{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2012:MEMZRF65XJZFUNNADXZNT3HTI4","short_pith_number":"pith:MEMZRF65","canonical_record":{"source":{"id":"1201.1839","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-01-09T17:01:46Z","cross_cats_sorted":[],"title_canon_sha256":"ce0ad60832dacf5a4b7088e3eeeaa27a615a33568e9976fb5116b140f510c30e","abstract_canon_sha256":"a61c1aaf1be35e805ecc60c8677df7551aa7ccff4ba8421bd6f1e37d2f807cbc"},"schema_version":"1.0"},"canonical_sha256":"61199897ddba725a35a01df2d9ecf34734a2cdff8df6d9f6ada0dec11e1970e9","source":{"kind":"arxiv","id":"1201.1839","version":1},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1201.1839","created_at":"2026-05-18T01:58:54Z"},{"alias_kind":"arxiv_version","alias_value":"1201.1839v1","created_at":"2026-05-18T01:58:54Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.1839","created_at":"2026-05-18T01:58:54Z"},{"alias_kind":"pith_short_12","alias_value":"MEMZRF65XJZF","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_16","alias_value":"MEMZRF65XJZFUNNA","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_8","alias_value":"MEMZRF65","created_at":"2026-05-18T12:27:14Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2012:MEMZRF65XJZFUNNADXZNT3HTI4","target":"record","payload":{"canonical_record":{"source":{"id":"1201.1839","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-01-09T17:01:46Z","cross_cats_sorted":[],"title_canon_sha256":"ce0ad60832dacf5a4b7088e3eeeaa27a615a33568e9976fb5116b140f510c30e","abstract_canon_sha256":"a61c1aaf1be35e805ecc60c8677df7551aa7ccff4ba8421bd6f1e37d2f807cbc"},"schema_version":"1.0"},"canonical_sha256":"61199897ddba725a35a01df2d9ecf34734a2cdff8df6d9f6ada0dec11e1970e9","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:58:54.000790Z","signature_b64":"/f9d6NU4bl+1RJkbzRwIStPk4werWkp0XYjrRS+K6mirzsuOpqfL97rAjY7tgiXs7m2zCBP38nNx7LBddJ7eAw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"61199897ddba725a35a01df2d9ecf34734a2cdff8df6d9f6ada0dec11e1970e9","last_reissued_at":"2026-05-18T01:58:54.000039Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:58:54.000039Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"1201.1839","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":"2026-05-18T01:58:54Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"E3lVzj8hd+ZgPgWx4UBMbra3T/o/hS22ycHJS643mWk020TYwZGgq0MLWEBZIG4OsyFsA9G1bbPJlMTkLgmyAA==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T11:47:47.467844Z"},"content_sha256":"dee5481bc4255c9da269de0d8df1872cb22353e8c5b36a203cc304911e625508","schema_version":"1.0","event_id":"sha256:dee5481bc4255c9da269de0d8df1872cb22353e8c5b36a203cc304911e625508"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2012:MEMZRF65XJZFUNNADXZNT3HTI4","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Absolute stability of axisymmetric perturbations in strongly-magnetized collisionless axisymmetric accretion disk plasmas","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"astro-ph.HE","authors_text":"C. Cremaschini, J. C. Miller, M. Tessarotto","submitted_at":"2012-01-09T17:01:46Z","abstract_excerpt":"The physical mechanism responsible for driving accretion flows in astrophysical accretion disks is commonly thought to be related to the development of plasma instabilities and turbulence. A key question is therefore the determination of consistent equilibrium configurations for accretion-disk plasmas and investigation of their stability properties. In the case of collisionless plasmas kinetic theory provides the appropriate theoretical framework. This paper presents a kinetic description of low-frequency and long-wavelength axisymmetric electromagnetic perturbations in non-relativistic, stron"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.1839","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":"2026-05-18T01:58:54Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"sJWmUbX9Bzr88sCcBoqXWkhlswzizYNCVuNuxTiJmW8xWrLIN4c7OfcRqRi5lNyNRVaNRqp4JxMnrE4u7m5bCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-05-26T11:47:47.468515Z"},"content_sha256":"052687a6d5c2293f94b146d0cb26f8ee0791536f7a5dc06493a2bb4c4ed6f74f","schema_version":"1.0","event_id":"sha256:052687a6d5c2293f94b146d0cb26f8ee0791536f7a5dc06493a2bb4c4ed6f74f"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/MEMZRF65XJZFUNNADXZNT3HTI4/bundle.json","state_url":"https://pith.science/pith/MEMZRF65