{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:MCTUNFEAXOE4726LY5QF3ODAZN","short_pith_number":"pith:MCTUNFEA","schema_version":"1.0","canonical_sha256":"60a7469480bb89cfebcbc7605db860cb43b6502305a880e419823eebe53e56e4","source":{"kind":"arxiv","id":"2304.14430","version":1},"attestation_state":"computed","paper":{"title":"Scalar polarization window in gravitational-wave signals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"Hidetoshi Omiya, Hiroki Takeda, Takahiro Tanaka, Yusuke Manita","submitted_at":"2023-04-27T18:00:00Z","abstract_excerpt":"Scalar polarization modes of gravitational waves, which are often introduced in the context of the viable extension of gravity, have been actively searched. However, couplings of the scalar modes to the matter are strongly constrained by the fifth-force experiments. Thus, the amplitude of scalar polarization in the observed gravitational-wave signal must be significantly suppressed compared to that of the tensor modes. Here, we discuss the implications of the experiments in the solar system on the detectability of scalar modes in gravitational waves from compact binary coalescences, taking int"},"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":"2304.14430","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-04-27T18:00:00Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"9cd3b039f8f39c745e8195a0dd69c7a2311ff99bb88ab931ec0afe86d199392f","abstract_canon_sha256":"e69d629d8a119fb945cf98c5cc8873ca3c7e09c60701e659bb253288294a4a61"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:32:27.418995Z","signature_b64":"Jixka3nGKeK7K4lStitiTNgvcAkH+jlQ+4HDLGE6cdMwar7YP6/ceaHU5MSELk4ded7RvNw8jKpwcPdFQH0oAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"60a7469480bb89cfebcbc7605db860cb43b6502305a880e419823eebe53e56e4","last_reissued_at":"2026-07-05T06:32:27.418577Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:32:27.418577Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Scalar polarization window in gravitational-wave signals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"gr-qc","authors_text":"Hidetoshi Omiya, Hiroki Takeda, Takahiro Tanaka, Yusuke Manita","submitted_at":"2023-04-27T18:00:00Z","abstract_excerpt":"Scalar polarization modes of gravitational waves, which are often introduced in the context of the viable extension of gravity, have been actively searched. However, couplings of the scalar modes to the matter are strongly constrained by the fifth-force experiments. Thus, the amplitude of scalar polarization in the observed gravitational-wave signal must be significantly suppressed compared to that of the tensor modes. Here, we discuss the implications of the experiments in the solar system on the detectability of scalar modes in gravitational waves from compact binary coalescences, taking int"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2304.14430","kind":"arxiv","version":1},"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/2304.14430/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":"2304.14430","created_at":"2026-07-05T06:32:27.418630+00:00"},{"alias_kind":"arxiv_version","alias_value":"2304.14430v1","created_at":"2026-07-05T06:32:27.418630+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2304.14430","created_at":"2026-07-05T06:32:27.418630+00:00"},{"alias_kind":"pith_short_12","alias_value":"MCTUNFEAXOE4","created_at":"2026-07-05T06:32:27.418630+00:00"},{"alias_kind":"pith_short_16","alias_value":"MCTUNFEAXOE4726L","created_at":"2026-07-05T06:32:27.418630+00:00"},{"alias_kind":"pith_short_8","alias_value":"MCTUNFEA","created_at":"2026-07-05T06:32:27.418630+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2501.18125","citing_title":"Better early than never: A new test for superluminal gravitational wave polarizations","ref_index":60,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN","json":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN.json","graph_json":"https://pith.science/api/pith-number/MCTUNFEAXOE4726LY5QF3ODAZN/graph.json","events_json":"https://pith.science/api/pith-number/MCTUNFEAXOE4726LY5QF3ODAZN/events.json","paper":"https://pith.science/paper/MCTUNFEA"},"agent_actions":{"view_html":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN","download_json":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN.json","view_paper":"https://pith.science/paper/MCTUNFEA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2304.14430&json=true","fetch_graph":"https://pith.science/api/pith-number/MCTUNFEAXOE4726LY5QF3ODAZN/graph.json","fetch_events":"https://pith.science/api/pith-number/MCTUNFEAXOE4726LY5QF3ODAZN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN/action/storage_attestation","attest_author":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN/action/author_attestation","sign_citation":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN/action/citation_signature","submit_replication":"https://pith.science/pith/MCTUNFEAXOE4726LY5QF3ODAZN/action/replication_record"}},"created_at":"2026-07-05T06:32:27.418630+00:00","updated_at":"2026-07-05T06:32:27.418630+00:00"}