{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2016:IV7HNZK4S3O2HGTXBXAPNMPXTF","short_pith_number":"pith:IV7HNZK4","schema_version":"1.0","canonical_sha256":"457e76e55c96dda39a770dc0f6b1f79976b05d08ef49260090b0f3fe03996a46","source":{"kind":"arxiv","id":"1609.04851","version":2},"attestation_state":"computed","paper":{"title":"Kinetic turbulence in relativistic plasma: from thermal bath to non-thermal continuum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.flu-dyn"],"primary_cat":"physics.plasm-ph","authors_text":"Dmitri A. Uzdensky, Gregory R. Werner, Mitchell C. Begelman, Vladimir Zhdankin","submitted_at":"2016-09-15T20:31:25Z","abstract_excerpt":"We present results from particle-in-cell simulations of driven turbulence in magnetized, collisionless, and relativistic pair plasma. We find that fluctuations are consistent with the classical $k_\\perp^{-5/3}$ magnetic energy spectrum at fluid scales and a steeper $k_\\perp^{-4}$ spectrum at sub-Larmor scales, where $k_\\perp$ is the wavevector perpendicular to the mean field. We demonstrate the development of a non-thermal, power-law particle energy distribution, $f(E) \\sim E^{-\\alpha}$, with index $\\alpha$ that decreases with increasing magnetization and increases with increasing system size "},"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":"1609.04851","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2016-09-15T20:31:25Z","cross_cats_sorted":["astro-ph.HE","physics.flu-dyn"],"title_canon_sha256":"5c29f11cd9beb32937775df1bd3df307edd37cace8ae2a346b0df1faccfef9b1","abstract_canon_sha256":"99cd9bc9b8ec5eaadca031af26f46cbd21544c0607bb25de0c86e016e2645d96"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:50:56.701854Z","signature_b64":"VDNCB0oHKz+Nv7UbJfJIKBYSkaEWwJrmTBxyDdCVpAHeGvLc8DHQvsis49cTV0I8uoVAtquwL9wau5kmHiyjDw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"457e76e55c96dda39a770dc0f6b1f79976b05d08ef49260090b0f3fe03996a46","last_reissued_at":"2026-05-18T00:50:56.701141Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:50:56.701141Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinetic turbulence in relativistic plasma: from thermal bath to non-thermal continuum","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE","physics.flu-dyn"],"primary_cat":"physics.plasm-ph","authors_text":"Dmitri A. Uzdensky, Gregory R. Werner, Mitchell C. Begelman, Vladimir Zhdankin","submitted_at":"2016-09-15T20:31:25Z","abstract_excerpt":"We present results from particle-in-cell simulations of driven turbulence in magnetized, collisionless, and relativistic pair plasma. We find that fluctuations are consistent with the classical $k_\\perp^{-5/3}$ magnetic energy spectrum at fluid scales and a steeper $k_\\perp^{-4}$ spectrum at sub-Larmor scales, where $k_\\perp$ is the wavevector perpendicular to the mean field. We demonstrate the development of a non-thermal, power-law particle energy distribution, $f(E) \\sim E^{-\\alpha}$, with index $\\alpha$ that decreases with increasing magnetization and increases with increasing system size "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1609.04851","kind":"arxiv","version":2},"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":"1609.04851","created_at":"2026-05-18T00:50:56.701258+00:00"},{"alias_kind":"arxiv_version","alias_value":"1609.04851v2","created_at":"2026-05-18T00:50:56.701258+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1609.04851","created_at":"2026-05-18T00:50:56.701258+00:00"},{"alias_kind":"pith_short_12","alias_value":"IV7HNZK4S3O2","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_16","alias_value":"IV7HNZK4S3O2HGTX","created_at":"2026-05-18T12:30:22.444734+00:00"},{"alias_kind":"pith_short_8","alias_value":"IV7HNZK4","created_at":"2026-05-18T12:30:22.444734+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2506.04212","citing_title":"Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence","ref_index":21,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF","json":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF.json","graph_json":"https://pith.science/api/pith-number/IV7HNZK4S3O2HGTXBXAPNMPXTF/graph.json","events_json":"https://pith.science/api/pith-number/IV7HNZK4S3O2HGTXBXAPNMPXTF/events.json","paper":"https://pith.science/paper/IV7HNZK4"},"agent_actions":{"view_html":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF","download_json":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF.json","view_paper":"https://pith.science/paper/IV7HNZK4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1609.04851&json=true","fetch_graph":"https://pith.science/api/pith-number/IV7HNZK4S3O2HGTXBXAPNMPXTF/graph.json","fetch_events":"https://pith.science/api/pith-number/IV7HNZK4S3O2HGTXBXAPNMPXTF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF/action/storage_attestation","attest_author":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF/action/author_attestation","sign_citation":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF/action/citation_signature","submit_replication":"https://pith.science/pith/IV7HNZK4S3O2HGTXBXAPNMPXTF/action/replication_record"}},"created_at":"2026-05-18T00:50:56.701258+00:00","updated_at":"2026-05-18T00:50:56.701258+00:00"}