{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:K7MTWPLPCDTKBQIEOGKQGWINKO","short_pith_number":"pith:K7MTWPLP","schema_version":"1.0","canonical_sha256":"57d93b3d6f10e6a0c104719503590d53a8baf4a97592edf97c98c5a59ed01d97","source":{"kind":"arxiv","id":"1408.0310","version":3},"attestation_state":"computed","paper":{"title":"Improved Theory of Neutrino Oscillations in Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Leonard S. Kisslinger","submitted_at":"2014-08-01T21:38:50Z","abstract_excerpt":"This is revision of the S-Matrix theory of neutrino oscillations used for many years. We evaluate the transition probability of a $\\mu$ to $e$ neutrino without an approximation used for many theoretical studies, and find important differences which could improve the extraction of neutrino parameters from experimental data in the future."},"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":"1408.0310","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2014-08-01T21:38:50Z","cross_cats_sorted":[],"title_canon_sha256":"e7881dac3587bdad180a6268623bc13ce139d88e6fd8c8a45bf91659430cf9d3","abstract_canon_sha256":"0fb70e27ad4a15dde638243695f22527361cda2b11d2d9ab08a7b94bc1de2558"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:29:45.436360Z","signature_b64":"J9OdvKD3RqIHEMqNXoByhmqNz5/eT6eBmXwHF+8u6CXrEVnZVXTubsPZ1IOZLmTypOhTOtQ+EFzD4+8cxtALBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"57d93b3d6f10e6a0c104719503590d53a8baf4a97592edf97c98c5a59ed01d97","last_reissued_at":"2026-05-18T02:29:45.435926Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:29:45.435926Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Improved Theory of Neutrino Oscillations in Matter","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"Leonard S. Kisslinger","submitted_at":"2014-08-01T21:38:50Z","abstract_excerpt":"This is revision of the S-Matrix theory of neutrino oscillations used for many years. We evaluate the transition probability of a $\\mu$ to $e$ neutrino without an approximation used for many theoretical studies, and find important differences which could improve the extraction of neutrino parameters from experimental data in the future."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1408.0310","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":""},"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":"1408.0310","created_at":"2026-05-18T02:29:45.435986+00:00"},{"alias_kind":"arxiv_version","alias_value":"1408.0310v3","created_at":"2026-05-18T02:29:45.435986+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1408.0310","created_at":"2026-05-18T02:29:45.435986+00:00"},{"alias_kind":"pith_short_12","alias_value":"K7MTWPLPCDTK","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_16","alias_value":"K7MTWPLPCDTKBQIE","created_at":"2026-05-18T12:28:35.611951+00:00"},{"alias_kind":"pith_short_8","alias_value":"K7MTWPLP","created_at":"2026-05-18T12:28:35.611951+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO","json":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO.json","graph_json":"https://pith.science/api/pith-number/K7MTWPLPCDTKBQIEOGKQGWINKO/graph.json","events_json":"https://pith.science/api/pith-number/K7MTWPLPCDTKBQIEOGKQGWINKO/events.json","paper":"https://pith.science/paper/K7MTWPLP"},"agent_actions":{"view_html":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO","download_json":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO.json","view_paper":"https://pith.science/paper/K7MTWPLP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1408.0310&json=true","fetch_graph":"https://pith.science/api/pith-number/K7MTWPLPCDTKBQIEOGKQGWINKO/graph.json","fetch_events":"https://pith.science/api/pith-number/K7MTWPLPCDTKBQIEOGKQGWINKO/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO/action/timestamp_anchor","attest_storage":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO/action/storage_attestation","attest_author":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO/action/author_attestation","sign_citation":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO/action/citation_signature","submit_replication":"https://pith.science/pith/K7MTWPLPCDTKBQIEOGKQGWINKO/action/replication_record"}},"created_at":"2026-05-18T02:29:45.435986+00:00","updated_at":"2026-05-18T02:29:45.435986+00:00"}