{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:J2JAP3DN3EXAGPBVJOFGKJFQFD","short_pith_number":"pith:J2JAP3DN","schema_version":"1.0","canonical_sha256":"4e9207ec6dd92e033c354b8a6524b028c14c013954fedea645f3b8d8575b81f8","source":{"kind":"arxiv","id":"2202.00694","version":1},"attestation_state":"computed","paper":{"title":"IceCube and High-Energy Cosmic Neutrinos","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Ali Kheirandish, Francis Halzen","submitted_at":"2022-02-01T19:00:03Z","abstract_excerpt":"The IceCube experiment discovered PeV-energy neutrinos originating beyond our Galaxy with an energy flux that is comparable to that of TeV-energy gamma rays and EeV-energy cosmic rays. Neutrinos provide the only unobstructed view of the cosmic accelerators that power the highest energy radiation reaching us from the universe. We will review the rationale for building kilometer-scale neutrino detectors that led to the IceCube project, which transformed a cubic kilometer of deep transparent natural Antarctic ice into a neutrino telescope of such a scale. We will summarize the results from the fi"},"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":"2202.00694","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/publicdomain/zero/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-02-01T19:00:03Z","cross_cats_sorted":["hep-ex","hep-ph"],"title_canon_sha256":"375d5598646f07701c84ac61a657a91722c740c974337f3fa8da710d3125cbd1","abstract_canon_sha256":"57ffec77bea0889eb9c76c9c4dfa4c9d2bdad026b2b41c075bf7f32362cd9256"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:53:26.534284Z","signature_b64":"YUvm1Fp0lbcvTQSySpo5XA7+fqVMLRE516FRXv+XMjZTNu/tnXH0+3FayFaMfMiVf985k3FmwV7CRzR3UH8bCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4e9207ec6dd92e033c354b8a6524b028c14c013954fedea645f3b8d8575b81f8","last_reissued_at":"2026-07-05T03:53:26.533847Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:53:26.533847Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"IceCube and High-Energy Cosmic Neutrinos","license":"http://creativecommons.org/publicdomain/zero/1.0/","headline":"","cross_cats":["hep-ex","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Ali Kheirandish, Francis Halzen","submitted_at":"2022-02-01T19:00:03Z","abstract_excerpt":"The IceCube experiment discovered PeV-energy neutrinos originating beyond our Galaxy with an energy flux that is comparable to that of TeV-energy gamma rays and EeV-energy cosmic rays. Neutrinos provide the only unobstructed view of the cosmic accelerators that power the highest energy radiation reaching us from the universe. We will review the rationale for building kilometer-scale neutrino detectors that led to the IceCube project, which transformed a cubic kilometer of deep transparent natural Antarctic ice into a neutrino telescope of such a scale. We will summarize the results from the fi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2202.00694","kind":"arxiv","version":1},"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/2202.00694/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":"2202.00694","created_at":"2026-07-05T03:53:26.533903+00:00"},{"alias_kind":"arxiv_version","alias_value":"2202.00694v1","created_at":"2026-07-05T03:53:26.533903+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2202.00694","created_at":"2026-07-05T03:53:26.533903+00:00"},{"alias_kind":"pith_short_12","alias_value":"J2JAP3DN3EXA","created_at":"2026-07-05T03:53:26.533903+00:00"},{"alias_kind":"pith_short_16","alias_value":"J2JAP3DN3EXAGPBV","created_at":"2026-07-05T03:53:26.533903+00:00"},{"alias_kind":"pith_short_8","alias_value":"J2JAP3DN","created_at":"2026-07-05T03:53:26.533903+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2602.20969","citing_title":"Turbulent AGN coronae as the origin of diffuse neutrinos up to PeV energies","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13968","citing_title":"Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes","ref_index":13,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD","json":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD.json","graph_json":"https://pith.science/api/pith-number/J2JAP3DN3EXAGPBVJOFGKJFQFD/graph.json","events_json":"https://pith.science/api/pith-number/J2JAP3DN3EXAGPBVJOFGKJFQFD/events.json","paper":"https://pith.science/paper/J2JAP3DN"},"agent_actions":{"view_html":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD","download_json":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD.json","view_paper":"https://pith.science/paper/J2JAP3DN","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2202.00694&json=true","fetch_graph":"https://pith.science/api/pith-number/J2JAP3DN3EXAGPBVJOFGKJFQFD/graph.json","fetch_events":"https://pith.science/api/pith-number/J2JAP3DN3EXAGPBVJOFGKJFQFD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD/action/storage_attestation","attest_author":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD/action/author_attestation","sign_citation":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD/action/citation_signature","submit_replication":"https://pith.science/pith/J2JAP3DN3EXAGPBVJOFGKJFQFD/action/replication_record"}},"created_at":"2026-07-05T03:53:26.533903+00:00","updated_at":"2026-07-05T03:53:26.533903+00:00"}