XJZFUNNADXZNT3HTI4/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/MEMZRF65XJZFUNNADXZNT3HTI4/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":"2026-05-26T11:47:47Z","links":{"resolver":"https://pith.science/pith/MEMZRF65XJZFUNNADXZNT3HTI4","bundle":"https://pith.science/pith/MEMZRF65XJZFUNNADXZNT3HTI4/bundle.json","state":"https://pith.science/pith/MEMZRF65XJZFUNNADXZNT3HTI4/state.json","well_known_bundle":"https://pith.science/.well-known/pith/MEMZRF65XJZFUNNADXZNT3HTI4/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2012:MEMZRF65XJZFUNNADXZNT3HTI4","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":"a61c1aaf1be35e805ecc60c8677df7551aa7ccff4ba8421bd6f1e37d2f807cbc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-01-09T17:01:46Z","title_canon_sha256":"ce0ad60832dacf5a4b7088e3eeeaa27a615a33568e9976fb5116b140f510c30e"},"schema_version":"1.0","source":{"id":"1201.1839","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1201.1839","created_at":"2026-05-18T01:58:54Z"},{"alias_kind":"arxiv_version","alias_value":"1201.1839v1","created_at":"2026-05-18T01:58:54Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1201.1839","created_at":"2026-05-18T01:58:54Z"},{"alias_kind":"pith_short_12","alias_value":"MEMZRF65XJZF","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_16","alias_value":"MEMZRF65XJZFUNNA","created_at":"2026-05-18T12:27:14Z"},{"alias_kind":"pith_short_8","alias_value":"MEMZRF65","created_at":"2026-05-18T12:27:14Z"}],"graph_snapshots":[{"event_id":"sha256:052687a6d5c2293f94b146d0cb26f8ee0791536f7a5dc06493a2bb4c4ed6f74f","target":"graph","created_at":"2026-05-18T01:58:54Z","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":"The physical mechanism responsible for driving accretion flows in astrophysical accretion disks is commonly thought to be related to the development of plasma instabilities and turbulence. A key question is therefore the determination of consistent equilibrium configurations for accretion-disk plasmas and investigation of their stability properties. In the case of collisionless plasmas kinetic theory provides the appropriate theoretical framework. This paper presents a kinetic description of low-frequency and long-wavelength axisymmetric electromagnetic perturbations in non-relativistic, stron","authors_text":"C. Cremaschini, J. C. Miller, M. Tessarotto","cross_cats":[],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-01-09T17:01:46Z","title":"Absolute stability of axisymmetric perturbations in strongly-magnetized collisionless axisymmetric accretion disk plasmas"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1201.1839","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:dee5481bc4255c9da269de0d8df1872cb22353e8c5b36a203cc304911e625508","target":"record","created_at":"2026-05-18T01:58:54Z","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":"a61c1aaf1be35e805ecc60c8677df7551aa7ccff4ba8421bd6f1e37d2f807cbc","cross_cats_sorted":[],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.HE","submitted_at":"2012-01-09T17:01:46Z","title_canon_sha256":"ce0ad60832dacf5a4b7088e3eeeaa27a615a33568e9976fb5116b140f510c30e"},"schema_version":"1.0","source":{"id":"1201.1839","kind":"arxiv","version":1}},"canonical_sha256":"61199897ddba725a35a01df2d9ecf34734a2cdff8df6d9f6ada0dec11e1970e9","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"61199897ddba725a35a01df2d9ecf34734a2cdff8df6d9f6ada0dec11e1970e9","first_computed_at":"2026-05-18T01:58:54.000039Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:58:54.000039Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"/f9d6NU4bl+1RJkbzRwIStPk4werWkp0XYjrRS+K6mirzsuOpqfL97rAjY7tgiXs7m2zCBP38nNx7LBddJ7eAw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:58:54.000790Z","signed_message":"canonical_sha256_bytes"},"source_id":"1201.1839","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:dee5481bc4255c9da269de0d8df1872cb22353e8c5b36a203cc304911e625508","sha256:052687a6d5c2293f94b146d0cb26f8ee0791536f7a5dc06493a2bb4c4ed6f74f"],"state_sha256":"8fbd5999b332b1ea586073066bd69f240ab432008123673fd88384cc5858fcf7"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"a2r1+lcYAsr2GVPKZ2F7EEx2Fsiz+r4dh0vI1ATnyf0tPWZY87ZbXbzBw4YSB+GibOfxrFkcZNxQBV+veVY2DA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-05-26T11:47:47.472789Z","bundle_sha256":"c8a2f67db18fa93309af32a6af7b8c45c77b7df740221918fd696eae4d1d7da2"}}