{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2013:5NMBG2MT4BOSSH7EIGMVSD5TQP","short_pith_number":"pith:5NMBG2MT","schema_version":"1.0","canonical_sha256":"eb58136993e05d291fe44199590fb383ff676fbb6697207be8af6b0ac222dc59","source":{"kind":"arxiv","id":"1303.3294","version":2},"attestation_state":"computed","paper":{"title":"Exploring \\nu_\\tau - \\nu_s mixing with cascade events in DeepCore","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Arman Esmaili, Francis Halzen, O. L. G. Peres","submitted_at":"2013-03-13T21:27:20Z","abstract_excerpt":"The atmospheric neutrino data collected by the IceCube experiment and its low-energy extension DeepCore provide a unique opportunity to probe the neutrino sector of the Standard Model. In the low energy range the experiment have observed neutrino oscillations, and the high energy data are especially sensitive to signatures of new physics in the neutrino sector. In this context, we previously demonstrated the unmatched potential of the experiment to reveal the existence of light sterile neutrinos. The studies are routinely performed in the simplest 3+1 model concentrating on disappearance of mu"},"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":"1303.3294","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2013-03-13T21:27:20Z","cross_cats_sorted":["astro-ph.EP","astro-ph.HE","hep-ex"],"title_canon_sha256":"6306d38b97120d6d79910706926d184fd01d450b49ec4dd62aed0337425a63c7","abstract_canon_sha256":"7a7c10d1e638b59852dae612166618929985bb06090d355032024435dfc8213d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:16:06.103989Z","signature_b64":"eFYvPZ2hEq6/quSOePI1C3FN9J/ILY3phdcdoaMDrsT91hFld9EW1oay6hZs/qIrOmEwkoaQ2T1SY+cf6cHEDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eb58136993e05d291fe44199590fb383ff676fbb6697207be8af6b0ac222dc59","last_reissued_at":"2026-05-18T03:16:06.103337Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:16:06.103337Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Exploring \\nu_\\tau - \\nu_s mixing with cascade events in DeepCore","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.EP","astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Arman Esmaili, Francis Halzen, O. L. G. Peres","submitted_at":"2013-03-13T21:27:20Z","abstract_excerpt":"The atmospheric neutrino data collected by the IceCube experiment and its low-energy extension DeepCore provide a unique opportunity to probe the neutrino sector of the Standard Model. In the low energy range the experiment have observed neutrino oscillations, and the high energy data are especially sensitive to signatures of new physics in the neutrino sector. In this context, we previously demonstrated the unmatched potential of the experiment to reveal the existence of light sterile neutrinos. The studies are routinely performed in the simplest 3+1 model concentrating on disappearance of mu"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1303.3294","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":"1303.3294","created_at":"2026-05-18T03:16:06.103430+00:00"},{"alias_kind":"arxiv_version","alias_value":"1303.3294v2","created_at":"2026-05-18T03:16:06.103430+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1303.3294","created_at":"2026-05-18T03:16:06.103430+00:00"},{"alias_kind":"pith_short_12","alias_value":"5NMBG2MT4BOS","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_16","alias_value":"5NMBG2MT4BOSSH7E","created_at":"2026-05-18T12:27:34.582898+00:00"},{"alias_kind":"pith_short_8","alias_value":"5NMBG2MT","created_at":"2026-05-18T12:27:34.582898+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"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":108,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP","json":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP.json","graph_json":"https://pith.science/api/pith-number/5NMBG2MT4BOSSH7EIGMVSD5TQP/graph.json","events_json":"https://pith.science/api/pith-number/5NMBG2MT4BOSSH7EIGMVSD5TQP/events.json","paper":"https://pith.science/paper/5NMBG2MT"},"agent_actions":{"view_html":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP","download_json":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP.json","view_paper":"https://pith.science/paper/5NMBG2MT","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1303.3294&json=true","fetch_graph":"https://pith.science/api/pith-number/5NMBG2MT4BOSSH7EIGMVSD5TQP/graph.json","fetch_events":"https://pith.science/api/pith-number/5NMBG2MT4BOSSH7EIGMVSD5TQP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP/action/storage_attestation","attest_author":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP/action/author_attestation","sign_citation":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP/action/citation_signature","submit_replication":"https://pith.science/pith/5NMBG2MT4BOSSH7EIGMVSD5TQP/action/replication_record"}},"created_at":"2026-05-18T03:16:06.103430+00:00","updated_at":"2026-05-18T03:16:06.103430+00:00"}