{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:IVL45A63ICH7RHIQZXKTBJACLA","short_pith_number":"pith:IVL45A63","schema_version":"1.0","canonical_sha256":"4557ce83db408ff89d10cdd530a4025821de72fcff4f20d4266e1adfe26d070a","source":{"kind":"arxiv","id":"2112.05031","version":2},"attestation_state":"computed","paper":{"title":"A cautionary case of casual causality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Andrew J. Tolley, Aoibheann Margalit, Calvin Y.-R. Chen, Claudia de Rham","submitted_at":"2021-12-09T16:47:06Z","abstract_excerpt":"We distinguish between the notions of asymptotic causality and infrared causality for gravitational effective field theories, and show that the latter gives constraints consistent with gravitational positivity bounds. We re-explore the scattering of gravitational waves in a spherically symmetric background in the EFT of gravity in $D\\ge 5$, for which the leading-order correction to Einstein gravity is determined by the Gauss-Bonnet operator. We reproduce the known result that the truncated effective theory exhibits apparent time advances relative to the background geometry for specific polaris"},"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":"2112.05031","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2021-12-09T16:47:06Z","cross_cats_sorted":["astro-ph.CO","gr-qc"],"title_canon_sha256":"2a3d2eed15c83986ab57e370490130717f495a21965cf490ad9f6ce0e37c3511","abstract_canon_sha256":"8072456c3650ede323d70af39fa8cc8eb116c13fdd5cb90f8a0e20bcabfbf150"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:07:29.107987Z","signature_b64":"O59PW8sDyTRUXscvz1DyBPTXwFlr0fKfYSmtXswTkzoC2ga+rUetiOQlBgpaWHeMYyJRiptJS8oSzbEjyJxYBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4557ce83db408ff89d10cdd530a4025821de72fcff4f20d4266e1adfe26d070a","last_reissued_at":"2026-07-05T04:07:29.107508Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:07:29.107508Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A cautionary case of casual causality","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc"],"primary_cat":"hep-th","authors_text":"Andrew J. Tolley, Aoibheann Margalit, Calvin Y.-R. Chen, Claudia de Rham","submitted_at":"2021-12-09T16:47:06Z","abstract_excerpt":"We distinguish between the notions of asymptotic causality and infrared causality for gravitational effective field theories, and show that the latter gives constraints consistent with gravitational positivity bounds. We re-explore the scattering of gravitational waves in a spherically symmetric background in the EFT of gravity in $D\\ge 5$, for which the leading-order correction to Einstein gravity is determined by the Gauss-Bonnet operator. We reproduce the known result that the truncated effective theory exhibits apparent time advances relative to the background geometry for specific polaris"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2112.05031","kind":"arxiv","version":2},"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/2112.05031/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":"2112.05031","created_at":"2026-07-05T04:07:29.107565+00:00"},{"alias_kind":"arxiv_version","alias_value":"2112.05031v2","created_at":"2026-07-05T04:07:29.107565+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2112.05031","created_at":"2026-07-05T04:07:29.107565+00:00"},{"alias_kind":"pith_short_12","alias_value":"IVL45A63ICH7","created_at":"2026-07-05T04:07:29.107565+00:00"},{"alias_kind":"pith_short_16","alias_value":"IVL45A63ICH7RHIQ","created_at":"2026-07-05T04:07:29.107565+00:00"},{"alias_kind":"pith_short_8","alias_value":"IVL45A63","created_at":"2026-07-05T04:07:29.107565+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.05319","citing_title":"Non-linear evolution of five-dimensional black strings in effective field theory","ref_index":30,"is_internal_anchor":false},{"citing_arxiv_id":"2605.00089","citing_title":"On the Asymptotic Causal Structure in Gravitational EFTs","ref_index":15,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA","json":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA.json","graph_json":"https://pith.science/api/pith-number/IVL45A63ICH7RHIQZXKTBJACLA/graph.json","events_json":"https://pith.science/api/pith-number/IVL45A63ICH7RHIQZXKTBJACLA/events.json","paper":"https://pith.science/paper/IVL45A63"},"agent_actions":{"view_html":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA","download_json":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA.json","view_paper":"https://pith.science/paper/IVL45A63","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2112.05031&json=true","fetch_graph":"https://pith.science/api/pith-number/IVL45A63ICH7RHIQZXKTBJACLA/graph.json","fetch_events":"https://pith.science/api/pith-number/IVL45A63ICH7RHIQZXKTBJACLA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA/action/storage_attestation","attest_author":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA/action/author_attestation","sign_citation":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA/action/citation_signature","submit_replication":"https://pith.science/pith/IVL45A63ICH7RHIQZXKTBJACLA/action/replication_record"}},"created_at":"2026-07-05T04:07:29.107565+00:00","updated_at":"2026-07-05T04:07:29.107565+00:00"}