{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:JRIFYESS67HZQOBM3AA2X56DYD","short_pith_number":"pith:JRIFYESS","schema_version":"1.0","canonical_sha256":"4c505c1252f7cf98382cd801abf7c3c0d5fa426909b24d0700c623e26020a7ff","source":{"kind":"arxiv","id":"2504.00918","version":1},"attestation_state":"computed","paper":{"title":"Lorentz Invariance Violation from Gamma-Ray Bursts","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Bo-Qiang Ma, Hanlin Song","submitted_at":"2025-04-01T15:52:40Z","abstract_excerpt":"Lorentz invariance violation (LV) is examined through the time delay between high-energy and low-energy photons in gamma-ray bursts (GRBs). Previous studies determined the LV energy scale as $E_{\\rm LV} \\simeq 3.60 \\times 10^{17}$~GeV using Fermi Gamma-ray Space Telescope (FGST) data. This study updates the time-delay model and reaffirms these findings with new observations. High-energy photons from GRBs at GeV and TeV bands are analyzed, including the 99.3 GeV photon from GRB 221009A (FGST), the 1.07 TeV photon from GRB 190114C (MAGIC), and the 12.2 TeV photon from GRB 221009A (LHAASO). Our a"},"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":"2504.00918","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2025-04-01T15:52:40Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"d7ccf6dc712228f180ed93705172fb329b7e78fb348b07545cc79ece67fc123a","abstract_canon_sha256":"f682b7cda67646a06dce8c32ec477c9e545490ddf138a3671e0d49f5cb9b3302"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:42:52.911618Z","signature_b64":"5oOwGuC/i5SidULTt4G1Cg/OSufIyY4BnX4oYIcNuSzWJjIZh8C9s2u9JfvT8E0/PCVX4XgIS0sucExLCChFDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"4c505c1252f7cf98382cd801abf7c3c0d5fa426909b24d0700c623e26020a7ff","last_reissued_at":"2026-07-05T10:42:52.911166Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:42:52.911166Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Lorentz Invariance Violation from Gamma-Ray Bursts","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Bo-Qiang Ma, Hanlin Song","submitted_at":"2025-04-01T15:52:40Z","abstract_excerpt":"Lorentz invariance violation (LV) is examined through the time delay between high-energy and low-energy photons in gamma-ray bursts (GRBs). Previous studies determined the LV energy scale as $E_{\\rm LV} \\simeq 3.60 \\times 10^{17}$~GeV using Fermi Gamma-ray Space Telescope (FGST) data. This study updates the time-delay model and reaffirms these findings with new observations. High-energy photons from GRBs at GeV and TeV bands are analyzed, including the 99.3 GeV photon from GRB 221009A (FGST), the 1.07 TeV photon from GRB 190114C (MAGIC), and the 12.2 TeV photon from GRB 221009A (LHAASO). Our a"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2504.00918","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/2504.00918/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":"2504.00918","created_at":"2026-07-05T10:42:52.911229+00:00"},{"alias_kind":"arxiv_version","alias_value":"2504.00918v1","created_at":"2026-07-05T10:42:52.911229+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2504.00918","created_at":"2026-07-05T10:42:52.911229+00:00"},{"alias_kind":"pith_short_12","alias_value":"JRIFYESS67HZ","created_at":"2026-07-05T10:42:52.911229+00:00"},{"alias_kind":"pith_short_16","alias_value":"JRIFYESS67HZQOBM","created_at":"2026-07-05T10:42:52.911229+00:00"},{"alias_kind":"pith_short_8","alias_value":"JRIFYESS","created_at":"2026-07-05T10:42:52.911229+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2504.15685","citing_title":"Monte Carlo simulation of GRB data to test Lorentz-invariance violation","ref_index":32,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD","json":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD.json","graph_json":"https://pith.science/api/pith-number/JRIFYESS67HZQOBM3AA2X56DYD/graph.json","events_json":"https://pith.science/api/pith-number/JRIFYESS67HZQOBM3AA2X56DYD/events.json","paper":"https://pith.science/paper/JRIFYESS"},"agent_actions":{"view_html":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD","download_json":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD.json","view_paper":"https://pith.science/paper/JRIFYESS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2504.00918&json=true","fetch_graph":"https://pith.science/api/pith-number/JRIFYESS67HZQOBM3AA2X56DYD/graph.json","fetch_events":"https://pith.science/api/pith-number/JRIFYESS67HZQOBM3AA2X56DYD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD/action/storage_attestation","attest_author":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD/action/author_attestation","sign_citation":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD/action/citation_signature","submit_replication":"https://pith.science/pith/JRIFYESS67HZQOBM3AA2X56DYD/action/replication_record"}},"created_at":"2026-07-05T10:42:52.911229+00:00","updated_at":"2026-07-05T10:42:52.911229+00:00"}