{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:XX6U4DL7CSZ5UQMAGR2POPPONZ","short_pith_number":"pith:XX6U4DL7","schema_version":"1.0","canonical_sha256":"bdfd4e0d7f14b3da41803474f73dee6e630e6e2798bde6a3cf2dd0e7847b9811","source":{"kind":"arxiv","id":"1806.05696","version":1},"attestation_state":"computed","paper":{"title":"Probing Particle Physics with IceCube","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.HE","authors_text":"Carlos P\\'erez de los Heros, Klaus Helbing, Markus Ahlers","submitted_at":"2018-06-14T18:12:00Z","abstract_excerpt":"The IceCube observatory located at the South Pole is a cubic-kilometre optical Cherenkov telescope primarily designed for the detection of high-energy astrophysical neutrinos. IceCube became fully operational in 2010, after a seven-year construction phase, and reached a milestone in 2013 by the first observation of cosmic neutrinos in the TeV-PeV energy range. This observation does not only mark an important breakthrough in neutrino astronomy, but it also provides a new probe of particle physics related to neutrino production, mixing, and interaction. In this review we give an overview of the "},"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":"1806.05696","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2018-06-14T18:12:00Z","cross_cats_sorted":["hep-ex"],"title_canon_sha256":"b12d26aac22f41f17bc5a9c353c8e5a6d8bdf5a7ee4430b88f44e045d52d6fe0","abstract_canon_sha256":"b01dba8c1a2f2c5ab4d420f88299b9f77ce0655872ba61a2aa6fd676d0b70a37"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:00:30.161946Z","signature_b64":"5Uxh6nA8yfSXgkmaUGlfKaXTd5TBKoO7+aGT40/1krKc1ZALuJlXNv6TfP5XpWvXVVUG3UbNevJCOgwjZa4dBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"bdfd4e0d7f14b3da41803474f73dee6e630e6e2798bde6a3cf2dd0e7847b9811","last_reissued_at":"2026-05-18T00:00:30.161400Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:00:30.161400Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probing Particle Physics with IceCube","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex"],"primary_cat":"astro-ph.HE","authors_text":"Carlos P\\'erez de los Heros, Klaus Helbing, Markus Ahlers","submitted_at":"2018-06-14T18:12:00Z","abstract_excerpt":"The IceCube observatory located at the South Pole is a cubic-kilometre optical Cherenkov telescope primarily designed for the detection of high-energy astrophysical neutrinos. IceCube became fully operational in 2010, after a seven-year construction phase, and reached a milestone in 2013 by the first observation of cosmic neutrinos in the TeV-PeV energy range. This observation does not only mark an important breakthrough in neutrino astronomy, but it also provides a new probe of particle physics related to neutrino production, mixing, and interaction. In this review we give an overview of the "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1806.05696","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":""},"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":"1806.05696","created_at":"2026-05-18T00:00:30.161494+00:00"},{"alias_kind":"arxiv_version","alias_value":"1806.05696v1","created_at":"2026-05-18T00:00:30.161494+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1806.05696","created_at":"2026-05-18T00:00:30.161494+00:00"},{"alias_kind":"pith_short_12","alias_value":"XX6U4DL7CSZ5","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_16","alias_value":"XX6U4DL7CSZ5UQMA","created_at":"2026-05-18T12:33:04.347982+00:00"},{"alias_kind":"pith_short_8","alias_value":"XX6U4DL7","created_at":"2026-05-18T12:33:04.347982+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"1907.08690","citing_title":"Fundamental physics with high-energy cosmic neutrinos today and in the future","ref_index":3,"is_internal_anchor":true},{"citing_arxiv_id":"2502.09538","citing_title":"Neutrino Masses and Phenomenology in Nnaturalness","ref_index":41,"is_internal_anchor":true},{"citing_arxiv_id":"2604.12521","citing_title":"POLARIS: A Sparse Radial Neutrino Telescope Design for the Pacific Ocean","ref_index":1,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14409","citing_title":"Astrophysical bounds on the high-energy evolution of neutrino mixing","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ","json":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ.json","graph_json":"https://pith.science/api/pith-number/XX6U4DL7CSZ5UQMAGR2POPPONZ/graph.json","events_json":"https://pith.science/api/pith-number/XX6U4DL7CSZ5UQMAGR2POPPONZ/events.json","paper":"https://pith.science/paper/XX6U4DL7"},"agent_actions":{"view_html":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ","download_json":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ.json","view_paper":"https://pith.science/paper/XX6U4DL7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1806.05696&json=true","fetch_graph":"https://pith.science/api/pith-number/XX6U4DL7CSZ5UQMAGR2POPPONZ/graph.json","fetch_events":"https://pith.science/api/pith-number/XX6U4DL7CSZ5UQMAGR2POPPONZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ/action/storage_attestation","attest_author":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ/action/author_attestation","sign_citation":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ/action/citation_signature","submit_replication":"https://pith.science/pith/XX6U4DL7CSZ5UQMAGR2POPPONZ/action/replication_record"}},"created_at":"2026-05-18T00:00:30.161494+00:00","updated_at":"2026-05-18T00:00:30.161494+00:00"}