{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:EAMRZLTKZMAANVRW4E535F3CTY","short_pith_number":"pith:EAMRZLTK","schema_version":"1.0","canonical_sha256":"20191cae6acb0006d636e13bbe97629e2da79fcd1eac54b042c38d1c6e1d826f","source":{"kind":"arxiv","id":"1010.5390","version":1},"attestation_state":"computed","paper":{"title":"Orders of Fermi- and Plasma-Accelerations of Cosmic Rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Saleh (Egyptian Ctr. Theor. Phys., A. Tawfik (Egyptian Ctr. Theor. Phys., Cairo)","submitted_at":"2010-10-26T13:19:35Z","abstract_excerpt":"The generic acceleration model for ultra high energy cosmic rays, which has been introduced in {\\tt 1006.5708 [astro-ph.HE]}, suggests various types of electromagnetic interactions between cosmic charged particles and the different types of the plasma fields, which are assumed to have general configurations, spatially and temporally. The well-known Fermi acceleration mechanisms are also included in the model. Meanwhile Fermi mechanisms in non-relativistic limit adhere first- and second-order of $\\beta$, the ratio of particle's velocity relative to the velocity of the stellar magnetic cloud, in"},"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":"1010.5390","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2010-10-26T13:19:35Z","cross_cats_sorted":[],"title_canon_sha256":"871657561db7ec65ff2126ed56ce95bfda461502b5e9d3da41ad64cf5c8fd912","abstract_canon_sha256":"61abb84cc048214d5791e68aa73d2f836a6645a7725198520edb2337be0088cf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:56:19.561323Z","signature_b64":"4Kn03yjh8BXClt/GAjqTjnWQ1HD9vMYdgpAaLDaP90Yt0+J8VnQhmwab2ISE3vfRyn64sr7IJKrsG3ebaCoSDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"20191cae6acb0006d636e13bbe97629e2da79fcd1eac54b042c38d1c6e1d826f","last_reissued_at":"2026-05-18T02:56:19.560749Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:56:19.560749Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Orders of Fermi- and Plasma-Accelerations of Cosmic Rays","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"A. Saleh (Egyptian Ctr. Theor. Phys., A. Tawfik (Egyptian Ctr. Theor. Phys., Cairo)","submitted_at":"2010-10-26T13:19:35Z","abstract_excerpt":"The generic acceleration model for ultra high energy cosmic rays, which has been introduced in {\\tt 1006.5708 [astro-ph.HE]}, suggests various types of electromagnetic interactions between cosmic charged particles and the different types of the plasma fields, which are assumed to have general configurations, spatially and temporally. The well-known Fermi acceleration mechanisms are also included in the model. Meanwhile Fermi mechanisms in non-relativistic limit adhere first- and second-order of $\\beta$, the ratio of particle's velocity relative to the velocity of the stellar magnetic cloud, in"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1010.5390","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":"1010.5390","created_at":"2026-05-18T02:56:19.560843+00:00"},{"alias_kind":"arxiv_version","alias_value":"1010.5390v1","created_at":"2026-05-18T02:56:19.560843+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1010.5390","created_at":"2026-05-18T02:56:19.560843+00:00"},{"alias_kind":"pith_short_12","alias_value":"EAMRZLTKZMAA","created_at":"2026-05-18T12:26:06.534383+00:00"},{"alias_kind":"pith_short_16","alias_value":"EAMRZLTKZMAANVRW","created_at":"2026-05-18T12:26:06.534383+00:00"},{"alias_kind":"pith_short_8","alias_value":"EAMRZLTK","created_at":"2026-05-18T12:26:06.534383+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/EAMRZLTKZMAANVRW4E535F3CTY","json":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY.json","graph_json":"https://pith.science/api/pith-number/EAMRZLTKZMAANVRW4E535F3CTY/graph.json","events_json":"https://pith.science/api/pith-number/EAMRZLTKZMAANVRW4E535F3CTY/events.json","paper":"https://pith.science/paper/EAMRZLTK"},"agent_actions":{"view_html":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY","download_json":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY.json","view_paper":"https://pith.science/paper/EAMRZLTK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1010.5390&json=true","fetch_graph":"https://pith.science/api/pith-number/EAMRZLTKZMAANVRW4E535F3CTY/graph.json","fetch_events":"https://pith.science/api/pith-number/EAMRZLTKZMAANVRW4E535F3CTY/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY/action/storage_attestation","attest_author":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY/action/author_attestation","sign_citation":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY/action/citation_signature","submit_replication":"https://pith.science/pith/EAMRZLTKZMAANVRW4E535F3CTY/action/replication_record"}},"created_at":"2026-05-18T02:56:19.560843+00:00","updated_at":"2026-05-18T02:56:19.560843+00:00"}