{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:EJNK7AXJFNNAXFTOKOPWIQ3ZX3","short_pith_number":"pith:EJNK7AXJ","schema_version":"1.0","canonical_sha256":"225aaf82e92b5a0b966e539f644379bef9037c29cbe4160da7b50a89c48cd2db","source":{"kind":"arxiv","id":"2408.01699","version":1},"attestation_state":"computed","paper":{"title":"Electrostatic Waves and Electron Holes in Simulations of Low-Mach Quasi-Perpendicular Shocks","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Aaron Tran, Artem Bohdan, Lorenzo Sironi, Lynn B. Wilson III","submitted_at":"2024-08-03T07:41:29Z","abstract_excerpt":"Collisionless low Mach number shocks are abundant in astrophysical and space plasma environments, exhibiting complex wave activity and wave-particle interactions. In this paper, we present 2D Particle-in-Cell (PIC) simulations of quasi-perpendicular nonrelativistic ($\\vsh \\approx (5500-22000)$ km/s) low Mach number shocks, with a specific focus on studying electrostatic waves in the shock ramp and the precursor regions. In these shocks, an ion-scale oblique whistler wave creates a configuration with two hot counter-streaming electron beams, which drive unstable electron acoustic waves (EAWs) t"},"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":"2408.01699","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"physics.space-ph","submitted_at":"2024-08-03T07:41:29Z","cross_cats_sorted":["astro-ph.HE","physics.plasm-ph"],"title_canon_sha256":"b7b4b118b8a2e313630a41be5a92a2b2760a37ba12c524112a2d5e5b363157b2","abstract_canon_sha256":"f6c52e14b81b6182cfb88e0d69f52a2d6da27e2a4b80da9b0dd459d29776400b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:52:01.494408Z","signature_b64":"oJyleUQj2n6eUKTz99TN0umcUl17yQ1vfPONPZ0vZzgDwL3GE8lUcUgKsh97yGzSrlDE4NkMWd0eCSu0XTadBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"225aaf82e92b5a0b966e539f644379bef9037c29cbe4160da7b50a89c48cd2db","last_reissued_at":"2026-07-05T08:52:01.493985Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:52:01.493985Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Electrostatic Waves and Electron Holes in Simulations of Low-Mach Quasi-Perpendicular Shocks","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.HE","physics.plasm-ph"],"primary_cat":"physics.space-ph","authors_text":"Aaron Tran, Artem Bohdan, Lorenzo Sironi, Lynn B. Wilson III","submitted_at":"2024-08-03T07:41:29Z","abstract_excerpt":"Collisionless low Mach number shocks are abundant in astrophysical and space plasma environments, exhibiting complex wave activity and wave-particle interactions. In this paper, we present 2D Particle-in-Cell (PIC) simulations of quasi-perpendicular nonrelativistic ($\\vsh \\approx (5500-22000)$ km/s) low Mach number shocks, with a specific focus on studying electrostatic waves in the shock ramp and the precursor regions. In these shocks, an ion-scale oblique whistler wave creates a configuration with two hot counter-streaming electron beams, which drive unstable electron acoustic waves (EAWs) t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.01699","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/2408.01699/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":"2408.01699","created_at":"2026-07-05T08:52:01.494040+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.01699v1","created_at":"2026-07-05T08:52:01.494040+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.01699","created_at":"2026-07-05T08:52:01.494040+00:00"},{"alias_kind":"pith_short_12","alias_value":"EJNK7AXJFNNA","created_at":"2026-07-05T08:52:01.494040+00:00"},{"alias_kind":"pith_short_16","alias_value":"EJNK7AXJFNNAXFTO","created_at":"2026-07-05T08:52:01.494040+00:00"},{"alias_kind":"pith_short_8","alias_value":"EJNK7AXJ","created_at":"2026-07-05T08:52:01.494040+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.18020","citing_title":"Kinetic simulations underestimate the effects of waves during magnetic reconnection","ref_index":28,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3","json":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3.json","graph_json":"https://pith.science/api/pith-number/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/graph.json","events_json":"https://pith.science/api/pith-number/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/events.json","paper":"https://pith.science/paper/EJNK7AXJ"},"agent_actions":{"view_html":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3","download_json":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3.json","view_paper":"https://pith.science/paper/EJNK7AXJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.01699&json=true","fetch_graph":"https://pith.science/api/pith-number/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/graph.json","fetch_events":"https://pith.science/api/pith-number/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/action/storage_attestation","attest_author":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/action/author_attestation","sign_citation":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/action/citation_signature","submit_replication":"https://pith.science/pith/EJNK7AXJFNNAXFTOKOPWIQ3ZX3/action/replication_record"}},"created_at":"2026-07-05T08:52:01.494040+00:00","updated_at":"2026-07-05T08:52:01.494040+00:00"}