{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:53BACX74HCF7ISZQLRD6LHEKUX","short_pith_number":"pith:53BACX74","schema_version":"1.0","canonical_sha256":"eec2015ffc388bf44b305c47e59c8aa5d4a028e2433ab58dd05d40ba97b40050","source":{"kind":"arxiv","id":"2212.06978","version":1},"attestation_state":"computed","paper":{"title":"Non-adiabatic Level Crossing in Resonant Neutrino Oscillations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Stephen J. Parke","submitted_at":"2022-12-14T02:09:16Z","abstract_excerpt":"Analytic results are presented for the probability of detecting an electron neutrino after passage through a resonant oscillation region. If the electron neutrino is produced far above the resonance density, this probability is simply given by $\\langle \\,P_{\\nu_e} \\, \\rangle \\approx \\sin^2 \\theta_0+ P_\\text{x} \\cos 2 \\theta_0$, where $\\theta_0$ is the vacuum mixing angle. The probability is averaged over the production as well as the detection positions of the neutrino and $P_\\text{x} $ is the Landau-Zener transition probability between adiabatic states. Finally, this result is applied to reso"},"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":"2212.06978","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2022-12-14T02:09:16Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"299724dcb98cc6b2407c27d888028089a33ad5a03274d41b94ad44ace3e061ae","abstract_canon_sha256":"1acaf975b782c445f61088e751fa42a266161ab45bd3ef8146df090e186cd58d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:25:19.571710Z","signature_b64":"vgN2Y3Kr/ltOA7MUPNcz83c6c6sCujvLlBi7bT1+ZKd8t5bZccDhN7TjU7pSAudqmdNwlx+txnd96HTSsGWoCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eec2015ffc388bf44b305c47e59c8aa5d4a028e2433ab58dd05d40ba97b40050","last_reissued_at":"2026-07-05T05:25:19.571350Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:25:19.571350Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-adiabatic Level Crossing in Resonant Neutrino Oscillations","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"Stephen J. Parke","submitted_at":"2022-12-14T02:09:16Z","abstract_excerpt":"Analytic results are presented for the probability of detecting an electron neutrino after passage through a resonant oscillation region. If the electron neutrino is produced far above the resonance density, this probability is simply given by $\\langle \\,P_{\\nu_e} \\, \\rangle \\approx \\sin^2 \\theta_0+ P_\\text{x} \\cos 2 \\theta_0$, where $\\theta_0$ is the vacuum mixing angle. The probability is averaged over the production as well as the detection positions of the neutrino and $P_\\text{x} $ is the Landau-Zener transition probability between adiabatic states. Finally, this result is applied to reso"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2212.06978","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/2212.06978/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":"2212.06978","created_at":"2026-07-05T05:25:19.571412+00:00"},{"alias_kind":"arxiv_version","alias_value":"2212.06978v1","created_at":"2026-07-05T05:25:19.571412+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2212.06978","created_at":"2026-07-05T05:25:19.571412+00:00"},{"alias_kind":"pith_short_12","alias_value":"53BACX74HCF7","created_at":"2026-07-05T05:25:19.571412+00:00"},{"alias_kind":"pith_short_16","alias_value":"53BACX74HCF7ISZQ","created_at":"2026-07-05T05:25:19.571412+00:00"},{"alias_kind":"pith_short_8","alias_value":"53BACX74","created_at":"2026-07-05T05:25:19.571412+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.18337","citing_title":"Standard Candles for Supernova Neutrino Detection at DUNE","ref_index":53,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX","json":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX.json","graph_json":"https://pith.science/api/pith-number/53BACX74HCF7ISZQLRD6LHEKUX/graph.json","events_json":"https://pith.science/api/pith-number/53BACX74HCF7ISZQLRD6LHEKUX/events.json","paper":"https://pith.science/paper/53BACX74"},"agent_actions":{"view_html":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX","download_json":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX.json","view_paper":"https://pith.science/paper/53BACX74","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2212.06978&json=true","fetch_graph":"https://pith.science/api/pith-number/53BACX74HCF7ISZQLRD6LHEKUX/graph.json","fetch_events":"https://pith.science/api/pith-number/53BACX74HCF7ISZQLRD6LHEKUX/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX/action/timestamp_anchor","attest_storage":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX/action/storage_attestation","attest_author":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX/action/author_attestation","sign_citation":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX/action/citation_signature","submit_replication":"https://pith.science/pith/53BACX74HCF7ISZQLRD6LHEKUX/action/replication_record"}},"created_at":"2026-07-05T05:25:19.571412+00:00","updated_at":"2026-07-05T05:25:19.571412+00:00"}