{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2011:RGGPKJVZNS25ATKJQUYS76KIRQ","short_pith_number":"pith:RGGPKJVZ","canonical_record":{"source":{"id":"1107.1308","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-07-07T07:12:46Z","cross_cats_sorted":[],"title_canon_sha256":"14a28b97f93d82cd7095838d345466e945f1d730c4d21371b66c9f11c0b9d4a2","abstract_canon_sha256":"5d92388d6c9434b5eca23ca0a15b9d8f176d24406b647a38b37342c910191d88"},"schema_version":"1.0"},"canonical_sha256":"898cf526b96cb5d04d4985312ff9488c02e29a16d728cd8e757d18afa6e8863b","source":{"kind":"arxiv","id":"1107.1308","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1107.1308","created_at":"2026-05-18T03:42:55Z"},{"alias_kind":"arxiv_version","alias_value":"1107.1308v1","created_at":"2026-05-18T03:42:55Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.1308","created_at":"2026-05-18T03:42:55Z"},{"alias_kind":"pith_short_12","alias_value":"RGGPKJVZNS25","created_at":"2026-05-18T12:26:41Z"},{"alias_kind":"pith_short_16","alias_value":"RGGPKJVZNS25ATKJ","created_at":"2026-05-18T12:26:41Z"},{"alias_kind":"pith_short_8","alias_value":"RGGPKJVZ","created_at":"2026-05-18T12:26:41Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2011:RGGPKJVZNS25ATKJQUYS76KIRQ","target":"record","payload":{"canonical_record":{"source":{"id":"1107.1308","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-07-07T07:12:46Z","cross_cats_sorted":[],"title_canon_sha256":"14a28b97f93d82cd7095838d345466e945f1d730c4d21371b66c9f11c0b9d4a2","abstract_canon_sha256":"5d92388d6c9434b5eca23ca0a15b9d8f176d24406b647a38b37342c910191d88"},"schema_version":"1.0"},"canonical_sha256":"898cf526b96cb5d04d4985312ff9488c02e29a16d728cd8e757d18afa6e8863b","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:42:55.908899Z","signature_b64":"yXDkMyESfSPv/5A52IzhYC3PHpGb0wLow5vV6uut6kVpD0OLYut6Nr2thq0hblohnAKo90vdi5x3hw9GUiJ/Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"898cf526b96cb5d04d4985312ff9488c02e29a16d728cd8e757d18afa6e8863b","last_reissued_at":"2026-05-18T03:42:55.908361Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:42:55.908361Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1107.1308","source_version":1,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:42:55Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Is5kHj8ht3zofNcnehk2ZfLLQpeUX3v9RX2zbF7qoqxxYWzAp+1xGnyJTymkXcoKchFTCDiZLSDeW2jP1jMQDg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T03:10:20.428824Z"},"content_sha256":"0885ab70d880c5de5b1ad36fb67dd385499d2bed16ff02f539dba9fe0947c16f","schema_version":"1.0","event_id":"sha256:0885ab70d880c5de5b1ad36fb67dd385499d2bed16ff02f539dba9fe0947c16f"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2011:RGGPKJVZNS25ATKJQUYS76KIRQ","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Drift wave turbulence in a dense semiclassical magnetoplasma","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"physics.plasm-ph","authors_text":"Alexander Kendl, Padma K. Shukla","submitted_at":"2011-07-07T07:12:46Z","abstract_excerpt":"A semiclassical nonlinear collisional drift wave model for dense magnetized plasmas is developed and solved numerically. The effects of fluid electron density fluctuations associated with quantum statistical pressure and quantum Bohm force are included, and their influences on the collisional drift wave instability and the resulting fully developed nanoscale drift wave turbulence are discussed. It is found that the quantum effects increase the growth rate of the collisional drift wave instability, and introduce a finite de Broglie length screening on the drift wave turbulent density perturbati"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.1308","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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-05-18T03:42:55Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"2+E4iJGFj0JCypovkfd0eVW86gY7BTY8GcPtyWnUmyvg3cN73zSDhBcanhZt3A/hMJE2w/dFNzsng+ayqi7sCg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-06-04T03:10:20.429474Z"},"content_sha256":"2901965fdd702a04eda0bb1ed139c091de587fb94ee7cf13c64bd95f890fe0fe","schema_version":"1.0","event_id":"sha256:2901965fdd702a04eda0bb1ed139c091de587fb94ee7cf13c64bd95f890fe0fe"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/RGGPKJVZNS25ATKJQUYS76KIRQ/bundle.json","state