{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:QV7OY7QAKQTAZGENHPLRKNFJMC","short_pith_number":"pith:QV7OY7QA","schema_version":"1.0","canonical_sha256":"857eec7e0054260c988d3bd71534a960b975fe0d86b1e79d9a9d4bbd4f850c50","source":{"kind":"arxiv","id":"1909.10478","version":2},"attestation_state":"computed","paper":{"title":"Neutrino Oscillations in Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Eung Jin Chun, Jongkuk Kim, Ki-Young Choi","submitted_at":"2019-09-23T16:58:14Z","abstract_excerpt":"We study neutrino oscillations in a medium of dark matter which generalizes the standard matter effect. A general formula is derived to describe the effect of various mediums and their mediators to neutrinos. Neutrinos and anti-neutrinos receive opposite contributions from asymmetric distribution of (dark) matter and anti-matter, and thus it could appear in precision measurement of neutrino or anti-neutrino oscillations. Furthermore, the standard neutrino oscillation can occur from the symmetric dark matter effect even for massless neutrinos."},"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":"1909.10478","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-09-23T16:58:14Z","cross_cats_sorted":["astro-ph.HE","hep-ex"],"title_canon_sha256":"8374a8d3a37567406ff3a312daa35c0e3d69e78e373dcbf14086e0a37410cd19","abstract_canon_sha256":"a60f81363f363a2ccfeda1501932417ab0058962f1d1810cd9b9dba95ff507f8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:10:04.316042Z","signature_b64":"JN+ScOY1ACkP3pSEZc7ybHZfUGJW7nozW6HtO4LyygpRRwHm0wHQdQd0iVd16LIEGGQ1F7tg+gX6pvBp5/vcDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"857eec7e0054260c988d3bd71534a960b975fe0d86b1e79d9a9d4bbd4f850c50","last_reissued_at":"2026-07-05T00:10:04.315602Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:10:04.315602Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino Oscillations in Dark Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Eung Jin Chun, Jongkuk Kim, Ki-Young Choi","submitted_at":"2019-09-23T16:58:14Z","abstract_excerpt":"We study neutrino oscillations in a medium of dark matter which generalizes the standard matter effect. A general formula is derived to describe the effect of various mediums and their mediators to neutrinos. Neutrinos and anti-neutrinos receive opposite contributions from asymmetric distribution of (dark) matter and anti-matter, and thus it could appear in precision measurement of neutrino or anti-neutrino oscillations. Furthermore, the standard neutrino oscillation can occur from the symmetric dark matter effect even for massless neutrinos."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1909.10478","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/1909.10478/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":"1909.10478","created_at":"2026-07-05T00:10:04.315658+00:00"},{"alias_kind":"arxiv_version","alias_value":"1909.10478v2","created_at":"2026-07-05T00:10:04.315658+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1909.10478","created_at":"2026-07-05T00:10:04.315658+00:00"},{"alias_kind":"pith_short_12","alias_value":"QV7OY7QAKQTA","created_at":"2026-07-05T00:10:04.315658+00:00"},{"alias_kind":"pith_short_16","alias_value":"QV7OY7QAKQTAZGEN","created_at":"2026-07-05T00:10:04.315658+00:00"},{"alias_kind":"pith_short_8","alias_value":"QV7OY7QA","created_at":"2026-07-05T00:10:04.315658+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2508.10983","citing_title":"Shedding light on dark matter spikes through refractive neutrino masses","ref_index":3,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15146","citing_title":"Effective Matter Flavor Conversion Mediated by Pseudo-Sterile States as the Possible Origin of Neutrino Oscillation Anomalies","ref_index":117,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC","json":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC.json","graph_json":"https://pith.science/api/pith-number/QV7OY7QAKQTAZGENHPLRKNFJMC/graph.json","events_json":"https://pith.science/api/pith-number/QV7OY7QAKQTAZGENHPLRKNFJMC/events.json","paper":"https://pith.science/paper/QV7OY7QA"},"agent_actions":{"view_html":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC","download_json":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC.json","view_paper":"https://pith.science/paper/QV7OY7QA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1909.10478&json=true","fetch_graph":"https://pith.science/api/pith-number/QV7OY7QAKQTAZGENHPLRKNFJMC/graph.json","fetch_events":"https://pith.science/api/pith-number/QV7OY7QAKQTAZGENHPLRKNFJMC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC/action/storage_attestation","attest_author":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC/action/author_attestation","sign_citation":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC/action/citation_signature","submit_replication":"https://pith.science/pith/QV7OY7QAKQTAZGENHPLRKNFJMC/action/replication_record"}},"created_at":"2026-07-05T00:10:04.315658+00:00","updated_at":"2026-07-05T00:10:04.315658+00:00"}