarity-factorization bootstrap techniques. We also discuss in detail the dependence of that ampl"},"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":"2407.16457","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-07-23T13:14:05Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"ea3c736614dcf6dc9c95473c782c7089b54de7b2354ca1d7279aeb8f5732125c","abstract_canon_sha256":"ebd5ef91f131c125b37c116e77cd506d8388aecccea932afc02f71d468088809"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:41:13.989389Z","signature_b64":"GkxmkSheiyWbFv7Otz+KyA/TUBSMzAMkkvgyrt8IYnTC/Zc9bHA+ElivMKbspsyNDqydmJTWaf/eSpizkb61Aw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"417427d56730ef49da110ac27ed740815dddcd870f0e14e26a2f1098e297eb64","last_reissued_at":"2026-07-05T10:41:13.988885Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:41:13.988885Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spinning waveforms of scalar radiation in quadratic modified gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Adam Falkowski, Panagiotis Marinellis","submitted_at":"2024-07-23T13:14:05Z","abstract_excerpt":"We study scalar-tensor gravitational theories using on-shell amplitude methods. We focus on theories with gravity coupled to a massless scalar via the Gauss-Bonnet and Chern-Simons terms. In this framework, we calculate the waveforms for classical scalar radiation emitted in scattering of macroscopic objects, including spin effects. To this end, we use the Kosower-Maybee-O'Connell formalism, with the 5-particle amplitude for scalar emission in matter scattering calculated at tree level using the unitarity-factorization bootstrap techniques. We also discuss in detail the dependence of that ampl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2407.16457","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/2407.16457/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":"2407.16457","created_at":"2026-07-05T10:41:13.988947+00:00"},{"alias_kind":"arxiv_version","alias_value":"2407.16457v3","created_at":"2026-07-05T10:41:13.988947+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2407.16457","created_at":"2026-07-05T10:41:13.988947+00:00"},{"alias_kind":"pith_short_12","alias_value":"IF2CPVLHGDXU","created_at":"2026-07-05T10:41:13.988947+00:00"},{"alias_kind":"pith_short_16","alias_value":"IF2CPVLHGDXUTWQR","created_at":"2026-07-05T10:41:13.988947+00:00"},{"alias_kind":"pith_short_8","alias_value":"IF2CPVLH","created_at":"2026-07-05T10:41:13.988947+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.28239","citing_title":"Gravitational Compton scattering at the fourth post-Minkowskian order","ref_index":50,"is_internal_anchor":false},{"citing_arxiv_id":"2510.07390","citing_title":"Heterotic Footprints in Classical Gravity: PM dynamics from On-Shell soft amplitudes at one loop","ref_index":136,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF","json":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF.json","graph_json":"https://pith.science/api/pith-number/IF2CPVLHGDXUTWQRBLBH5V2AQF/graph.json","events_json":"https://pith.science/api/pith-number/IF2CPVLHGDXUTWQRBLBH5V2AQF/events.json","paper":"https://pith.science/paper/IF2CPVLH"},"agent_actions":{"view_html":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF","download_json":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF.json","view_paper":"https://pith.science/paper/IF2CPVLH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2407.16457&json=true","fetch_graph":"https://pith.science/api/pith-number/IF2CPVLHGDXUTWQRBLBH5V2AQF/graph.json","fetch_events":"https://pith.science/api/pith-number/IF2CPVLHGDXUTWQRBLBH5V2AQF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF/action/storage_attestation","attest_author":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF/action/author_attestation","sign_citation":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF/action/citation_signature","submit_replication":"https://pith.science/pith/IF2CPVLHGDXUTWQRBLBH5V2AQF/action/replication_record"}},"created_at":"2026-07-05T10:41:13.988947+00:00","updated_at":"2026-07-05T10:41:13.988947+00:00"}