_url":"https://pith.science/pith/RGGPKJVZNS25ATKJQUYS76KIRQ/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/RGGPKJVZNS25ATKJQUYS76KIRQ/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-06-04T03:10:20Z","links":{"resolver":"https://pith.science/pith/RGGPKJVZNS25ATKJQUYS76KIRQ","bundle":"https://pith.science/pith/RGGPKJVZNS25ATKJQUYS76KIRQ/bundle.json","state":"https://pith.science/pith/RGGPKJVZNS25ATKJQUYS76KIRQ/state.json","well_known_bundle":"https://pith.science/.well-known/pith/RGGPKJVZNS25ATKJQUYS76KIRQ/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2011:RGGPKJVZNS25ATKJQUYS76KIRQ","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"5d92388d6c9434b5eca23ca0a15b9d8f176d24406b647a38b37342c910191d88","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-07-07T07:12:46Z","title_canon_sha256":"14a28b97f93d82cd7095838d345466e945f1d730c4d21371b66c9f11c0b9d4a2"},"schema_version":"1.0","source":{"id":"1107.1308","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1107.1308","created_at":"2026-05-18T03:42:55Z"},{"alias_kind":"arxiv_version","alias_value":"1107.1308v1","created_at":"2026-05-18T03:42:55Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1107.1308","created_at":"2026-05-18T03:42:55Z"},{"alias_kind":"pith_short_12","alias_value":"RGGPKJVZNS25","created_at":"2026-05-18T12:26:41Z"},{"alias_kind":"pith_short_16","alias_value":"RGGPKJVZNS25ATKJ","created_at":"2026-05-18T12:26:41Z"},{"alias_kind":"pith_short_8","alias_value":"RGGPKJVZ","created_at":"2026-05-18T12:26:41Z"}],"graph_snapshots":[{"event_id":"sha256:2901965fdd702a04eda0bb1ed139c091de587fb94ee7cf13c64bd95f890fe0fe","target":"graph","created_at":"2026-05-18T03:42:55Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"A semiclassical nonlinear collisional drift wave model for dense magnetized plasmas is developed and solved numerically. The effects of fluid electron density fluctuations associated with quantum statistical pressure and quantum Bohm force are included, and their influences on the collisional drift wave instability and the resulting fully developed nanoscale drift wave turbulence are discussed. It is found that the quantum effects increase the growth rate of the collisional drift wave instability, and introduce a finite de Broglie length screening on the drift wave turbulent density perturbati","authors_text":"Alexander Kendl, Padma K. Shukla","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-07-07T07:12:46Z","title":"Drift wave turbulence in a dense semiclassical magnetoplasma"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1107.1308","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:0885ab70d880c5de5b1ad36fb67dd385499d2bed16ff02f539dba9fe0947c16f","target":"record","created_at":"2026-05-18T03:42:55Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"5d92388d6c9434b5eca23ca0a15b9d8f176d24406b647a38b37342c910191d88","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.plasm-ph","submitted_at":"2011-07-07T07:12:46Z","title_canon_sha256":"14a28b97f93d82cd7095838d345466e945f1d730c4d21371b66c9f11c0b9d4a2"},"schema_version":"1.0","source":{"id":"1107.1308","kind":"arxiv","version":1}},"canonical_sha256":"898cf526b96cb5d04d4985312ff9488c02e29a16d728cd8e757d18afa6e8863b","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"898cf526b96cb5d04d4985312ff9488c02e29a16d728cd8e757d18afa6e8863b","first_computed_at":"2026-05-18T03:42:55.908361Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T03:42:55.908361Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"yXDkMyESfSPv/5A52IzhYC3PHpGb0wLow5vV6uut6kVpD0OLYut6Nr2thq0hblohnAKo90vdi5x3hw9GUiJ/Bw==","signature_status":"signed_v1","signed_at":"2026-05-18T03:42:55.908899Z","signed_message":"canonical_sha256_bytes"},"source_id":"1107.1308","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:0885ab70d880c5de5b1ad36fb67dd385499d2bed16ff02f539dba9fe0947c16f","sha256:2901965fdd702a04eda0bb1ed139c091de587fb94ee7cf13c64bd95f890fe0fe"],"state_sha256":"8a4c0af34aed4bded7cd0e8e404aff15e7809f1054865e177b69a55bdff1851f"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"yV8/Zn+jvWZE6dwZxJa/uJ6VLpMBYdKENVjJv+P1rnb6PId5MLPg0CZPPjNcQO8pPMVxu6CK/G+SHzU4Yl+fCA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-06-04T03:10:20.432729Z","bundle_sha256":"0093f5275dfbdf8812726db3df604c423558a342b72a3a3b3ff9465aab04fd63"}}