{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:QYHRGD2LFTXDUADB3OKBIPHTGZ","short_pith_number":"pith:QYHRGD2L","schema_version":"1.0","canonical_sha256":"860f130f4b2cee3a0061db94143cf33671b346a3399bfd992cb8b1515b41f015","source":{"kind":"arxiv","id":"1903.04080","version":1},"attestation_state":"computed","paper":{"title":"[Plasma 2020 Decadal] The Material Properties of Weakly Collisional, High-Beta Plasmas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"physics.plasm-ph","authors_text":"A. A. Schekochihin, A. Spitkovsky, C. B. Forest, C. F. Gammie, C. H. K. Chen, C. S. Reynolds, E. Churazov, E. G. Zweibel, E. Quataert, I. Zhuravleva, J. M. Stone, J. Squire, L. Sironi, M. W. Kunz, S. A. Balbus, S. C. Cowley, S. D. Bale","submitted_at":"2019-03-11T00:08:44Z","abstract_excerpt":"This white paper, submitted for the Plasma 2020 Decadal Survey, concerns the physics of weakly collisional, high-beta plasmas -- plasmas in which the thermal pressure dominates over the magnetic pressure and in which the inter-particle collision time is comparable to the characteristic timescales of bulk motions. This state of matter, although widespread in the Universe, remains poorly understood: we lack a predictive theory for how it responds to perturbations, how it transports momentum and energy, and how it generates and amplifies magnetic fields. Such topics are foundational to the scient"},"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":"1903.04080","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2019-03-11T00:08:44Z","cross_cats_sorted":["astro-ph.HE"],"title_canon_sha256":"5f96a43c829eae039d0eb5a62b4d9dc53112d2b16878ffa653cc4f776ea7afb4","abstract_canon_sha256":"829e2f8ff2b76408d014353dd4bd0bc86421506be7e57a64fdbfd686afe92dbf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:51:40.108284Z","signature_b64":"+rGi4LUGpA2gFTSpu+zYUzngEkcroPuuR91dA4kH4BlDSZJbbEkxwEBQFhSAmw1qS8rQQhKfv08MOJ512MjMAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"860f130f4b2cee3a0061db94143cf33671b346a3399bfd992cb8b1515b41f015","last_reissued_at":"2026-05-17T23:51:40.107634Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:51:40.107634Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"[Plasma 2020 Decadal] The Material Properties of Weakly Collisional, High-Beta Plasmas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["astro-ph.HE"],"primary_cat":"physics.plasm-ph","authors_text":"A. A. Schekochihin, A. Spitkovsky, C. B. Forest, C. F. Gammie, C. H. K. Chen, C. S. Reynolds, E. Churazov, E. G. Zweibel, E. Quataert, I. Zhuravleva, J. M. Stone, J. Squire, L. Sironi, M. W. Kunz, S. A. Balbus, S. C. Cowley, S. D. Bale","submitted_at":"2019-03-11T00:08:44Z","abstract_excerpt":"This white paper, submitted for the Plasma 2020 Decadal Survey, concerns the physics of weakly collisional, high-beta plasmas -- plasmas in which the thermal pressure dominates over the magnetic pressure and in which the inter-particle collision time is comparable to the characteristic timescales of bulk motions. This state of matter, although widespread in the Universe, remains poorly understood: we lack a predictive theory for how it responds to perturbations, how it transports momentum and energy, and how it generates and amplifies magnetic fields. Such topics are foundational to the scient"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1903.04080","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":"1903.04080","created_at":"2026-05-17T23:51:40.107723+00:00"},{"alias_kind":"arxiv_version","alias_value":"1903.04080v1","created_at":"2026-05-17T23:51:40.107723+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1903.04080","created_at":"2026-05-17T23:51:40.107723+00:00"},{"alias_kind":"pith_short_12","alias_value":"QYHRGD2LFTXD","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_16","alias_value":"QYHRGD2LFTXDUADB","created_at":"2026-05-18T12:33:27.125529+00:00"},{"alias_kind":"pith_short_8","alias_value":"QYHRGD2L","created_at":"2026-05-18T12:33:27.125529+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/QYHRGD2LFTXDUADB3OKBIPHTGZ","json":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ.json","graph_json":"https://pith.science/api/pith-number/QYHRGD2LFTXDUADB3OKBIPHTGZ/graph.json","events_json":"https://pith.science/api/pith-number/QYHRGD2LFTXDUADB3OKBIPHTGZ/events.json","paper":"https://pith.science/paper/QYHRGD2L"},"agent_actions":{"view_html":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ","download_json":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ.json","view_paper":"https://pith.science/paper/QYHRGD2L","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1903.04080&json=true","fetch_graph":"https://pith.science/api/pith-number/QYHRGD2LFTXDUADB3OKBIPHTGZ/graph.json","fetch_events":"https://pith.science/api/pith-number/QYHRGD2LFTXDUADB3OKBIPHTGZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ/action/storage_attestation","attest_author":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ/action/author_attestation","sign_citation":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ/action/citation_signature","submit_replication":"https://pith.science/pith/QYHRGD2LFTXDUADB3OKBIPHTGZ/action/replication_record"}},"created_at":"2026-05-17T23:51:40.107723+00:00","updated_at":"2026-05-17T23:51:40.107723+00:00"}