{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1999:DWA2MDT4T5F7I5SNSGLUOPTGC3","short_pith_number":"pith:DWA2MDT4","schema_version":"1.0","canonical_sha256":"1d81a60e7c9f4bf4764d9197473e6616dc9155a2b55540d16cf82871f29dfea8","source":{"kind":"arxiv","id":"hep-ph/9904259","version":2},"attestation_state":"computed","paper":{"title":"Oscillation Solutions to Solar Neutrino Problem","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"V.Berezinsky","submitted_at":"1999-04-07T13:07:07Z","abstract_excerpt":"The current status of oscillation solutions to the Solar Neutrino Problem is reviewed. Four oscillation solutions are discussed in the light of 708d Superkamiokande data: MSW, Just-So VO, VO with Energy-Independent Suppression (EIS) and Resonant-Spin-Flavor-Precession (RSFP). Only EIS VO is strongly disfavoured by the global rates, mostly due to the Homestake data. Vacuum oscillations give an interesting solution which explains high-energy excess of events observed by Superkamiokande and predicts {\\em semi-annual} seasonal variation of $Be$-neutrino flux. There are indications to these variati"},"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":"hep-ph/9904259","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-ph","submitted_at":"1999-04-07T13:07:07Z","cross_cats_sorted":[],"title_canon_sha256":"101fb28e7b52564439717dfb00ed6b56e4fea73eb98b5ab13f66952ca6a68fa4","abstract_canon_sha256":"a8dc25c14893445cac8b485c7366fb1d9c42e27478a4b644ceb5dee8c4d5392a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:15:26.965031Z","signature_b64":"LKLh2ryuNjLXmWdgTRkSGHno7Uj1mj0xm8Cc24b32QYvaH4NqlJzU9K31zjMl9XkgkflAMc7VLjUJKwNDVKMDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1d81a60e7c9f4bf4764d9197473e6616dc9155a2b55540d16cf82871f29dfea8","last_reissued_at":"2026-05-18T04:15:26.964656Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:15:26.964656Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Oscillation Solutions to Solar Neutrino Problem","license":"","headline":"","cross_cats":[],"primary_cat":"hep-ph","authors_text":"V.Berezinsky","submitted_at":"1999-04-07T13:07:07Z","abstract_excerpt":"The current status of oscillation solutions to the Solar Neutrino Problem is reviewed. Four oscillation solutions are discussed in the light of 708d Superkamiokande data: MSW, Just-So VO, VO with Energy-Independent Suppression (EIS) and Resonant-Spin-Flavor-Precession (RSFP). Only EIS VO is strongly disfavoured by the global rates, mostly due to the Homestake data. Vacuum oscillations give an interesting solution which explains high-energy excess of events observed by Superkamiokande and predicts {\\em semi-annual} seasonal variation of $Be$-neutrino flux. There are indications to these variati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-ph/9904259","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":""},"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":"hep-ph/9904259","created_at":"2026-05-18T04:15:26.964710+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-ph/9904259v2","created_at":"2026-05-18T04:15:26.964710+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-ph/9904259","created_at":"2026-05-18T04:15:26.964710+00:00"},{"alias_kind":"pith_short_12","alias_value":"DWA2MDT4T5F7","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_16","alias_value":"DWA2MDT4T5F7I5SN","created_at":"2026-05-18T12:25:49.631198+00:00"},{"alias_kind":"pith_short_8","alias_value":"DWA2MDT4","created_at":"2026-05-18T12:25:49.631198+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/DWA2MDT4T5F7I5SNSGLUOPTGC3","json":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3.json","graph_json":"https://pith.science/api/pith-number/DWA2MDT4T5F7I5SNSGLUOPTGC3/graph.json","events_json":"https://pith.science/api/pith-number/DWA2MDT4T5F7I5SNSGLUOPTGC3/events.json","paper":"https://pith.science/paper/DWA2MDT4"},"agent_actions":{"view_html":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3","download_json":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3.json","view_paper":"https://pith.science/paper/DWA2MDT4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-ph/9904259&json=true","fetch_graph":"https://pith.science/api/pith-number/DWA2MDT4T5F7I5SNSGLUOPTGC3/graph.json","fetch_events":"https://pith.science/api/pith-number/DWA2MDT4T5F7I5SNSGLUOPTGC3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3/action/storage_attestation","attest_author":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3/action/author_attestation","sign_citation":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3/action/citation_signature","submit_replication":"https://pith.science/pith/DWA2MDT4T5F7I5SNSGLUOPTGC3/action/replication_record"}},"created_at":"2026-05-18T04:15:26.964710+00:00","updated_at":"2026-05-18T04:15:26.964710+00:00"}