{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:QAG3MRZRWUNVS5SAKFRJRJ2R4N","short_pith_number":"pith:QAG3MRZR","schema_version":"1.0","canonical_sha256":"800db64731b51b597640516298a751e370f806bffef171ae969c441d3875747e","source":{"kind":"arxiv","id":"2309.12264","version":1},"attestation_state":"computed","paper":{"title":"GRB221009A gamma-ray events from non-standard neutrino self-interactions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Mansi Dhuria","submitted_at":"2023-09-21T17:14:47Z","abstract_excerpt":"The flux of high-energy astrophysical neutrinos observed by the present generation of neutrino detectors has already indicated a few hints of new physics beyond the Standard Model. In this work, we show that high-energy gamma-ray observations can also be considered as a complementary probe for unveiling the source of high-energy astrophysical neutrino events and new physics. Recently, the LHAASO collaboration has reported O(5000) gamma-ray events in the energy range between 0.5 TeV -18 TeV from gamma-ray burst GRB221009A within 2000 seconds after the initial outburst. We showed that attenuated"},"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":"2309.12264","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2023-09-21T17:14:47Z","cross_cats_sorted":["astro-ph.CO","astro-ph.HE"],"title_canon_sha256":"dc5c3cf5686a49751a92a0c4555a971f0a09f6175e6598377192d71c05cc9772","abstract_canon_sha256":"f72a5d320d02ec59c5070cb2bf5559ccbb2057ced9a63bfcea614b3e7e5e06a0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:53:00.853670Z","signature_b64":"LD5Eo+YcE1+NpttK2mM0YA4YzoGpyuadfXwnrv/d0smMUeFooZ9vPv8vyg2VSitbMoUDudc+VEZXUnI72mKQBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"800db64731b51b597640516298a751e370f806bffef171ae969c441d3875747e","last_reissued_at":"2026-07-05T06:53:00.853194Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:53:00.853194Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"GRB221009A gamma-ray events from non-standard neutrino self-interactions","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","astro-ph.HE"],"primary_cat":"hep-ph","authors_text":"Mansi Dhuria","submitted_at":"2023-09-21T17:14:47Z","abstract_excerpt":"The flux of high-energy astrophysical neutrinos observed by the present generation of neutrino detectors has already indicated a few hints of new physics beyond the Standard Model. In this work, we show that high-energy gamma-ray observations can also be considered as a complementary probe for unveiling the source of high-energy astrophysical neutrino events and new physics. Recently, the LHAASO collaboration has reported O(5000) gamma-ray events in the energy range between 0.5 TeV -18 TeV from gamma-ray burst GRB221009A within 2000 seconds after the initial outburst. We showed that attenuated"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.12264","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/2309.12264/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":"2309.12264","created_at":"2026-07-05T06:53:00.853253+00:00"},{"alias_kind":"arxiv_version","alias_value":"2309.12264v1","created_at":"2026-07-05T06:53:00.853253+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2309.12264","created_at":"2026-07-05T06:53:00.853253+00:00"},{"alias_kind":"pith_short_12","alias_value":"QAG3MRZRWUNV","created_at":"2026-07-05T06:53:00.853253+00:00"},{"alias_kind":"pith_short_16","alias_value":"QAG3MRZRWUNVS5SA","created_at":"2026-07-05T06:53:00.853253+00:00"},{"alias_kind":"pith_short_8","alias_value":"QAG3MRZR","created_at":"2026-07-05T06:53:00.853253+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.02425","citing_title":"Carpet-3 detection of a photon-like air shower with estimated primary energy above 100 TeV in a spatial and temporal coincidence with GRB 221009A","ref_index":72,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N","json":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N.json","graph_json":"https://pith.science/api/pith-number/QAG3MRZRWUNVS5SAKFRJRJ2R4N/graph.json","events_json":"https://pith.science/api/pith-number/QAG3MRZRWUNVS5SAKFRJRJ2R4N/events.json","paper":"https://pith.science/paper/QAG3MRZR"},"agent_actions":{"view_html":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N","download_json":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N.json","view_paper":"https://pith.science/paper/QAG3MRZR","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2309.12264&json=true","fetch_graph":"https://pith.science/api/pith-number/QAG3MRZRWUNVS5SAKFRJRJ2R4N/graph.json","fetch_events":"https://pith.science/api/pith-number/QAG3MRZRWUNVS5SAKFRJRJ2R4N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N/action/storage_attestation","attest_author":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N/action/author_attestation","sign_citation":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N/action/citation_signature","submit_replication":"https://pith.science/pith/QAG3MRZRWUNVS5SAKFRJRJ2R4N/action/replication_record"}},"created_at":"2026-07-05T06:53:00.853253+00:00","updated_at":"2026-07-05T06:53:00.853253+00:00"}