{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:6GVLD5UX4YSXWLAD2NLVYC46LQ","short_pith_number":"pith:6GVLD5UX","schema_version":"1.0","canonical_sha256":"f1aab1f697e6257b2c03d3575c0b9e5c0bb00015cd484dc4e753f7abb311577d","source":{"kind":"arxiv","id":"astro-ph/0410266","version":3},"attestation_state":"computed","paper":{"title":"Particle Acceleration, Magnetic Field Generation, and Emission in Relativistic Shocks","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"C. B. Hededal (Niels Bohr Institute), G. J. Fishman (MSFC/NSSTC), G. Richardson (NSSTC), H. Sol (OBSPM), K.-I. Nishikawa (NSSTC), P. Hardee (UA), R. Preece (UAH/NSSTC)","submitted_at":"2004-10-11T14:19:05Z","abstract_excerpt":"Shock acceleration is an ubiquitous phenomenon in astrophysical plasmas. Plasma waves and their associated instabilities (e.g., Buneman, Weibel and other two-stream instabilities) created in collisionless shocks are responsible for particle (electron, positron, and ion) acceleration. Using a 3-D relativistic electromagnetic particle (REMP) code, we have investigated particle acceleration associated with a relativistic jet front propagating into an ambient plasma. We find small differences in the results for no ambient and modest ambient magnetic fields. Simulations show that the Weibel instabi"},"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":"astro-ph/0410266","kind":"arxiv","version":3},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2004-10-11T14:19:05Z","cross_cats_sorted":[],"title_canon_sha256":"47054d06f2832e116583ab714ceb54ab71363f0c7804719e3559afbb07ac8b19","abstract_canon_sha256":"03e4f9aecb39d2665b46e1cde4379d5f1884a025f820f8da74ab278ab938dd89"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:40:34.950677Z","signature_b64":"vaOwa0DxcMEEgv6hqPD4KI9rH9mt/Fr2Yc3/xW9fmRT4vH3gEjnqSnXvQBA3AtWAcXljJscryDFsqXgka9cnDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f1aab1f697e6257b2c03d3575c0b9e5c0bb00015cd484dc4e753f7abb311577d","last_reissued_at":"2026-05-18T01:40:34.949986Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:40:34.949986Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Particle Acceleration, Magnetic Field Generation, and Emission in Relativistic Shocks","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"C. B. Hededal (Niels Bohr Institute), G. J. Fishman (MSFC/NSSTC), G. Richardson (NSSTC), H. Sol (OBSPM), K.-I. Nishikawa (NSSTC), P. Hardee (UA), R. Preece (UAH/NSSTC)","submitted_at":"2004-10-11T14:19:05Z","abstract_excerpt":"Shock acceleration is an ubiquitous phenomenon in astrophysical plasmas. Plasma waves and their associated instabilities (e.g., Buneman, Weibel and other two-stream instabilities) created in collisionless shocks are responsible for particle (electron, positron, and ion) acceleration. Using a 3-D relativistic electromagnetic particle (REMP) code, we have investigated particle acceleration associated with a relativistic jet front propagating into an ambient plasma. We find small differences in the results for no ambient and modest ambient magnetic fields. Simulations show that the Weibel instabi"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0410266","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":"astro-ph/0410266","created_at":"2026-05-18T01:40:34.950093+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0410266v3","created_at":"2026-05-18T01:40:34.950093+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0410266","created_at":"2026-05-18T01:40:34.950093+00:00"},{"alias_kind":"pith_short_12","alias_value":"6GVLD5UX4YSX","created_at":"2026-05-18T12:25:52.051335+00:00"},{"alias_kind":"pith_short_16","alias_value":"6GVLD5UX4YSXWLAD","created_at":"2026-05-18T12:25:52.051335+00:00"},{"alias_kind":"pith_short_8","alias_value":"6GVLD5UX","created_at":"2026-05-18T12:25:52.051335+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/6GVLD5UX4YSXWLAD2NLVYC46LQ","json":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ.json","graph_json":"https://pith.science/api/pith-number/6GVLD5UX4YSXWLAD2NLVYC46LQ/graph.json","events_json":"https://pith.science/api/pith-number/6GVLD5UX4YSXWLAD2NLVYC46LQ/events.json","paper":"https://pith.science/paper/6GVLD5UX"},"agent_actions":{"view_html":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ","download_json":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ.json","view_paper":"https://pith.science/paper/6GVLD5UX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0410266&json=true","fetch_graph":"https://pith.science/api/pith-number/6GVLD5UX4YSXWLAD2NLVYC46LQ/graph.json","fetch_events":"https://pith.science/api/pith-number/6GVLD5UX4YSXWLAD2NLVYC46LQ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ/action/storage_attestation","attest_author":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ/action/author_attestation","sign_citation":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ/action/citation_signature","submit_replication":"https://pith.science/pith/6GVLD5UX4YSXWLAD2NLVYC46LQ/action/replication_record"}},"created_at":"2026-05-18T01:40:34.950093+00:00","updated_at":"2026-05-18T01:40:34.950093+00:00"}