{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:6DLKPH3EIUGWZJEP3ZLY6534L3","short_pith_number":"pith:6DLKPH3E","schema_version":"1.0","canonical_sha256":"f0d6a79f64450d6ca48fde578f777c5efc86a713f71d3cff6553933d4d9b9fdf","source":{"kind":"arxiv","id":"1206.3890","version":2},"attestation_state":"computed","paper":{"title":"Thermal stability of a weakly magnetized rotating plasma","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.GA","authors_text":"Carlo Nipoti, Lorenzo Posti (Bologna University)","submitted_at":"2012-06-18T11:13:05Z","abstract_excerpt":"The thermal stability of a weakly magnetized, rotating, stratified, optically thin plasma is studied by means of linear-perturbation analysis. We derive dispersion relations and criteria for stability against axisymmetric perturbations that generalize previous results on either non-rotating or unmagnetized fluids. The implications for the hot atmospheres of galaxies and galaxy clusters are discussed."},"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":"1206.3890","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.GA","submitted_at":"2012-06-18T11:13:05Z","cross_cats_sorted":["physics.plasm-ph"],"title_canon_sha256":"daf2d0701b677686369b7dce227f3fcc830fb874433fcbe0231e0ee457ba40cc","abstract_canon_sha256":"72236d776ff1d78011dfa83aead6736addd1f3e0dff9794b6e80b1a6ea95b079"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:56:51.742187Z","signature_b64":"1dCxe28qZ8GJydmO/x4502OJnstJkUzXb1DJA++jNG6l31hfEgk1KGMprGwIwpn38z3AHoO7QXK7zuiYYt81AA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f0d6a79f64450d6ca48fde578f777c5efc86a713f71d3cff6553933d4d9b9fdf","last_reissued_at":"2026-05-18T01:56:51.741611Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:56:51.741611Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermal stability of a weakly magnetized rotating plasma","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["physics.plasm-ph"],"primary_cat":"astro-ph.GA","authors_text":"Carlo Nipoti, Lorenzo Posti (Bologna University)","submitted_at":"2012-06-18T11:13:05Z","abstract_excerpt":"The thermal stability of a weakly magnetized, rotating, stratified, optically thin plasma is studied by means of linear-perturbation analysis. We derive dispersion relations and criteria for stability against axisymmetric perturbations that generalize previous results on either non-rotating or unmagnetized fluids. The implications for the hot atmospheres of galaxies and galaxy clusters are discussed."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.3890","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":""},"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":"1206.3890","created_at":"2026-05-18T01:56:51.741686+00:00"},{"alias_kind":"arxiv_version","alias_value":"1206.3890v2","created_at":"2026-05-18T01:56:51.741686+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1206.3890","created_at":"2026-05-18T01:56:51.741686+00:00"},{"alias_kind":"pith_short_12","alias_value":"6DLKPH3EIUGW","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_16","alias_value":"6DLKPH3EIUGWZJEP","created_at":"2026-05-18T12:26:56.085431+00:00"},{"alias_kind":"pith_short_8","alias_value":"6DLKPH3E","created_at":"2026-05-18T12:26:56.085431+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/6DLKPH3EIUGWZJEP3ZLY6534L3","json":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3.json","graph_json":"https://pith.science/api/pith-number/6DLKPH3EIUGWZJEP3ZLY6534L3/graph.json","events_json":"https://pith.science/api/pith-number/6DLKPH3EIUGWZJEP3ZLY6534L3/events.json","paper":"https://pith.science/paper/6DLKPH3E"},"agent_actions":{"view_html":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3","download_json":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3.json","view_paper":"https://pith.science/paper/6DLKPH3E","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1206.3890&json=true","fetch_graph":"https://pith.science/api/pith-number/6DLKPH3EIUGWZJEP3ZLY6534L3/graph.json","fetch_events":"https://pith.science/api/pith-number/6DLKPH3EIUGWZJEP3ZLY6534L3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3/action/storage_attestation","attest_author":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3/action/author_attestation","sign_citation":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3/action/citation_signature","submit_replication":"https://pith.science/pith/6DLKPH3EIUGWZJEP3ZLY6534L3/action/replication_record"}},"created_at":"2026-05-18T01:56:51.741686+00:00","updated_at":"2026-05-18T01:56:51.741686+00:00"}