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The CC reaction is sensitive exclusively to nu_e's, while the ES reaction also has a small sensitivity to nu_mu's and nu_tau's. The flux of nu_e's from ^8B decay measured by the CC reaction rate is\n  \\phi^CC(nu_e) = 1.75 +/- 0.07 (stat)+0.12/-0.11 (sys.) +/- 0.05(theor) x 10^6 /cm^2 s.\n  Assuming no flavor transformation, the flux inferred from the ES reaction rate is\n  \\phi^ES(nu_x) = 2.39+/-0.3"},"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":"nucl-ex/0106015","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"nucl-ex","submitted_at":"2001-06-18T16:22:42Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"dfb30baa8d4305ecc9323c789097d4e356164a6fd15aca1dfbdd7dac4cf7fd3d","abstract_canon_sha256":"3e6a5397d1caed707b87e59f251c1d540654e90e5326b1e8bb48d421626626d1"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:47:10.428270Z","signature_b64":"8IYlG1idE7Ef6sVI/ydpUfn95+7/aeHUuqp58wzJmlJuHU6c1ZB2GzkOmQTJHn+mwfA88VtcF7oz5ZXgt+DrCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"42270b75b1da8c8c11d628a2dd176dfffafcc64ec6196ad6e9e893d17bcdf982","last_reissued_at":"2026-05-18T03:47:10.427786Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:47:10.427786Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Measurement of the rate of nu_e + d --> p + p + e^- interactions produced by 8B solar neutrinos at the Sudbury Neutrino Observatory","license":"","headline":"","cross_cats":["hep-ex"],"primary_cat":"nucl-ex","authors_text":"SNO Collaboration","submitted_at":"2001-06-18T16:22:42Z","abstract_excerpt":"Solar neutrinos from the decay of $^8$B have been detected at the Sudbury Neutrino Observatory (SNO) via the charged current (CC) reaction on deuterium and by the elastic scattering (ES) of electrons. The CC reaction is sensitive exclusively to nu_e's, while the ES reaction also has a small sensitivity to nu_mu's and nu_tau's. The flux of nu_e's from ^8B decay measured by the CC reaction rate is\n  \\phi^CC(nu_e) = 1.75 +/- 0.07 (stat)+0.12/-0.11 (sys.) +/- 0.05(theor) x 10^6 /cm^2 s.\n  Assuming no flavor transformation, the flux inferred from the ES reaction rate is\n  \\phi^ES(nu_x) = 2.39+/-0.3"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"nucl-ex/0106015","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":"nucl-ex/0106015","created_at":"2026-05-18T03:47:10.427861+00:00"},{"alias_kind":"arxiv_version","alias_value":"nucl-ex/0106015v2","created_at":"2026-05-18T03:47:10.427861+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.nucl-ex/0106015","created_at":"2026-05-18T03:47:10.427861+00:00"},{"alias_kind":"pith_short_12","alias_value":"IITQW5NR3KGI","created_at":"2026-05-18T12:25:50.254431+00:00"},{"alias_kind":"pith_short_16","alias_value":"IITQW5NR3KGIYEOW","created_at":"2026-05-18T12:25:50.254431+00:00"},{"alias_kind":"pith_short_8","alias_value":"IITQW5NR","created_at":"2026-05-18T12:25:50.254431+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2303.02358","citing_title":"Equal Majorana Phases from a Minimal and Predictive Neutrino Texture","ref_index":2,"is_internal_anchor":true},{"citing_arxiv_id":"2504.13259","citing_title":"The $\\beta$-decay spectrum of Tritiated graphene: combining nuclear quantum mechanics with Density Functional Theory","ref_index":2,"is_internal_anchor":true},{"citing_arxiv_id":"2605.18154","citing_title":"The Triadic Texture: Neutrino Predictions, Viable Vacuum, and Phenomenological Constraints","ref_index":1,"is_internal_anchor":true},{"citing_arxiv_id":"2507.07176","citing_title":"Amplifying muon-to-positron conversion in nuclei with ultralight dark matter","ref_index":7,"is_internal_anchor":true},{"citing_arxiv_id":"2512.24215","citing_title":"Neutrino Mass, Vacuum Stability and Higgs Inflation with Vector-Like Quarks and a Single Right-Handed Neutrino","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2605.10424","citing_title":"Quantum Correlations of Neutrinos in the Kerr-Newman Space-time","ref_index":4,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14504","citing_title":"Forecasting neutrino mass constraints from the Nancy Grace Roman Space Telescope","ref_index":6,"is_internal_anchor":false},{"citing_arxiv_id":"2604.16157","citing_title":"$\\delta_{\\rm CP}$-free constraints on NSI parameters $\\varepsilon_{e\\mu}$ and $\\varepsilon_{e\\tau}$ using high-purity $\\nu_\\mu\\,{\\rm CC}$ events at IceCube DeepCore","ref_index":2,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77","json":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77.json","graph_json":"https://pith.science/api/pith-number/IITQW5NR3KGIYEOWFCRN2F3N77/graph.json","events_json":"https://pith.science/api/pith-number/IITQW5NR3KGIYEOWFCRN2F3N77/events.json","paper":"https://pith.science/paper/IITQW5NR"},"agent_actions":{"view_html":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77","download_json":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77.json","view_paper":"https://pith.science/paper/IITQW5NR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=nucl-ex/0106015&json=true","fetch_graph":"https://pith.science/api/pith-number/IITQW5NR3KGIYEOWFCRN2F3N77/graph.json","fetch_events":"https://pith.science/api/pith-number/IITQW5NR3KGIYEOWFCRN2F3N77/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77/action/storage_attestation","attest_author":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77/action/author_attestation","sign_citation":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77/action/citation_signature","submit_replication":"https://pith.science/pith/IITQW5NR3KGIYEOWFCRN2F3N77/action/replication_record"}},"created_at":"2026-05-18T03:47:10.427861+00:00","updated_at":"2026-05-18T03:47:10.427861+00:00"}