{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:3A2GRY6FEIN6EU2APU4F7A72CG","short_pith_number":"pith:3A2GRY6F","schema_version":"1.0","canonical_sha256":"d83468e3c5221be253407d385f83fa11a4c7641d3fe7e110a1c229e7955925d3","source":{"kind":"arxiv","id":"1908.08032","version":2},"attestation_state":"computed","paper":{"title":"Kinetic turbulence in shining pair plasma: intermittent beaming and thermalization by radiative cooling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Dmitri A. Uzdensky, Gregory R. Werner, Mitchell C. Begelman, Vladimir Zhdankin","submitted_at":"2019-08-21T17:55:11Z","abstract_excerpt":"High-energy astrophysical systems frequently contain collisionless relativistic plasmas that are heated by turbulent cascades and cooled by emission of radiation. Understanding the nature of this radiative turbulence is a frontier of extreme plasma astrophysics. In this paper, we use particle-in-cell simulations to study the effects of external inverse Compton radiation on turbulence driven in an optically thin, relativistic pair plasma. We focus on the statistical steady state (where injected energy is balanced by radiated energy) and perform a parameter scan spanning from low magnetization 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":"1908.08032","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2019-08-21T17:55:11Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"c7b80b7d5f9fc9a9a6cb110a7c0627b6b57638aa9e336fe0266371a1a56d21b7","abstract_canon_sha256":"9ecfef70958529f46ba1c228a7fec780a8c84deba36b4a31e572a4c266f860be"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:38:03.722396Z","signature_b64":"S83VzJpA0+KsRsI6xsqIcKsdVu812476cJlHNQlsrbRCJGPpv/0D7TqcZJIP/kyXeZUP9n0EuOG+y8JCyjcLDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d83468e3c5221be253407d385f83fa11a4c7641d3fe7e110a1c229e7955925d3","last_reissued_at":"2026-07-05T00:38:03.721801Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:38:03.721801Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Kinetic turbulence in shining pair plasma: intermittent beaming and thermalization by radiative cooling","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Dmitri A. Uzdensky, Gregory R. Werner, Mitchell C. Begelman, Vladimir Zhdankin","submitted_at":"2019-08-21T17:55:11Z","abstract_excerpt":"High-energy astrophysical systems frequently contain collisionless relativistic plasmas that are heated by turbulent cascades and cooled by emission of radiation. Understanding the nature of this radiative turbulence is a frontier of extreme plasma astrophysics. In this paper, we use particle-in-cell simulations to study the effects of external inverse Compton radiation on turbulence driven in an optically thin, relativistic pair plasma. We focus on the statistical steady state (where injected energy is balanced by radiated energy) and perform a parameter scan spanning from low magnetization t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1908.08032","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/1908.08032/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":"1908.08032","created_at":"2026-07-05T00:38:03.721860+00:00"},{"alias_kind":"arxiv_version","alias_value":"1908.08032v2","created_at":"2026-07-05T00:38:03.721860+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1908.08032","created_at":"2026-07-05T00:38:03.721860+00:00"},{"alias_kind":"pith_short_12","alias_value":"3A2GRY6FEIN6","created_at":"2026-07-05T00:38:03.721860+00:00"},{"alias_kind":"pith_short_16","alias_value":"3A2GRY6FEIN6EU2A","created_at":"2026-07-05T00:38:03.721860+00:00"},{"alias_kind":"pith_short_8","alias_value":"3A2GRY6F","created_at":"2026-07-05T00:38:03.721860+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":23,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG","json":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG.json","graph_json":"https://pith.science/api/pith-number/3A2GRY6FEIN6EU2APU4F7A72CG/graph.json","events_json":"https://pith.science/api/pith-number/3A2GRY6FEIN6EU2APU4F7A72CG/events.json","paper":"https://pith.science/paper/3A2GRY6F"},"agent_actions":{"view_html":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG","download_json":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG.json","view_paper":"https://pith.science/paper/3A2GRY6F","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1908.08032&json=true","fetch_graph":"https://pith.science/api/pith-number/3A2GRY6FEIN6EU2APU4F7A72CG/graph.json","fetch_events":"https://pith.science/api/pith-number/3A2GRY6FEIN6EU2APU4F7A72CG/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG/action/storage_attestation","attest_author":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG/action/author_attestation","sign_citation":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG/action/citation_signature","submit_replication":"https://pith.science/pith/3A2GRY6FEIN6EU2APU4F7A72CG/action/replication_record"}},"created_at":"2026-07-05T00:38:03.721860+00:00","updated_at":"2026-07-05T00:38:03.721860+00:00"}