{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:E22CNT7YYXDVLLW7TRBOFIAXHF","short_pith_number":"pith:E22CNT7Y","schema_version":"1.0","canonical_sha256":"26b426cff8c5c755aedf9c42e2a017394ff8431da751d07b40c027b3bcb9d8a8","source":{"kind":"arxiv","id":"1912.04309","version":2},"attestation_state":"computed","paper":{"title":"Physics potential of the ESS$\\nu$SB","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"E. Fernandez-Martinez, M. Blennow, S. Rosauro-Alcaraz, T. Ota","submitted_at":"2019-12-09T19:00:14Z","abstract_excerpt":"The ESS$\\nu$SB project proposes to base a neutrino ''Super Beam'' of unprecedented luminosity at the European Spallation Source. The original proposal identified the second peak of the oscillation probability as the optimal to maximize the discovery potential to leptonic CP violation. However this choice reduces the statistics at the detector and penalizes other complementary searches such as the determination of the atmospheric oscillation parameters, particularly the octant of $\\theta_{23}$ as well as the neutrino mass ordering. We explore how these shortcomings can be alleviated by the comb"},"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":"1912.04309","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2019-12-09T19:00:14Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"87f02169e72b9085906d7813f28e5b68906288a83cc86e174d4aa5c7a5d6c7ce","abstract_canon_sha256":"bb7a79060fc61986de156dd4d4b129afee51bbc320f3c76ea76e530aa97b3377"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T01:34:51.099070Z","signature_b64":"3YV9anz94xcfrZ/MFnFAJEoWUxJGasO7Oyjsi+61V3o4730sF5oqlu2TrC2NzgXmfTnj0u55B5Qje+yoDr57DA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"26b426cff8c5c755aedf9c42e2a017394ff8431da751d07b40c027b3bcb9d8a8","last_reissued_at":"2026-07-05T01:34:51.098583Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T01:34:51.098583Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Physics potential of the ESS$\\nu$SB","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"hep-ph","authors_text":"E. Fernandez-Martinez, M. Blennow, S. Rosauro-Alcaraz, T. Ota","submitted_at":"2019-12-09T19:00:14Z","abstract_excerpt":"The ESS$\\nu$SB project proposes to base a neutrino ''Super Beam'' of unprecedented luminosity at the European Spallation Source. The original proposal identified the second peak of the oscillation probability as the optimal to maximize the discovery potential to leptonic CP violation. However this choice reduces the statistics at the detector and penalizes other complementary searches such as the determination of the atmospheric oscillation parameters, particularly the octant of $\\theta_{23}$ as well as the neutrino mass ordering. We explore how these shortcomings can be alleviated by the comb"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1912.04309","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/1912.04309/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":"1912.04309","created_at":"2026-07-05T01:34:51.098644+00:00"},{"alias_kind":"arxiv_version","alias_value":"1912.04309v2","created_at":"2026-07-05T01:34:51.098644+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1912.04309","created_at":"2026-07-05T01:34:51.098644+00:00"},{"alias_kind":"pith_short_12","alias_value":"E22CNT7YYXDV","created_at":"2026-07-05T01:34:51.098644+00:00"},{"alias_kind":"pith_short_16","alias_value":"E22CNT7YYXDVLLW7","created_at":"2026-07-05T01:34:51.098644+00:00"},{"alias_kind":"pith_short_8","alias_value":"E22CNT7Y","created_at":"2026-07-05T01:34:51.098644+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2508.18103","citing_title":"Searching non-standard interactions with atmospheric neutrinos at ESSnuSB","ref_index":31,"is_internal_anchor":false},{"citing_arxiv_id":"2604.11774","citing_title":"Neutron Reconstruction via Blips in Liquid Argon Time Projection Chambers","ref_index":11,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF","json":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF.json","graph_json":"https://pith.science/api/pith-number/E22CNT7YYXDVLLW7TRBOFIAXHF/graph.json","events_json":"https://pith.science/api/pith-number/E22CNT7YYXDVLLW7TRBOFIAXHF/events.json","paper":"https://pith.science/paper/E22CNT7Y"},"agent_actions":{"view_html":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF","download_json":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF.json","view_paper":"https://pith.science/paper/E22CNT7Y","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1912.04309&json=true","fetch_graph":"https://pith.science/api/pith-number/E22CNT7YYXDVLLW7TRBOFIAXHF/graph.json","fetch_events":"https://pith.science/api/pith-number/E22CNT7YYXDVLLW7TRBOFIAXHF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF/action/storage_attestation","attest_author":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF/action/author_attestation","sign_citation":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF/action/citation_signature","submit_replication":"https://pith.science/pith/E22CNT7YYXDVLLW7TRBOFIAXHF/action/replication_record"}},"created_at":"2026-07-05T01:34:51.098644+00:00","updated_at":"2026-07-05T01:34:51.098644+00:00"}