{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2017:SJNS5RTQB5YF7LGXZFAU2CJA6Q","short_pith_number":"pith:SJNS5RTQ","schema_version":"1.0","canonical_sha256":"925b2ec6700f705facd7c9414d0920f408eeab482248ce811062c36e4988a0ba","source":{"kind":"arxiv","id":"1703.02795","version":1},"attestation_state":"computed","paper":{"title":"Particle Spectra and Mass Composition in the Ultra-High Energy Region in the Framework of the Galactic Origin of Cosmic Rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Lagutin, A.G. Tyumentsev, N.V. Volkov, R.I. Raikin","submitted_at":"2017-03-08T11:54:08Z","abstract_excerpt":"The possibility for a self-consistent description of all the basic features of the observed cosmic ray spectra and primary composition variations in the energy range of $10^{15}\\div 10^{20}$ eV within the Galactic origin scenario is examined.\n  We assume the existence of Galactic sources that accelerate particles up to $\\sim 3\\cdot 10^{18}Z$ eV and take into account a highly inhomogeneous (fractal-like) distribution of matter and magnetic fields in the Galaxy that leads to extremely large free paths of particles (\"L\\'{e}vy flights\"), along with an overwhelming contribution to the cosmic ray fl"},"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":"1703.02795","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2017-03-08T11:54:08Z","cross_cats_sorted":[],"title_canon_sha256":"d85ee5094e35ba82c10a2ff010b882eb0760dfe552f572d6fa91568b347d0f42","abstract_canon_sha256":"5b6ef265175f8e94e1f6da8400a41381f93c28dfb989842e8b231d5d851ab37d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:46:04.648431Z","signature_b64":"XL3/mgG/xKmYrdY/5ZO43c+HnBH3VJi7IWlknjdw4sNjDOBLHyxPiZvCnylHcGGbsSAI2CGmK3qIY6/AD8fTCQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"925b2ec6700f705facd7c9414d0920f408eeab482248ce811062c36e4988a0ba","last_reissued_at":"2026-05-17T23:46:04.647288Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:46:04.647288Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Particle Spectra and Mass Composition in the Ultra-High Energy Region in the Framework of the Galactic Origin of Cosmic Rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A.A. Lagutin, A.G. Tyumentsev, N.V. Volkov, R.I. Raikin","submitted_at":"2017-03-08T11:54:08Z","abstract_excerpt":"The possibility for a self-consistent description of all the basic features of the observed cosmic ray spectra and primary composition variations in the energy range of $10^{15}\\div 10^{20}$ eV within the Galactic origin scenario is examined.\n  We assume the existence of Galactic sources that accelerate particles up to $\\sim 3\\cdot 10^{18}Z$ eV and take into account a highly inhomogeneous (fractal-like) distribution of matter and magnetic fields in the Galaxy that leads to extremely large free paths of particles (\"L\\'{e}vy flights\"), along with an overwhelming contribution to the cosmic ray fl"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1703.02795","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":""},"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":"1703.02795","created_at":"2026-05-17T23:46:04.647391+00:00"},{"alias_kind":"arxiv_version","alias_value":"1703.02795v1","created_at":"2026-05-17T23:46:04.647391+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1703.02795","created_at":"2026-05-17T23:46:04.647391+00:00"},{"alias_kind":"pith_short_12","alias_value":"SJNS5RTQB5YF","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_16","alias_value":"SJNS5RTQB5YF7LGX","created_at":"2026-05-18T12:31:43.269735+00:00"},{"alias_kind":"pith_short_8","alias_value":"SJNS5RTQ","created_at":"2026-05-18T12:31:43.269735+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/SJNS5RTQB5YF7LGXZFAU2CJA6Q","json":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q.json","graph_json":"https://pith.science/api/pith-number/SJNS5RTQB5YF7LGXZFAU2CJA6Q/graph.json","events_json":"https://pith.science/api/pith-number/SJNS5RTQB5YF7LGXZFAU2CJA6Q/events.json","paper":"https://pith.science/paper/SJNS5RTQ"},"agent_actions":{"view_html":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q","download_json":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q.json","view_paper":"https://pith.science/paper/SJNS5RTQ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1703.02795&json=true","fetch_graph":"https://pith.science/api/pith-number/SJNS5RTQB5YF7LGXZFAU2CJA6Q/graph.json","fetch_events":"https://pith.science/api/pith-number/SJNS5RTQB5YF7LGXZFAU2CJA6Q/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q/action/storage_attestation","attest_author":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q/action/author_attestation","sign_citation":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q/action/citation_signature","submit_replication":"https://pith.science/pith/SJNS5RTQB5YF7LGXZFAU2CJA6Q/action/replication_record"}},"created_at":"2026-05-17T23:46:04.647391+00:00","updated_at":"2026-05-17T23:46:04.647391+00:00"}