{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:4CNROEHW2JAZFAENIJMS4IG6NH","short_pith_number":"pith:4CNROEHW","schema_version":"1.0","canonical_sha256":"e09b1710f6d24192808d42592e20de69d4fcb9b799dc03e5949acbb45f4cf6f5","source":{"kind":"arxiv","id":"1603.00230","version":2},"attestation_state":"computed","paper":{"title":"Neutrino masses and ordering via multimessenger astronomy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ex"],"primary_cat":"hep-ph","authors_text":"Aurora Meroni, Francesco Sannino, Kasper Langaeble","submitted_at":"2016-03-01T11:05:31Z","abstract_excerpt":"We define the theoretical framework and deduce the conditions under which multi-messenger astronomy can provide useful information about neutrino masses and their ordering. The framework uses time differences between the arrival of neutrinos and the other light messenger, i.e. the graviton, emitted in astrophysical catastrophes. We also provide a preliminary feasibility study elucidating the experimental reach and challenges for planned neutrino detectors such as Hyper-Kamiokande as well as future several megaton detectors. This study shows that future experiments can be useful in testing inde"},"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":"1603.00230","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2016-03-01T11:05:31Z","cross_cats_sorted":["astro-ph.HE","gr-qc","hep-ex"],"title_canon_sha256":"41962a71670ecba207c7c6ecdaab55cce4b54bdd94e9d7704228137c34ae0fae","abstract_canon_sha256":"8a5789e644f31246efde0fd362b9c334f2a5df6ef8a95a024739e4cdb8294044"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:03:19.645961Z","signature_b64":"yKsM0/D/uLyMVamX436d26AQQ+1ahnhWJfZ+MeqcPAyoIMyzsRlmPSZo8/EBdjqy4hMd+745cMpRixN0VgbIAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e09b1710f6d24192808d42592e20de69d4fcb9b799dc03e5949acbb45f4cf6f5","last_reissued_at":"2026-05-18T01:03:19.645526Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:03:19.645526Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Neutrino masses and ordering via multimessenger astronomy","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc","hep-ex"],"primary_cat":"hep-ph","authors_text":"Aurora Meroni, Francesco Sannino, Kasper Langaeble","submitted_at":"2016-03-01T11:05:31Z","abstract_excerpt":"We define the theoretical framework and deduce the conditions under which multi-messenger astronomy can provide useful information about neutrino masses and their ordering. The framework uses time differences between the arrival of neutrinos and the other light messenger, i.e. the graviton, emitted in astrophysical catastrophes. We also provide a preliminary feasibility study elucidating the experimental reach and challenges for planned neutrino detectors such as Hyper-Kamiokande as well as future several megaton detectors. This study shows that future experiments can be useful in testing inde"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1603.00230","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":"1603.00230","created_at":"2026-05-18T01:03:19.645590+00:00"},{"alias_kind":"arxiv_version","alias_value":"1603.00230v2","created_at":"2026-05-18T01:03:19.645590+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1603.00230","created_at":"2026-05-18T01:03:19.645590+00:00"},{"alias_kind":"pith_short_12","alias_value":"4CNROEHW2JAZ","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_16","alias_value":"4CNROEHW2JAZFAEN","created_at":"2026-05-18T12:29:58.707656+00:00"},{"alias_kind":"pith_short_8","alias_value":"4CNROEHW","created_at":"2026-05-18T12:29:58.707656+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/4CNROEHW2JAZFAENIJMS4IG6NH","json":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH.json","graph_json":"https://pith.science/api/pith-number/4CNROEHW2JAZFAENIJMS4IG6NH/graph.json","events_json":"https://pith.science/api/pith-number/4CNROEHW2JAZFAENIJMS4IG6NH/events.json","paper":"https://pith.science/paper/4CNROEHW"},"agent_actions":{"view_html":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH","download_json":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH.json","view_paper":"https://pith.science/paper/4CNROEHW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1603.00230&json=true","fetch_graph":"https://pith.science/api/pith-number/4CNROEHW2JAZFAENIJMS4IG6NH/graph.json","fetch_events":"https://pith.science/api/pith-number/4CNROEHW2JAZFAENIJMS4IG6NH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH/action/storage_attestation","attest_author":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH/action/author_attestation","sign_citation":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH/action/citation_signature","submit_replication":"https://pith.science/pith/4CNROEHW2JAZFAENIJMS4IG6NH/action/replication_record"}},"created_at":"2026-05-18T01:03:19.645590+00:00","updated_at":"2026-05-18T01:03:19.645590+00:00"}