{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:PKJ7UVLI7WQ43JTSGWH6Z3V6JA","short_pith_number":"pith:PKJ7UVLI","schema_version":"1.0","canonical_sha256":"7a93fa5568fda1cda672358feceebe48021c0f6adeb5ab7b8101650784c21f68","source":{"kind":"arxiv","id":"2109.03247","version":2},"attestation_state":"computed","paper":{"title":"Impact of COHERENT measurements, cross section uncertainties and new interactions on the neutrino floor","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. Aristizabal Sierra, D. K. Papoulias, L. J. Flores, V. De Romeri","submitted_at":"2021-09-07T18:00:01Z","abstract_excerpt":"We reconsider the discovery limit of multi-ton direct detection dark matter experiments in the light of recent measurements of the coherent elastic neutrino-nucleus scattering process. Assuming the cross section to be a parameter entirely determined by data, rather than using its Standard Model prediction, we use the COHERENT CsI and LAr data sets to determine WIMP discovery limits. Being based on a data-driven approach, the results are thus free from theoretical assumptions and fall within the WIMP mass regions where XENONnT and DARWIN have best expected sensitivities. We further determine th"},"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":"2109.03247","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2021-09-07T18:00:01Z","cross_cats_sorted":[],"title_canon_sha256":"ac5589b15b1bd0d7c6fae3883b66e13de28140dd4fcb3b483e0f167e97f363c0","abstract_canon_sha256":"2143508e7d7a742c86ffa4fb300094ee094a03fcf62d767d27ea49b926081f54"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:52:09.097534Z","signature_b64":"2vgJWbBYDzp4s4/A/8MBTGZ2r4cyv5GHW9OexpM+2EahBzqCZXEB6dYXmy2dNv7CZIxP8iuPepV3IPokZm2nBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7a93fa5568fda1cda672358feceebe48021c0f6adeb5ab7b8101650784c21f68","last_reissued_at":"2026-07-05T03:52:09.097046Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:52:09.097046Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Impact of COHERENT measurements, cross section uncertainties and new interactions on the neutrino floor","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"D. Aristizabal Sierra, D. K. Papoulias, L. J. Flores, V. De Romeri","submitted_at":"2021-09-07T18:00:01Z","abstract_excerpt":"We reconsider the discovery limit of multi-ton direct detection dark matter experiments in the light of recent measurements of the coherent elastic neutrino-nucleus scattering process. Assuming the cross section to be a parameter entirely determined by data, rather than using its Standard Model prediction, we use the COHERENT CsI and LAr data sets to determine WIMP discovery limits. Being based on a data-driven approach, the results are thus free from theoretical assumptions and fall within the WIMP mass regions where XENONnT and DARWIN have best expected sensitivities. We further determine th"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2109.03247","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/2109.03247/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":"2109.03247","created_at":"2026-07-05T03:52:09.097106+00:00"},{"alias_kind":"arxiv_version","alias_value":"2109.03247v2","created_at":"2026-07-05T03:52:09.097106+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2109.03247","created_at":"2026-07-05T03:52:09.097106+00:00"},{"alias_kind":"pith_short_12","alias_value":"PKJ7UVLI7WQ4","created_at":"2026-07-05T03:52:09.097106+00:00"},{"alias_kind":"pith_short_16","alias_value":"PKJ7UVLI7WQ43JTS","created_at":"2026-07-05T03:52:09.097106+00:00"},{"alias_kind":"pith_short_8","alias_value":"PKJ7UVLI","created_at":"2026-07-05T03:52:09.097106+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.13469","citing_title":"Simulations of 3-Dimensional Recoil Response to Coherent Elastic Neutrino-Nucleus Scattering Events in Directional Direct Dark Matter Detectors","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.29031","citing_title":"Twilight of the WIMP: Comprehensive Phenomenology of Electroweak Triplet Dark Matter","ref_index":76,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA","json":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA.json","graph_json":"https://pith.science/api/pith-number/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/graph.json","events_json":"https://pith.science/api/pith-number/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/events.json","paper":"https://pith.science/paper/PKJ7UVLI"},"agent_actions":{"view_html":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA","download_json":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA.json","view_paper":"https://pith.science/paper/PKJ7UVLI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2109.03247&json=true","fetch_graph":"https://pith.science/api/pith-number/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/graph.json","fetch_events":"https://pith.science/api/pith-number/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/action/storage_attestation","attest_author":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/action/author_attestation","sign_citation":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/action/citation_signature","submit_replication":"https://pith.science/pith/PKJ7UVLI7WQ43JTSGWH6Z3V6JA/action/replication_record"}},"created_at":"2026-07-05T03:52:09.097106+00:00","updated_at":"2026-07-05T03:52:09.097106+00:00"}