{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:Z5GHH2KXLYAS4ENG2DCGGSDLPT","short_pith_number":"pith:Z5GHH2KX","schema_version":"1.0","canonical_sha256":"cf4c73e9575e012e11a6d0c463486b7cda6649465ca8b955ecabe54ea3fa8341","source":{"kind":"arxiv","id":"2203.02414","version":3},"attestation_state":"computed","paper":{"title":"Consequences of the Dresden-II reactor data for the weak mixing angle and new physics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex","nucl-ex","nucl-th"],"primary_cat":"hep-ph","authors_text":"D. Aristizabal Sierra, D. K. Papoulias, V. De Romeri","submitted_at":"2022-03-04T16:40:48Z","abstract_excerpt":"The Dresden-II reactor experiment has recently reported a suggestive evidence for the observation of coherent elastic neutrino-nucleus scattering, using a germanium detector. Given the low recoil energy threshold, these data are particularly interesting for a low-energy determination of the weak mixing angle and for the study of new physics leading to spectral distortions at low momentum transfer. Using two hypotheses for the quenching factor, we study the impact of the data on: (i) The weak mixing angle at a renormalization scale of $\\sim 10\\,\\text{MeV}$, (ii) neutrino generalized interaction"},"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":"2203.02414","kind":"arxiv","version":3},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-03-04T16:40:48Z","cross_cats_sorted":["hep-ex","nucl-ex","nucl-th"],"title_canon_sha256":"d855968d3b664efbf8354aa51116a70eaa53b7f633c89c31103b4547045cc4ae","abstract_canon_sha256":"be0d1bca789f00b2d65ff4e5b4a45a5f3df6bf1ffdcbf0ea965847fa57d8631c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:58:02.982836Z","signature_b64":"Qs9Yv9A8in8iUPtLdqKsINAxxDkTpBiRaZgjDy1VVW1/iBcrJ2vuB00MazXjHoouPxDYkI/9O7/fO7uS8JwWDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"cf4c73e9575e012e11a6d0c463486b7cda6649465ca8b955ecabe54ea3fa8341","last_reissued_at":"2026-07-05T04:58:02.982432Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:58:02.982432Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Consequences of the Dresden-II reactor data for the weak mixing angle and new physics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex","nucl-ex","nucl-th"],"primary_cat":"hep-ph","authors_text":"D. Aristizabal Sierra, D. K. Papoulias, V. De Romeri","submitted_at":"2022-03-04T16:40:48Z","abstract_excerpt":"The Dresden-II reactor experiment has recently reported a suggestive evidence for the observation of coherent elastic neutrino-nucleus scattering, using a germanium detector. Given the low recoil energy threshold, these data are particularly interesting for a low-energy determination of the weak mixing angle and for the study of new physics leading to spectral distortions at low momentum transfer. Using two hypotheses for the quenching factor, we study the impact of the data on: (i) The weak mixing angle at a renormalization scale of $\\sim 10\\,\\text{MeV}$, (ii) neutrino generalized interaction"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2203.02414","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/2203.02414/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":"2203.02414","created_at":"2026-07-05T04:58:02.982489+00:00"},{"alias_kind":"arxiv_version","alias_value":"2203.02414v3","created_at":"2026-07-05T04:58:02.982489+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2203.02414","created_at":"2026-07-05T04:58:02.982489+00:00"},{"alias_kind":"pith_short_12","alias_value":"Z5GHH2KXLYAS","created_at":"2026-07-05T04:58:02.982489+00:00"},{"alias_kind":"pith_short_16","alias_value":"Z5GHH2KXLYAS4ENG","created_at":"2026-07-05T04:58:02.982489+00:00"},{"alias_kind":"pith_short_8","alias_value":"Z5GHH2KX","created_at":"2026-07-05T04:58:02.982489+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.07975","citing_title":"Phenomenological implications of the high-precision COHERENT germanium CE$\\nu$NS data","ref_index":79,"is_internal_anchor":false},{"citing_arxiv_id":"2604.06002","citing_title":"Probing the Solar $^8$B Neutrino Fog with XENONnT","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT","json":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT.json","graph_json":"https://pith.science/api/pith-number/Z5GHH2KXLYAS4ENG2DCGGSDLPT/graph.json","events_json":"https://pith.science/api/pith-number/Z5GHH2KXLYAS4ENG2DCGGSDLPT/events.json","paper":"https://pith.science/paper/Z5GHH2KX"},"agent_actions":{"view_html":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT","download_json":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT.json","view_paper":"https://pith.science/paper/Z5GHH2KX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2203.02414&json=true","fetch_graph":"https://pith.science/api/pith-number/Z5GHH2KXLYAS4ENG2DCGGSDLPT/graph.json","fetch_events":"https://pith.science/api/pith-number/Z5GHH2KXLYAS4ENG2DCGGSDLPT/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT/action/timestamp_anchor","attest_storage":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT/action/storage_attestation","attest_author":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT/action/author_attestation","sign_citation":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT/action/citation_signature","submit_replication":"https://pith.science/pith/Z5GHH2KXLYAS4ENG2DCGGSDLPT/action/replication_record"}},"created_at":"2026-07-05T04:58:02.982489+00:00","updated_at":"2026-07-05T04:58:02.982489+00:00"}