{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2014:HCCDX6QLJ76XXABBEPX5OMECID","short_pith_number":"pith:HCCDX6QL","schema_version":"1.0","canonical_sha256":"38843bfa0b4ffd7b802123efd7308240e66c8c8e115430ab0ba5fa766ca49cab","source":{"kind":"arxiv","id":"1404.2288","version":3},"attestation_state":"computed","paper":{"title":"Cosmic neutrino cascades from secret neutrino interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"John F. Beacom (Ohio State University), Kenny C. Y. Ng","submitted_at":"2014-04-08T20:02:30Z","abstract_excerpt":"The first detection of high-energy astrophysical neutrinos by IceCube provides new opportunities for tests of neutrino properties. The long baseline through the Cosmic Neutrino Background (C$\\nu$B) is particularly useful for directly testing secret neutrino interactions ($\\nu$SI) that would cause neutrino-neutrino elastic scattering at a larger rate than the usual weak interactions. We show that IceCube can provide competitive sensitivity to $\\nu$SI compared to other astrophysical and cosmological probes, which are complementary to laboratory tests. We study the spectral distortions caused by "},"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":"1404.2288","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2014-04-08T20:02:30Z","cross_cats_sorted":["hep-ph","nucl-th"],"title_canon_sha256":"7ac44d3034d4e8b9da971ae1a93cf878a2dd75cdad9cf2a49b252da6ae5ef4e3","abstract_canon_sha256":"0d179ab54865dee4bab1f5d434e89448c91dc737aeac1abf42d36325ca76020e"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:38:52.995225Z","signature_b64":"TuM22EmNXNV02cLjKygrVYtFDvkohUjcicKuKwNYtmpdcM5MXtgFT1KXhloI4xObNcOldBt1SdK8agvoOSNwBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"38843bfa0b4ffd7b802123efd7308240e66c8c8e115430ab0ba5fa766ca49cab","last_reissued_at":"2026-05-18T02:38:52.994910Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:38:52.994910Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic neutrino cascades from secret neutrino interactions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph","nucl-th"],"primary_cat":"astro-ph.HE","authors_text":"John F. Beacom (Ohio State University), Kenny C. Y. Ng","submitted_at":"2014-04-08T20:02:30Z","abstract_excerpt":"The first detection of high-energy astrophysical neutrinos by IceCube provides new opportunities for tests of neutrino properties. The long baseline through the Cosmic Neutrino Background (C$\\nu$B) is particularly useful for directly testing secret neutrino interactions ($\\nu$SI) that would cause neutrino-neutrino elastic scattering at a larger rate than the usual weak interactions. We show that IceCube can provide competitive sensitivity to $\\nu$SI compared to other astrophysical and cosmological probes, which are complementary to laboratory tests. We study the spectral distortions caused by "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1404.2288","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":"1404.2288","created_at":"2026-05-18T02:38:52.994957+00:00"},{"alias_kind":"arxiv_version","alias_value":"1404.2288v3","created_at":"2026-05-18T02:38:52.994957+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1404.2288","created_at":"2026-05-18T02:38:52.994957+00:00"},{"alias_kind":"pith_short_12","alias_value":"HCCDX6QLJ76X","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_16","alias_value":"HCCDX6QLJ76XXABB","created_at":"2026-05-18T12:28:30.664211+00:00"},{"alias_kind":"pith_short_8","alias_value":"HCCDX6QL","created_at":"2026-05-18T12:28:30.664211+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"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":27,"is_internal_anchor":true},{"citing_arxiv_id":"2602.12477","citing_title":"Towards a complete scheme of cosmological neutrino self-interactions: Collision term for a wide range of mediator masses","ref_index":112,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID","json":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID.json","graph_json":"https://pith.science/api/pith-number/HCCDX6QLJ76XXABBEPX5OMECID/graph.json","events_json":"https://pith.science/api/pith-number/HCCDX6QLJ76XXABBEPX5OMECID/events.json","paper":"https://pith.science/paper/HCCDX6QL"},"agent_actions":{"view_html":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID","download_json":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID.json","view_paper":"https://pith.science/paper/HCCDX6QL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1404.2288&json=true","fetch_graph":"https://pith.science/api/pith-number/HCCDX6QLJ76XXABBEPX5OMECID/graph.json","fetch_events":"https://pith.science/api/pith-number/HCCDX6QLJ76XXABBEPX5OMECID/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID/action/storage_attestation","attest_author":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID/action/author_attestation","sign_citation":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID/action/citation_signature","submit_replication":"https://pith.science/pith/HCCDX6QLJ76XXABBEPX5OMECID/action/replication_record"}},"created_at":"2026-05-18T02:38:52.994957+00:00","updated_at":"2026-05-18T02:38:52.994957+00:00"}