{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:NR7JADJPMOT53UYRKTBALNPCIE","short_pith_number":"pith:NR7JADJP","schema_version":"1.0","canonical_sha256":"6c7e900d2f63a7ddd31154c205b5e2413d9f051e91fdb5e6d7e460b48f5f9198","source":{"kind":"arxiv","id":"2401.05524","version":1},"attestation_state":"computed","paper":{"title":"Causality and quasi-normal modes in the GREFT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Scott Melville","submitted_at":"2024-01-10T19:42:46Z","abstract_excerpt":"The General Relativity Effective Field Theory (GREFT) introduces higher-derivative interactions to parameterise the gravitational effects of massive degrees of freedom which are too heavy to be probed directly. The coefficients of these interactions have recently been constrained using causality: both from the analytic structure of 4-point graviton scattering and the time delay of gravitational waves on a black hole background. In this work, causality is used to constrain the quasi-normal mode spectrum of GREFT black holes. Demanding that quasi-normal mode perturbations decay faster in the GRE"},"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":"2401.05524","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2024-01-10T19:42:46Z","cross_cats_sorted":["hep-th"],"title_canon_sha256":"32f7dd18869335d79780cd88f02c89794d9f8e00d91f6f0db3c69d88371c436f","abstract_canon_sha256":"e556f2fb7bcba1b7b05eb0982c61d4a429a43b1f3d129fcdb7a062a49c9fd57b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:17:31.813160Z","signature_b64":"TD+dpulkOGfK0ZyFTyW+/hP57OILgYC0iuzmVi5yj6DDCKaDAfmkk0JO7Uitm0QToZVv4gn/gNPm9/gh5m5bAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"6c7e900d2f63a7ddd31154c205b5e2413d9f051e91fdb5e6d7e460b48f5f9198","last_reissued_at":"2026-07-05T11:17:31.812718Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:17:31.812718Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Causality and quasi-normal modes in the GREFT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-th"],"primary_cat":"gr-qc","authors_text":"Scott Melville","submitted_at":"2024-01-10T19:42:46Z","abstract_excerpt":"The General Relativity Effective Field Theory (GREFT) introduces higher-derivative interactions to parameterise the gravitational effects of massive degrees of freedom which are too heavy to be probed directly. The coefficients of these interactions have recently been constrained using causality: both from the analytic structure of 4-point graviton scattering and the time delay of gravitational waves on a black hole background. In this work, causality is used to constrain the quasi-normal mode spectrum of GREFT black holes. Demanding that quasi-normal mode perturbations decay faster in the GRE"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2401.05524","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/2401.05524/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":"2401.05524","created_at":"2026-07-05T11:17:31.812774+00:00"},{"alias_kind":"arxiv_version","alias_value":"2401.05524v1","created_at":"2026-07-05T11:17:31.812774+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2401.05524","created_at":"2026-07-05T11:17:31.812774+00:00"},{"alias_kind":"pith_short_12","alias_value":"NR7JADJPMOT5","created_at":"2026-07-05T11:17:31.812774+00:00"},{"alias_kind":"pith_short_16","alias_value":"NR7JADJPMOT53UYR","created_at":"2026-07-05T11:17:31.812774+00:00"},{"alias_kind":"pith_short_8","alias_value":"NR7JADJP","created_at":"2026-07-05T11:17:31.812774+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2512.02338","citing_title":"Leading effective field theory corrections to the Kerr metric at all spins","ref_index":27,"is_internal_anchor":false},{"citing_arxiv_id":"2601.13411","citing_title":"Quasinormal modes and their excitation beyond general relativity. II: isospectrality loss in gravitational waveforms","ref_index":43,"is_internal_anchor":false},{"citing_arxiv_id":"2603.10102","citing_title":"Kerr Black Hole Ringdown in Effective Field Theory","ref_index":51,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE","json":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE.json","graph_json":"https://pith.science/api/pith-number/NR7JADJPMOT53UYRKTBALNPCIE/graph.json","events_json":"https://pith.science/api/pith-number/NR7JADJPMOT53UYRKTBALNPCIE/events.json","paper":"https://pith.science/paper/NR7JADJP"},"agent_actions":{"view_html":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE","download_json":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE.json","view_paper":"https://pith.science/paper/NR7JADJP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2401.05524&json=true","fetch_graph":"https://pith.science/api/pith-number/NR7JADJPMOT53UYRKTBALNPCIE/graph.json","fetch_events":"https://pith.science/api/pith-number/NR7JADJPMOT53UYRKTBALNPCIE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE/action/storage_attestation","attest_author":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE/action/author_attestation","sign_citation":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE/action/citation_signature","submit_replication":"https://pith.science/pith/NR7JADJPMOT53UYRKTBALNPCIE/action/replication_record"}},"created_at":"2026-07-05T11:17:31.812774+00:00","updated_at":"2026-07-05T11:17:31.812774+00:00"}