{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:G7U5YAPILR3Q2V3KHANJNKQKPE","short_pith_number":"pith:G7U5YAPI","schema_version":"1.0","canonical_sha256":"37e9dc01e85c770d576a381a96aa0a7913490f09e42ae00a382ba77c6de99431","source":{"kind":"arxiv","id":"2205.02489","version":1},"attestation_state":"computed","paper":{"title":"Plasma physics of the intracluster medium","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Irina Zhuravleva, Matthew W. Kunz, Thomas W. Jones","submitted_at":"2022-05-05T07:59:42Z","abstract_excerpt":"This Chapter provides a brief tutorial on some aspects of plasma physics that are fundamental to understanding the dynamics and energetics of the intracluster medium (ICM). The tutorial is split into two parts: one that focuses on the thermal plasma component -- its stability, viscosity, conductivity, and ability to amplify magnetic fields to dynamical strengths via turbulence and other plasma processes; and one that focuses on the non-thermal population of charged particles known as cosmic rays -- their acceleration, re-acceleration, and transport throughout the cluster volume. Observational "},"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":"2205.02489","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"astro-ph.HE","submitted_at":"2022-05-05T07:59:42Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"95ad6290c0af4c05e128e1137312ea518235abdb8b3782191c62c28716f6d970","abstract_canon_sha256":"ebbf75b542a9d82aba458b59540aef7d3f9a13dc3abc3ec0fac5277b4966fb78"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:57:53.592979Z","signature_b64":"2qKAJxK0AjUNAdpT/WY+XjoODp2LDbzYVA5G2232AT9RxoMbslblGl9nDP2MIoGCrqMmtWXDc5/UppME6HxzCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"37e9dc01e85c770d576a381a96aa0a7913490f09e42ae00a382ba77c6de99431","last_reissued_at":"2026-07-05T05:57:53.592432Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:57:53.592432Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Plasma physics of the intracluster medium","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.HE","authors_text":"Irina Zhuravleva, Matthew W. Kunz, Thomas W. Jones","submitted_at":"2022-05-05T07:59:42Z","abstract_excerpt":"This Chapter provides a brief tutorial on some aspects of plasma physics that are fundamental to understanding the dynamics and energetics of the intracluster medium (ICM). The tutorial is split into two parts: one that focuses on the thermal plasma component -- its stability, viscosity, conductivity, and ability to amplify magnetic fields to dynamical strengths via turbulence and other plasma processes; and one that focuses on the non-thermal population of charged particles known as cosmic rays -- their acceleration, re-acceleration, and transport throughout the cluster volume. Observational "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.02489","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/2205.02489/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":"2205.02489","created_at":"2026-07-05T05:57:53.592563+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.02489v1","created_at":"2026-07-05T05:57:53.592563+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.02489","created_at":"2026-07-05T05:57:53.592563+00:00"},{"alias_kind":"pith_short_12","alias_value":"G7U5YAPILR3Q","created_at":"2026-07-05T05:57:53.592563+00:00"},{"alias_kind":"pith_short_16","alias_value":"G7U5YAPILR3Q2V3K","created_at":"2026-07-05T05:57:53.592563+00:00"},{"alias_kind":"pith_short_8","alias_value":"G7U5YAPI","created_at":"2026-07-05T05:57:53.592563+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2502.05235","citing_title":"A comparison of the turbulent dynamo in weakly-collisional and collisional plasmas: from subsonic to supersonic turbulence","ref_index":50,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE","json":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE.json","graph_json":"https://pith.science/api/pith-number/G7U5YAPILR3Q2V3KHANJNKQKPE/graph.json","events_json":"https://pith.science/api/pith-number/G7U5YAPILR3Q2V3KHANJNKQKPE/events.json","paper":"https://pith.science/paper/G7U5YAPI"},"agent_actions":{"view_html":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE","download_json":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE.json","view_paper":"https://pith.science/paper/G7U5YAPI","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.02489&json=true","fetch_graph":"https://pith.science/api/pith-number/G7U5YAPILR3Q2V3KHANJNKQKPE/graph.json","fetch_events":"https://pith.science/api/pith-number/G7U5YAPILR3Q2V3KHANJNKQKPE/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE/action/timestamp_anchor","attest_storage":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE/action/storage_attestation","attest_author":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE/action/author_attestation","sign_citation":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE/action/citation_signature","submit_replication":"https://pith.science/pith/G7U5YAPILR3Q2V3KHANJNKQKPE/action/replication_record"}},"created_at":"2026-07-05T05:57:53.592563+00:00","updated_at":"2026-07-05T05:57:53.592563+00:00"}