{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:F7JMNYYBXMYHBNF7H532ZNX556","short_pith_number":"pith:F7JMNYYB","schema_version":"1.0","canonical_sha256":"2fd2c6e301bb3070b4bf3f77acb6fdef9709339232095f0b3d2586f01fb68f10","source":{"kind":"arxiv","id":"2304.12335","version":2},"attestation_state":"computed","paper":{"title":"Cosmic ray transport in large-amplitude turbulence with small-scale field reversals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alexander A. Philippov, Alisa K. Galishnikova, Bart Ripperda, Drummond B. Fielding, Eliot Quataert, Matthew W. Kunz, Philipp Kempski","submitted_at":"2023-04-24T18:00:00Z","abstract_excerpt":"The nature of cosmic ray (CR) transport in the Milky Way remains elusive. The predictions of current micro-physical CR transport models in magneto-hydrodynamic (MHD) turbulence are drastically different from what is observed. These models usually focus on MHD turbulence with a strong guide field and ignore the impact of turbulent intermittency on particle propagation. This motivates our studying the alternative regime of large-amplitude turbulence with $\\delta B/B_0 \\gg 1$, in which intermittent small-scale magnetic field reversals are ubiquitous. We study particle transport in such turbulence"},"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":"2304.12335","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2023-04-24T18:00:00Z","cross_cats_sorted":["astro-ph.GA","physics.plasm-ph"],"title_canon_sha256":"4eaadbb2f32442d288cff8cfd2c946ba41226f65bf100fd15d52cad8eb375e78","abstract_canon_sha256":"6156fa698b2e455b8bbe8438a85bc9cd02b9241bb75a3bfabda1c6969249a50f"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:26:13.381480Z","signature_b64":"nBuAZaf2SLLzphfOqbc3xhL8TYW6i3LsTsgyxnclvg63xK8s7tt3C5BjJJESAXCGDgAgG3FhGhML8Mn14KL8BA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2fd2c6e301bb3070b4bf3f77acb6fdef9709339232095f0b3d2586f01fb68f10","last_reissued_at":"2026-07-05T07:26:13.381040Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:26:13.381040Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Cosmic ray transport in large-amplitude turbulence with small-scale field reversals","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.GA","physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Alexander A. Philippov, Alisa K. Galishnikova, Bart Ripperda, Drummond B. Fielding, Eliot Quataert, Matthew W. Kunz, Philipp Kempski","submitted_at":"2023-04-24T18:00:00Z","abstract_excerpt":"The nature of cosmic ray (CR) transport in the Milky Way remains elusive. The predictions of current micro-physical CR transport models in magneto-hydrodynamic (MHD) turbulence are drastically different from what is observed. These models usually focus on MHD turbulence with a strong guide field and ignore the impact of turbulent intermittency on particle propagation. This motivates our studying the alternative regime of large-amplitude turbulence with $\\delta B/B_0 \\gg 1$, in which intermittent small-scale magnetic field reversals are ubiquitous. We study particle transport in such turbulence"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2304.12335","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2304.12335/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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":"2304.12335","created_at":"2026-07-05T07:26:13.381097+00:00"},{"alias_kind":"arxiv_version","alias_value":"2304.12335v2","created_at":"2026-07-05T07:26:13.381097+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2304.12335","created_at":"2026-07-05T07:26:13.381097+00:00"},{"alias_kind":"pith_short_12","alias_value":"F7JMNYYBXMYH","created_at":"2026-07-05T07:26:13.381097+00:00"},{"alias_kind":"pith_short_16","alias_value":"F7JMNYYBXMYHBNF7","created_at":"2026-07-05T07:26:13.381097+00:00"},{"alias_kind":"pith_short_8","alias_value":"F7JMNYYB","created_at":"2026-07-05T07:26:13.381097+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06744","citing_title":"CRexit observed: probing cosmic ray transport in the circumgalactic medium with absorption line spectra","ref_index":283,"is_internal_anchor":true},{"citing_arxiv_id":"2606.28141","citing_title":"Transition from Diffusion to Drift-Dominated Cosmic Ray Transport and the Origin of the Knee","ref_index":65,"is_internal_anchor":false},{"citing_arxiv_id":"2509.07104","citing_title":"Cosmic Rays on Galaxy Scales: Progress and Pitfalls for CR-MHD Dynamical Models","ref_index":145,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13968","citing_title":"Particle Acceleration, Coronal Neutrino Production, and the Diffuse Extragalactic Neutrino Background from Supermassive Black Holes","ref_index":44,"is_internal_anchor":false},{"citing_arxiv_id":"2506.04212","citing_title":"Studying the mirror acceleration via kinetic simulations of relativistic plasma turbulence","ref_index":36,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556","json":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556.json","graph_json":"https://pith.science/api/pith-number/F7JMNYYBXMYHBNF7H532ZNX556/graph.json","events_json":"https://pith.science/api/pith-number/F7JMNYYBXMYHBNF7H532ZNX556/events.json","paper":"https://pith.science/paper/F7JMNYYB"},"agent_actions":{"view_html":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556","download_json":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556.json","view_paper":"https://pith.science/paper/F7JMNYYB","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2304.12335&json=true","fetch_graph":"https://pith.science/api/pith-number/F7JMNYYBXMYHBNF7H532ZNX556/graph.json","fetch_events":"https://pith.science/api/pith-number/F7JMNYYBXMYHBNF7H532ZNX556/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556/action/timestamp_anchor","attest_storage":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556/action/storage_attestation","attest_author":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556/action/author_attestation","sign_citation":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556/action/citation_signature","submit_replication":"https://pith.science/pith/F7JMNYYBXMYHBNF7H532ZNX556/action/replication_record"}},"created_at":"2026-07-05T07:26:13.381097+00:00","updated_at":"2026-07-05T07:26:13.381097+00:00"}