{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:EHKXWQ4TXI4D76VS6SWXXRB23B","short_pith_number":"pith:EHKXWQ4T","schema_version":"1.0","canonical_sha256":"21d57b4393ba383ffab2f4ad7bc43ad8414e616f148608e31fbc5591f299e859","source":{"kind":"arxiv","id":"2302.14200","version":2},"attestation_state":"computed","paper":{"title":"Spontaneous Lorentz symmetry breaking effects on GRBs jets arising from neutrino pair annihilation process near a black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc"],"primary_cat":"hep-ph","authors_text":"Gaetano Lambiase, Leonardo Mastrototaro, Mohsen Khodadi","submitted_at":"2023-02-27T23:35:41Z","abstract_excerpt":"The study of neutrino pair annihilation into electron-positron pairs ($\\nu{\\bar \\nu}\\to e^-e^+$) is astrophysically well-motivated because it is a possible powering mechanism for the gamma-ray bursts (GRBs). In this paper, we estimate the gamma-ray energy deposition rate (EDR) arising from the annihilation of the neutrino pairs in the equatorial plane of a slowly rotating black hole geometry modified by the broken Lorentz symmetry (induced by a background bumblebee vector field). More specifically, owing to the presence of a dimensionless Lorentz symmetry breaking (LSB) parameter $l$ arising f"},"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":"2302.14200","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2023-02-27T23:35:41Z","cross_cats_sorted":["astro-ph.HE","gr-qc"],"title_canon_sha256":"168ad270476bd8ad0e99a943b2e7b41050fe8653d5bde44fc33307d9b1058ee2","abstract_canon_sha256":"bfdc088197c0e8a3a068f4fac3b0b786c3844bd2fa12e3d9df8533a490ad098b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:53:36.274293Z","signature_b64":"NfsjyWvh12zQRL5+yKz2bHekGc828neTF6iYzyigHumMdGtXsfRuaBfI/YU/uylar4dMG7n+N96BxfN9yseuDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"21d57b4393ba383ffab2f4ad7bc43ad8414e616f148608e31fbc5591f299e859","last_reissued_at":"2026-07-05T05:53:36.273931Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:53:36.273931Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Spontaneous Lorentz symmetry breaking effects on GRBs jets arising from neutrino pair annihilation process near a black hole","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","gr-qc"],"primary_cat":"hep-ph","authors_text":"Gaetano Lambiase, Leonardo Mastrototaro, Mohsen Khodadi","submitted_at":"2023-02-27T23:35:41Z","abstract_excerpt":"The study of neutrino pair annihilation into electron-positron pairs ($\\nu{\\bar \\nu}\\to e^-e^+$) is astrophysically well-motivated because it is a possible powering mechanism for the gamma-ray bursts (GRBs). In this paper, we estimate the gamma-ray energy deposition rate (EDR) arising from the annihilation of the neutrino pairs in the equatorial plane of a slowly rotating black hole geometry modified by the broken Lorentz symmetry (induced by a background bumblebee vector field). More specifically, owing to the presence of a dimensionless Lorentz symmetry breaking (LSB) parameter $l$ arising f"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2302.14200","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2302.14200/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":"2302.14200","created_at":"2026-07-05T05:53:36.273994+00:00"},{"alias_kind":"arxiv_version","alias_value":"2302.14200v2","created_at":"2026-07-05T05:53:36.273994+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2302.14200","created_at":"2026-07-05T05:53:36.273994+00:00"},{"alias_kind":"pith_short_12","alias_value":"EHKXWQ4TXI4D","created_at":"2026-07-05T05:53:36.273994+00:00"},{"alias_kind":"pith_short_16","alias_value":"EHKXWQ4TXI4D76VS","created_at":"2026-07-05T05:53:36.273994+00:00"},{"alias_kind":"pith_short_8","alias_value":"EHKXWQ4T","created_at":"2026-07-05T05:53:36.273994+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07011","citing_title":"Primordial black hole in Lorentz-violating theories: Insights from Bumblebee gravity","ref_index":69,"is_internal_anchor":true},{"citing_arxiv_id":"2510.23292","citing_title":"Energy extraction from a rotating black hole via magnetic reconnection: Bumblebee gravity","ref_index":31,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B","json":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B.json","graph_json":"https://pith.science/api/pith-number/EHKXWQ4TXI4D76VS6SWXXRB23B/graph.json","events_json":"https://pith.science/api/pith-number/EHKXWQ4TXI4D76VS6SWXXRB23B/events.json","paper":"https://pith.science/paper/EHKXWQ4T"},"agent_actions":{"view_html":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B","download_json":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B.json","view_paper":"https://pith.science/paper/EHKXWQ4T","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2302.14200&json=true","fetch_graph":"https://pith.science/api/pith-number/EHKXWQ4TXI4D76VS6SWXXRB23B/graph.json","fetch_events":"https://pith.science/api/pith-number/EHKXWQ4TXI4D76VS6SWXXRB23B/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B/action/storage_attestation","attest_author":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B/action/author_attestation","sign_citation":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B/action/citation_signature","submit_replication":"https://pith.science/pith/EHKXWQ4TXI4D76VS6SWXXRB23B/action/replication_record"}},"created_at":"2026-07-05T05:53:36.273994+00:00","updated_at":"2026-07-05T05:53:36.273994+00:00"}