{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2004:OQS3WQC6YYZRWZZ4AQ477VQXDI","short_pith_number":"pith:OQS3WQC6","canonical_record":{"source":{"id":"physics/0407015","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"physics.plasm-ph","submitted_at":"2004-07-02T14:43:10Z","cross_cats_sorted":[],"title_canon_sha256":"57b817f867bee75c4d4a90eb607a2700ebf8d89bf6ad3a0ded98c9a62bdacdd7","abstract_canon_sha256":"04461d59b523eac89caca4d66c99245dcd5b2e0eede58349df3d6cc4968e45b8"},"schema_version":"1.0"},"canonical_sha256":"7425bb405ec6331b673c0439ffd6171a22cbbc1221598696443c62dba67ba961","source":{"kind":"arxiv","id":"physics/0407015","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"physics/0407015","created_at":"2026-05-18T04:28:10Z"},{"alias_kind":"arxiv_version","alias_value":"physics/0407015v1","created_at":"2026-05-18T04:28:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.physics/0407015","created_at":"2026-05-18T04:28:10Z"},{"alias_kind":"pith_short_12","alias_value":"OQS3WQC6YYZR","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_16","alias_value":"OQS3WQC6YYZRWZZ4","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_8","alias_value":"OQS3WQC6","created_at":"2026-05-18T12:25:52Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2004:OQS3WQC6YYZRWZZ4AQ477VQXDI","target":"record","payload":{"canonical_record":{"source":{"id":"physics/0407015","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"physics.plasm-ph","submitted_at":"2004-07-02T14:43:10Z","cross_cats_sorted":[],"title_canon_sha256":"57b817f867bee75c4d4a90eb607a2700ebf8d89bf6ad3a0ded98c9a62bdacdd7","abstract_canon_sha256":"04461d59b523eac89caca4d66c99245dcd5b2e0eede58349df3d6cc4968e45b8"},"schema_version":"1.0"},"canonical_sha256":"7425bb405ec6331b673c0439ffd6171a22cbbc1221598696443c62dba67ba961","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:28:10.238068Z","signature_b64":"zOc6k+M+5m73lFedYYmHnOHGtG759GJMRZBcvCUxGTnlrJb8rDVIs3PKFU231thPlHpxb5RmLcDuhAIp5OG7Dg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"7425bb405ec6331b673c0439ffd6171a22cbbc1221598696443c62dba67ba961","last_reissued_at":"2026-05-18T04:28:10.237474Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:28:10.237474Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"physics/0407015","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:28:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"IBF6memFrCjWQcS0BpXlZD6xtaJQQR7W5UkZ3WEY70+BbIIQFx0iQQ2WfZ4/iZdY9mZKHZiiZ1z1z0T5nNSoAQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T15:06:44.510468Z"},"content_sha256":"2f7627ca1b1bd028c40eb9416d7ef166e6b92ca681ef234242a8e013e42020e2","schema_version":"1.0","event_id":"sha256:2f7627ca1b1bd028c40eb9416d7ef166e6b92ca681ef234242a8e013e42020e2"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2004:OQS3WQC6YYZRWZZ4AQ477VQXDI","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Relativistic kinetic theory of magnetoplasmas","license":"","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"Alexei Beklemishev (Inst. of Nucl. Phys., CMFD, INFN, Massimo Tessarotto (Trieste U., Novosibirsk), Piero Nicolini (Trieste U., Trieste)","submitted_at":"2004-07-02T14:43:10Z","abstract_excerpt":"Recently, an increasing interest in astrophysical as well as laboratory plasmas has been manifested in reference to the existence of relativistic flows, related in turn to the production of intense electric fields in magnetized systems. Such phenomena require their description in the framework of a consistent relativistic kinetic theory, rather than on relativistic MHD equations, subject to specific closure conditions. The purpose of this work is to apply the relativistic single-particle guiding-center theory developed by Beklemishev and Tessarotto, including the nonlinear treatment of small-w"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"physics/0407015","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T04:28:10Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"h3EWuq+hHYLUpi57a6VQloyRmAsyKqc/zkwrMkl2JTVhsgY8PXiMkmFFpKpSMgy9YsS1T/lnfo415/qcUKvHBQ==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T15:06:44.511143Z"},"content_sha256":"22e3c73561110ed214d44cb6dae4eeb66d8b5612f7fb32e5fc2dc6e7d1d49c5c","schema_version":"1.0","event_id":"sha256:22e3c73561110ed214d44cb6dae4eeb66d8b5612f7fb32e5fc2dc6e7d1d49c5c"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/OQS3WQC6YYZRWZZ4AQ477VQXDI/bundle.json","state_url":"https://pith.science/pith/OQS3WQC6YYZRWZZ4AQ477VQXDI/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/OQS3WQC6YYZRWZZ4AQ477VQXDI/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-05-26T15:06:44Z","links":{"resolver":"https://pith.science/pith/OQS3WQC6YYZRWZZ4AQ477VQXDI","bundle":"https://pith.science/pith/OQS3WQC6YYZRWZZ4AQ477VQXDI/bundle.json","state":"https://pith.science/pith/OQS3WQC6YYZRWZZ4AQ477VQXDI/state.json","well_known_bundle":"https://pith.science/.well-known/pith/OQS3WQC6YYZRWZZ4AQ477VQXDI/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2004:OQS3WQC6YYZRWZZ4AQ477VQXDI","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"04461d59b523eac89caca4d66c99245dcd5b2e0eede58349df3d6cc4968e45b8","cross_cats_sorted":[],"license":"","primary_cat":"physics.plasm-ph","submitted_at":"2004-07-02T14:43:10Z","title_canon_sha256":"57b817f867bee75c4d4a90eb607a2700ebf8d89bf6ad3a0ded98c9a62bdacdd7"},"schema_version":"1.0","source":{"id":"physics/0407015","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"physics/0407015","created_at":"2026-05-18T04:28:10Z"},{"alias_kind":"arxiv_version","alias_value":"physics/0407015v1","created_at":"2026-05-18T04:28:10Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.physics/0407015","created_at":"2026-05-18T04:28:10Z"},{"alias_kind":"pith_short_12","alias_value":"OQS3WQC6YYZR","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_16","alias_value":"OQS3WQC6YYZRWZZ4","created_at":"2026-05-18T12:25:52Z"},{"alias_kind":"pith_short_8","alias_value":"OQS3WQC6","created_at":"2026-05-18T12:25:52Z"}],"graph_snapshots":[{"event_id":"sha256:22e3c73561110ed214d44cb6dae4eeb66d8b5612f7fb32e5fc2dc6e7d1d49c5c","target":"graph","created_at":"2026-05-18T04:28:10Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Recently, an increasing interest in astrophysical as well as laboratory plasmas has been manifested in reference to the existence of relativistic flows, related in turn to the production of intense electric fields in magnetized systems. Such phenomena require their description in the framework of a consistent relativistic kinetic theory, rather than on relativistic MHD equations, subject to specific closure conditions. The purpose of this work is to apply the relativistic single-particle guiding-center theory developed by Beklemishev and Tessarotto, including the nonlinear treatment of small-w","authors_text":"Alexei Beklemishev (Inst. of Nucl. Phys., CMFD, INFN, Massimo Tessarotto (Trieste U., Novosibirsk), Piero Nicolini (Trieste U., Trieste)","cross_cats":[],"headline":"","license":"","primary_cat":"physics.plasm-ph","submitted_at":"2004-07-02T14:43:10Z","title":"Relativistic kinetic theory of magnetoplasmas"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"physics/0407015","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:2f7627ca1b1bd028c40eb9416d7ef166e6b92ca681ef234242a8e013e42020e2","target":"record","created_at":"2026-05-18T04:28:10Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"04461d59b523eac89caca4d66c99245dcd5b2e0eede58349df3d6cc4968e45b8","cross_cats_sorted":[],"license":"","primary_cat":"physics.plasm-ph","submitted_at":"2004-07-02T14:43:10Z","title_canon_sha256":"57b817f867bee75c4d4a90eb607a2700ebf8d89bf6ad3a0ded98c9a62bdacdd7"},"schema_version":"1.0","source":{"id":"physics/0407015","kind":"arxiv","version":1}},"canonical_sha256":"7425bb405ec6331b673c0439ffd6171a22cbbc1221598696443c62dba67ba961","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"7425bb405ec6331b673c0439ffd6171a22cbbc1221598696443c62dba67ba961","first_computed_at":"2026-05-18T04:28:10.237474Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T04:28:10.237474Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"zOc6k+M+5m73lFedYYmHnOHGtG759GJMRZBcvCUxGTnlrJb8rDVIs3PKFU231thPlHpxb5RmLcDuhAIp5OG7Dg==","signature_status":"signed_v1","signed_at":"2026-05-18T04:28:10.238068Z","signed_message":"canonical_sha256_bytes"},"source_id":"physics/0407015","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:2f7627ca1b1bd028c40eb9416d7ef166e6b92ca681ef234242a8e013e42020e2","sha256:22e3c73561110ed214d44cb6dae4eeb66d8b5612f7fb32e5fc2dc6e7d1d49c5c"],"state_sha256":"78152d96ac4f890a8c278af5e3da178b80c9fe13771d2bbd7ca9810bc160741e"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"8mf4OuGKseIoaQg8dFsgAkAmHSjrwLwF/jMkifEu88KB7WTcuP01Y/8O5rfl+XEkr6qRdvC6esfsv6E+dHRMAw==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T15:06:44.514501Z","bundle_sha256":"179456bea770b108b8d6573b793d3282be1d4ce099211fa24cbc16e43b81fa45"}}