{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:AF2WOG6NPUGAX54J7SXIL25XY3","short_pith_number":"pith:AF2WOG6N","schema_version":"1.0","canonical_sha256":"0175671bcd7d0c0bf789fcae85ebb7c6c158d9bba8365400670ebc384d4b6917","source":{"kind":"arxiv","id":"1704.04027","version":3},"attestation_state":"computed","paper":{"title":"Constraining the Mass Scale of a Lorentz-Violating Hamiltonian with the Measurement of Astrophysical Neutrino-Flavor Composition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Guey-Lin Lin, Kwang-Chang Lai, Wei-Hao Lai","submitted_at":"2017-04-13T08:19:30Z","abstract_excerpt":"We study Lorentz violation effects on flavor transitions of high energy astrophysical neutrinos. It is shown that the appearance of Lorentz violating Hamiltonian can drastically change the flavor transition probabilities of astrophysical neutrinos. Predictions of Lorentz violation effects on flavor compositions of astrophysical neutrinos arriving on Earth are compared with IceCube flavor composition measurement which analyzes astrophysical neutrino events in the energy range between $25~{\\rm TeV}$ and $2.8~{\\rm PeV}$. Such a comparison indicates that the future IceCube-Gen2 will be able to pla"},"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":"1704.04027","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2017-04-13T08:19:30Z","cross_cats_sorted":["astro-ph.HE","hep-ex"],"title_canon_sha256":"055ff819b155fc4d256f4c0ce85e3ee4b60f0f298f168cf41e0d96cbd412895f","abstract_canon_sha256":"8e36af659a4ce162a9640f77f4f01a90b7595117c8ba825ed000470095759b5f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:26:12.870729Z","signature_b64":"85dv0cGZJ3EKslHQWzfrU208r8mBKj9eUdEOtgfye7FWY25CdBokAbNxyGcJdYCTIA1qO1ylRqzEnwmhGra6CA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0175671bcd7d0c0bf789fcae85ebb7c6c158d9bba8365400670ebc384d4b6917","last_reissued_at":"2026-05-18T00:26:12.870110Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:26:12.870110Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Constraining the Mass Scale of a Lorentz-Violating Hamiltonian with the Measurement of Astrophysical Neutrino-Flavor Composition","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","hep-ex"],"primary_cat":"hep-ph","authors_text":"Guey-Lin Lin, Kwang-Chang Lai, Wei-Hao Lai","submitted_at":"2017-04-13T08:19:30Z","abstract_excerpt":"We study Lorentz violation effects on flavor transitions of high energy astrophysical neutrinos. It is shown that the appearance of Lorentz violating Hamiltonian can drastically change the flavor transition probabilities of astrophysical neutrinos. Predictions of Lorentz violation effects on flavor compositions of astrophysical neutrinos arriving on Earth are compared with IceCube flavor composition measurement which analyzes astrophysical neutrino events in the energy range between $25~{\\rm TeV}$ and $2.8~{\\rm PeV}$. Such a comparison indicates that the future IceCube-Gen2 will be able to pla"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.04027","kind":"arxiv","version":3},"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":"1704.04027","created_at":"2026-05-18T00:26:12.870197+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.04027v3","created_at":"2026-05-18T00:26:12.870197+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.04027","created_at":"2026-05-18T00:26:12.870197+00:00"},{"alias_kind":"pith_short_12","alias_value":"AF2WOG6NPUGA","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_16","alias_value":"AF2WOG6NPUGAX54J","created_at":"2026-05-18T12:31:05.417338+00:00"},{"alias_kind":"pith_short_8","alias_value":"AF2WOG6N","created_at":"2026-05-18T12:31:05.417338+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3","json":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3.json","graph_json":"https://pith.science/api/pith-number/AF2WOG6NPUGAX54J7SXIL25XY3/graph.json","events_json":"https://pith.science/api/pith-number/AF2WOG6NPUGAX54J7SXIL25XY3/events.json","paper":"https://pith.science/paper/AF2WOG6N"},"agent_actions":{"view_html":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3","download_json":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3.json","view_paper":"https://pith.science/paper/AF2WOG6N","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.04027&json=true","fetch_graph":"https://pith.science/api/pith-number/AF2WOG6NPUGAX54J7SXIL25XY3/graph.json","fetch_events":"https://pith.science/api/pith-number/AF2WOG6NPUGAX54J7SXIL25XY3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3/action/storage_attestation","attest_author":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3/action/author_attestation","sign_citation":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3/action/citation_signature","submit_replication":"https://pith.science/pith/AF2WOG6NPUGAX54J7SXIL25XY3/action/replication_record"}},"created_at":"2026-05-18T00:26:12.870197+00:00","updated_at":"2026-05-18T00:26:12.870197+00:00"}