{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2018:FSE3FGD2SVUAATAAOD4F26ROPD","short_pith_number":"pith:FSE3FGD2","schema_version":"1.0","canonical_sha256":"2c89b2987a9568004c0070f85d7a2e78e54d37b554b9c91f23b2ada1e730037f","source":{"kind":"arxiv","id":"1810.12428","version":1},"attestation_state":"computed","paper":{"title":"Inertial Kinetic-Alfv\\'en Turbulence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"Christopher H.K. Chen, Daniel Gro\\v{s}elj, Gian Luca Delzanno, Nuno F. Loureiro, Stanislav Boldyrev, Vadim Roytershteyn","submitted_at":"2018-10-29T22:03:24Z","abstract_excerpt":"Recent observational and analytical studies suggested that a new regime of kinetic turbulence may exist in plasma environments with low electron beta (Chen and Boldyrev, 2017). Such a regime, termed inertial kinetic-Alfv\\'en turbulence, is relevant for the solar corona, Earth's magnetosheath, and other astrophysical systems where the electron and ion plasma beta parameters satisfy the condition $\\beta_e\\ll \\beta_i\\lesssim 1$. In this paper we present kinetic numerical simulations that confirm existence of the iKAW regime. Specifically, the simulations demonstrate a transition at scales below e"},"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":"1810.12428","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2018-10-29T22:03:24Z","cross_cats_sorted":["physics.space-ph"],"title_canon_sha256":"4dc398d7ebb7f380f05ee1ddddb7d19ed5216a95073ebc3e400e67362da16e47","abstract_canon_sha256":"d4bf9c51d27164353c24082dfaa480953f1371ceb11e1ddf865700ffc41d0209"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T00:02:02.696636Z","signature_b64":"Sj1rQtzn6ypH/HYEDehZDbdiguoAFWAiCJLkI8eiRmzaV/wPYDPGz1n2mOSob0eJ4z8Yt5hH3cf8omz13PJDBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2c89b2987a9568004c0070f85d7a2e78e54d37b554b9c91f23b2ada1e730037f","last_reissued_at":"2026-05-18T00:02:02.696091Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T00:02:02.696091Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Inertial Kinetic-Alfv\\'en Turbulence","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.space-ph"],"primary_cat":"physics.plasm-ph","authors_text":"Christopher H.K. Chen, Daniel Gro\\v{s}elj, Gian Luca Delzanno, Nuno F. Loureiro, Stanislav Boldyrev, Vadim Roytershteyn","submitted_at":"2018-10-29T22:03:24Z","abstract_excerpt":"Recent observational and analytical studies suggested that a new regime of kinetic turbulence may exist in plasma environments with low electron beta (Chen and Boldyrev, 2017). Such a regime, termed inertial kinetic-Alfv\\'en turbulence, is relevant for the solar corona, Earth's magnetosheath, and other astrophysical systems where the electron and ion plasma beta parameters satisfy the condition $\\beta_e\\ll \\beta_i\\lesssim 1$. In this paper we present kinetic numerical simulations that confirm existence of the iKAW regime. Specifically, the simulations demonstrate a transition at scales below e"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1810.12428","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":"1810.12428","created_at":"2026-05-18T00:02:02.696181+00:00"},{"alias_kind":"arxiv_version","alias_value":"1810.12428v1","created_at":"2026-05-18T00:02:02.696181+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1810.12428","created_at":"2026-05-18T00:02:02.696181+00:00"},{"alias_kind":"pith_short_12","alias_value":"FSE3FGD2SVUA","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_16","alias_value":"FSE3FGD2SVUAATAA","created_at":"2026-05-18T12:32:25.280505+00:00"},{"alias_kind":"pith_short_8","alias_value":"FSE3FGD2","created_at":"2026-05-18T12:32:25.280505+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/FSE3FGD2SVUAATAAOD4F26ROPD","json":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD.json","graph_json":"https://pith.science/api/pith-number/FSE3FGD2SVUAATAAOD4F26ROPD/graph.json","events_json":"https://pith.science/api/pith-number/FSE3FGD2SVUAATAAOD4F26ROPD/events.json","paper":"https://pith.science/paper/FSE3FGD2"},"agent_actions":{"view_html":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD","download_json":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD.json","view_paper":"https://pith.science/paper/FSE3FGD2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1810.12428&json=true","fetch_graph":"https://pith.science/api/pith-number/FSE3FGD2SVUAATAAOD4F26ROPD/graph.json","fetch_events":"https://pith.science/api/pith-number/FSE3FGD2SVUAATAAOD4F26ROPD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD/action/storage_attestation","attest_author":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD/action/author_attestation","sign_citation":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD/action/citation_signature","submit_replication":"https://pith.science/pith/FSE3FGD2SVUAATAAOD4F26ROPD/action/replication_record"}},"created_at":"2026-05-18T00:02:02.696181+00:00","updated_at":"2026-05-18T00:02:02.696181+00:00"}