{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:HCQ4JR5OORF5QLA4IFPBXTVTGP","short_pith_number":"pith:HCQ4JR5O","schema_version":"1.0","canonical_sha256":"38a1c4c7ae744bd82c1c415e1bceb333dbd8adfa195a1afa8394bb3a06c2ded2","source":{"kind":"arxiv","id":"1704.00015","version":3},"attestation_state":"computed","paper":{"title":"Linking High-Energy Cosmic Particles by Black-Hole Jets Embedded in Large-Scale Structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Ke Fang (U. Maryland), Kohta Murase (PSU)","submitted_at":"2017-03-31T18:00:53Z","abstract_excerpt":"The origin of ultrahigh-energy cosmic rays (UHECRs) is a half-century old enigma (Linsley 1963). The mystery has been deepened by an intriguing coincidence: over ten orders of magnitude in energy, the energy generation rates of UHECRs, PeV neutrinos, and isotropic sub-TeV gamma rays are comparable, which hints at a grand-unified picture (Murase and Waxman 2016). Here we report that powerful black hole jets in aggregates of galaxies can supply the common origin of all of these phenomena. Once accelerated by a jet, low-energy cosmic rays confined in the radio lobe are adiabatically cooled; highe"},"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":"1704.00015","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-03-31T18:00:53Z","cross_cats_sorted":["astro-ph.CO","hep-ph"],"title_canon_sha256":"9bf48fe8e7e435e22e328b828b9196a61707e93eb7b72e0b4547603b8dab19b4","abstract_canon_sha256":"dd640e132e3a96a039b54c3ec0d17ead3779c2c9aa87ed35d70e4a7c9a30b79a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:03:25.113068Z","signature_b64":"iTaHXgkupH3+Yb5OnLcZum+1baUlGfXbnRnEX0fsHBzBd0UdqGptOW1KkCc2KWKj5HZNaVZ3WuyNPtPHok5LAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"38a1c4c7ae744bd82c1c415e1bceb333dbd8adfa195a1afa8394bb3a06c2ded2","last_reissued_at":"2026-05-18T00:03:25.112652Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:03:25.112652Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Linking High-Energy Cosmic Particles by Black-Hole Jets Embedded in Large-Scale Structures","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.CO","hep-ph"],"primary_cat":"astro-ph.HE","authors_text":"Ke Fang (U. Maryland), Kohta Murase (PSU)","submitted_at":"2017-03-31T18:00:53Z","abstract_excerpt":"The origin of ultrahigh-energy cosmic rays (UHECRs) is a half-century old enigma (Linsley 1963). The mystery has been deepened by an intriguing coincidence: over ten orders of magnitude in energy, the energy generation rates of UHECRs, PeV neutrinos, and isotropic sub-TeV gamma rays are comparable, which hints at a grand-unified picture (Murase and Waxman 2016). Here we report that powerful black hole jets in aggregates of galaxies can supply the common origin of all of these phenomena. Once accelerated by a jet, low-energy cosmic rays confined in the radio lobe are adiabatically cooled; highe"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1704.00015","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":"1704.00015","created_at":"2026-05-18T00:03:25.112720+00:00"},{"alias_kind":"arxiv_version","alias_value":"1704.00015v3","created_at":"2026-05-18T00:03:25.112720+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1704.00015","created_at":"2026-05-18T00:03:25.112720+00:00"},{"alias_kind":"pith_short_12","alias_value":"HCQ4JR5OORF5","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_16","alias_value":"HCQ4JR5OORF5QLA4","created_at":"2026-05-18T12:31:18.294218+00:00"},{"alias_kind":"pith_short_8","alias_value":"HCQ4JR5O","created_at":"2026-05-18T12:31:18.294218+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":3,"sample":[{"citing_arxiv_id":"2405.17409","citing_title":"Ultraheavy Ultrahigh-Energy Cosmic Rays","ref_index":103,"is_internal_anchor":true},{"citing_arxiv_id":"2512.00660","citing_title":"Particle Astrophysics with High and Ultrahigh Energy Neutrinos","ref_index":66,"is_internal_anchor":true},{"citing_arxiv_id":"2605.13968","citing_title":"Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes","ref_index":4,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP","json":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP.json","graph_json":"https://pith.science/api/pith-number/HCQ4JR5OORF5QLA4IFPBXTVTGP/graph.json","events_json":"https://pith.science/api/pith-number/HCQ4JR5OORF5QLA4IFPBXTVTGP/events.json","paper":"https://pith.science/paper/HCQ4JR5O"},"agent_actions":{"view_html":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP","download_json":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP.json","view_paper":"https://pith.science/paper/HCQ4JR5O","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1704.00015&json=true","fetch_graph":"https://pith.science/api/pith-number/HCQ4JR5OORF5QLA4IFPBXTVTGP/graph.json","fetch_events":"https://pith.science/api/pith-number/HCQ4JR5OORF5QLA4IFPBXTVTGP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP/action/storage_attestation","attest_author":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP/action/author_attestation","sign_citation":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP/action/citation_signature","submit_replication":"https://pith.science/pith/HCQ4JR5OORF5QLA4IFPBXTVTGP/action/replication_record"}},"created_at":"2026-05-18T00:03:25.112720+00:00","updated_at":"2026-05-18T00:03:25.112720+00:00"}