{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:V242RVKT2CO4QBECJ3E5MVJVRD","short_pith_number":"pith:V242RVKT","schema_version":"1.0","canonical_sha256":"aeb9a8d553d09dc804824ec9d6553588c1dc4143133de66dfce4d73da58f0a6d","source":{"kind":"arxiv","id":"2302.08480","version":4},"attestation_state":"computed","paper":{"title":"Dipolar tidal effects in gravitational waves from scalarized black hole binary inspirals in quadratic gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Banafsheh Shiralilou, Iris van Gemeren, Tanja Hinderer","submitted_at":"2023-02-16T18:39:52Z","abstract_excerpt":"Gravitational waves (GWs) from merging binary black holes (BHs) enable unprecedented tests of gravitational theories beyond Einstein's General Relativity (GR) in highly nonlinear, dynamical regimes. Such GW measurements require an accurate description of GW signatures that may arise in alternative gravitational models. In this work, we focus on a class of higher-curvature extensions of GR, the scalar-Gauss-Bonnet theories, where BHs can develop scalar hair. In an inspiraling binary system, this leads to scalar-induced tidal effects in the dynamics and radiation. We calculate the dominant adiab"},"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":"2302.08480","kind":"arxiv","version":4},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2023-02-16T18:39:52Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"35de01f589e500bb44d634c84bc06592a506386c0a82779e278019b0dae83cbc","abstract_canon_sha256":"fb9e4066795d357c1b78580a4a61d4f849d68b4bee45ef3e76a0b686dc60569a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:48:11.689978Z","signature_b64":"N/brdEXmB81ElbHWTF6RHJ5nnx9iw6/sCiZgN2F9jhSnAlAaKtU9RO5eq8cNdrQM9fQG+KtD4sbmRHsP/LBiCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"aeb9a8d553d09dc804824ec9d6553588c1dc4143133de66dfce4d73da58f0a6d","last_reissued_at":"2026-07-05T10:48:11.689578Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:48:11.689578Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dipolar tidal effects in gravitational waves from scalarized black hole binary inspirals in quadratic gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Banafsheh Shiralilou, Iris van Gemeren, Tanja Hinderer","submitted_at":"2023-02-16T18:39:52Z","abstract_excerpt":"Gravitational waves (GWs) from merging binary black holes (BHs) enable unprecedented tests of gravitational theories beyond Einstein's General Relativity (GR) in highly nonlinear, dynamical regimes. Such GW measurements require an accurate description of GW signatures that may arise in alternative gravitational models. In this work, we focus on a class of higher-curvature extensions of GR, the scalar-Gauss-Bonnet theories, where BHs can develop scalar hair. In an inspiraling binary system, this leads to scalar-induced tidal effects in the dynamics and radiation. We calculate the dominant adiab"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.08480","kind":"arxiv","version":4},"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/2302.08480/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":"2302.08480","created_at":"2026-07-05T10:48:11.689630+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.08480v4","created_at":"2026-07-05T10:48:11.689630+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.08480","created_at":"2026-07-05T10:48:11.689630+00:00"},{"alias_kind":"pith_short_12","alias_value":"V242RVKT2CO4","created_at":"2026-07-05T10:48:11.689630+00:00"},{"alias_kind":"pith_short_16","alias_value":"V242RVKT2CO4QBEC","created_at":"2026-07-05T10:48:11.689630+00:00"},{"alias_kind":"pith_short_8","alias_value":"V242RVKT","created_at":"2026-07-05T10:48:11.689630+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2310.19679","citing_title":"Tidal effects up to next-to-next-to leading post-Newtonian order in massless scalar-tensor theories","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD","json":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD.json","graph_json":"https://pith.science/api/pith-number/V242RVKT2CO4QBECJ3E5MVJVRD/graph.json","events_json":"https://pith.science/api/pith-number/V242RVKT2CO4QBECJ3E5MVJVRD/events.json","paper":"https://pith.science/paper/V242RVKT"},"agent_actions":{"view_html":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD","download_json":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD.json","view_paper":"https://pith.science/paper/V242RVKT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.08480&json=true","fetch_graph":"https://pith.science/api/pith-number/V242RVKT2CO4QBECJ3E5MVJVRD/graph.json","fetch_events":"https://pith.science/api/pith-number/V242RVKT2CO4QBECJ3E5MVJVRD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD/action/storage_attestation","attest_author":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD/action/author_attestation","sign_citation":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD/action/citation_signature","submit_replication":"https://pith.science/pith/V242RVKT2CO4QBECJ3E5MVJVRD/action/replication_record"}},"created_at":"2026-07-05T10:48:11.689630+00:00","updated_at":"2026-07-05T10:48:11.689630+00:00"}