{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2020:QPMS7DCSR77AJRKEKT2GRS4YLX","short_pith_number":"pith:QPMS7DCS","schema_version":"1.0","canonical_sha256":"83d92f8c528ffe04c54454f468cb985de1f1c859814a9b163226ee08b0ef6e66","source":{"kind":"arxiv","id":"2005.13923","version":3},"attestation_state":"computed","paper":{"title":"Black Hole Gravitational Waves in the Effective Field Theory of Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Claudia de Rham, J\\'er\\'emie Francfort, Jun Zhang","submitted_at":"2020-05-28T11:41:37Z","abstract_excerpt":"We investigate the propagation of gravitational waves on a black hole background within the low energy effective field theory of gravity, where effects from heavy fields are captured by higher dimensional curvature operators. Depending on the spin of the particles integrated out, the speed of gravitational waves at low energy can be either superluminal or subluminal as compared to the causal structure observed by other species. Interestingly however, gravitational waves are always exactly luminal at the black hole horizon, implying that the horizon is identically defined for all species. We fu"},"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":"2005.13923","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2020-05-28T11:41:37Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"122e9335642dac558cce27ed5e6eee243bc79eea7e909a70609ea034a4bdc6fd","abstract_canon_sha256":"529618dff9baa128fec86150a5b673c9c2a9217275e209313cd639c914e3b9e0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:24:36.164917Z","signature_b64":"CwDsi8Lh6gst4TUpIdut1wRhmRWY5HjdcfNlS4OQ+ehcgpTJwVMvuBS2uDAW8XmOXxO8YnieMDueDJBdhLk2CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"83d92f8c528ffe04c54454f468cb985de1f1c859814a9b163226ee08b0ef6e66","last_reissued_at":"2026-07-05T01:24:36.164529Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:24:36.164529Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black Hole Gravitational Waves in the Effective Field Theory of Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Claudia de Rham, J\\'er\\'emie Francfort, Jun Zhang","submitted_at":"2020-05-28T11:41:37Z","abstract_excerpt":"We investigate the propagation of gravitational waves on a black hole background within the low energy effective field theory of gravity, where effects from heavy fields are captured by higher dimensional curvature operators. Depending on the spin of the particles integrated out, the speed of gravitational waves at low energy can be either superluminal or subluminal as compared to the causal structure observed by other species. Interestingly however, gravitational waves are always exactly luminal at the black hole horizon, implying that the horizon is identically defined for all species. We fu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2005.13923","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/2005.13923/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":"2005.13923","created_at":"2026-07-05T01:24:36.164582+00:00"},{"alias_kind":"arxiv_version","alias_value":"2005.13923v3","created_at":"2026-07-05T01:24:36.164582+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2005.13923","created_at":"2026-07-05T01:24:36.164582+00:00"},{"alias_kind":"pith_short_12","alias_value":"QPMS7DCSR77A","created_at":"2026-07-05T01:24:36.164582+00:00"},{"alias_kind":"pith_short_16","alias_value":"QPMS7DCSR77AJRKE","created_at":"2026-07-05T01:24:36.164582+00:00"},{"alias_kind":"pith_short_8","alias_value":"QPMS7DCS","created_at":"2026-07-05T01:24:36.164582+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.09766","citing_title":"Modified Teukolsky Formalism for Extreme Mass-Ratio Inspirals in Higher-Derivative Gravity","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2606.07070","citing_title":"Gravitational waveforms from binaries in higher-derivative gravity: a Love story","ref_index":58,"is_internal_anchor":false},{"citing_arxiv_id":"2512.02338","citing_title":"Leading effective field theory corrections to the Kerr metric at all spins","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2512.11911","citing_title":"Gravitational radiations from periodic orbits around a black hole in the effective field theory extension of general relativity","ref_index":81,"is_internal_anchor":false},{"citing_arxiv_id":"2512.22728","citing_title":"Probing higher curvature gravity via ringdown with overtones","ref_index":36,"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":33,"is_internal_anchor":false},{"citing_arxiv_id":"2604.02214","citing_title":"Quadratic gravity corrections to scalar QNMs of rapidly rotating black holes","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11755","citing_title":"Ringing of rapidly rotating black holes in effective field theory","ref_index":49,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX","json":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX.json","graph_json":"https://pith.science/api/pith-number/QPMS7DCSR77AJRKEKT2GRS4YLX/graph.json","events_json":"https://pith.science/api/pith-number/QPMS7DCSR77AJRKEKT2GRS4YLX/events.json","paper":"https://pith.science/paper/QPMS7DCS"},"agent_actions":{"view_html":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX","download_json":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX.json","view_paper":"https://pith.science/paper/QPMS7DCS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2005.13923&json=true","fetch_graph":"https://pith.science/api/pith-number/QPMS7DCSR77AJRKEKT2GRS4YLX/graph.json","fetch_events":"https://pith.science/api/pith-number/QPMS7DCSR77AJRKEKT2GRS4YLX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX/action/storage_attestation","attest_author":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX/action/author_attestation","sign_citation":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX/action/citation_signature","submit_replication":"https://pith.science/pith/QPMS7DCSR77AJRKEKT2GRS4YLX/action/replication_record"}},"created_at":"2026-07-05T01:24:36.164582+00:00","updated_at":"2026-07-05T01:24:36.164582+00:00"}