{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1994:A6C3CLCOZL45RVTSCLTLTW4ROC","short_pith_number":"pith:A6C3CLCO","schema_version":"1.0","canonical_sha256":"0785b12c4ecaf9d8d67212e6b9db9170baaad55b0d8d19ee65d5a19561f81ce7","source":{"kind":"arxiv","id":"hep-th/9409013","version":1},"attestation_state":"computed","paper":{"title":"Instabilities of Magnetically Charged Black Holes","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Erick J. Weinberg, S. Alexander Ridgway","submitted_at":"1994-09-02T20:36:34Z","abstract_excerpt":"The stability of the magnetically charged Reissner-Nordstrom black hole solution is investigated in the context of a theory with massive charged vector mesons. By exploiting the spherical symmetry of the problem, the linear perturbations about the Reissner-Nordstrom solution can be decomposed into modes of definite angular momentum $J$. For each value of $J$, unstable modes appear if the horizon radius is less than a critical value that depends on the vector meson gyromagnetic ratio $g$ and the monopole magnetic charge $q/e$. It is shown that such a critical radius exists (except in the anomal"},"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":"hep-th/9409013","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1994-09-02T20:36:34Z","cross_cats_sorted":[],"title_canon_sha256":"a0e94a0c145116407622449b44482d80168a96fbadf20d6ca092c37944b9eb72","abstract_canon_sha256":"6fc661ffdec495848b94da0b57af310a831e4f0689c7ce166f655d552d71edad"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:37:34.884208Z","signature_b64":"tSA9voQMM6/rQZKlg91eSm1tWRYAWVwfqDi/Igzz8LXb9ZqJ29zpwHqKooiRJa6q1vsx3a0/xBOAbaRTfRDHBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0785b12c4ecaf9d8d67212e6b9db9170baaad55b0d8d19ee65d5a19561f81ce7","last_reissued_at":"2026-05-18T04:37:34.883665Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:37:34.883665Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Instabilities of Magnetically Charged Black Holes","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Erick J. Weinberg, S. Alexander Ridgway","submitted_at":"1994-09-02T20:36:34Z","abstract_excerpt":"The stability of the magnetically charged Reissner-Nordstrom black hole solution is investigated in the context of a theory with massive charged vector mesons. By exploiting the spherical symmetry of the problem, the linear perturbations about the Reissner-Nordstrom solution can be decomposed into modes of definite angular momentum $J$. For each value of $J$, unstable modes appear if the horizon radius is less than a critical value that depends on the vector meson gyromagnetic ratio $g$ and the monopole magnetic charge $q/e$. It is shown that such a critical radius exists (except in the anomal"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9409013","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":"hep-th/9409013","created_at":"2026-05-18T04:37:34.883739+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9409013v1","created_at":"2026-05-18T04:37:34.883739+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9409013","created_at":"2026-05-18T04:37:34.883739+00:00"},{"alias_kind":"pith_short_12","alias_value":"A6C3CLCOZL45","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_16","alias_value":"A6C3CLCOZL45RVTS","created_at":"2026-05-18T12:25:47.102015+00:00"},{"alias_kind":"pith_short_8","alias_value":"A6C3CLCO","created_at":"2026-05-18T12:25:47.102015+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/A6C3CLCOZL45RVTSCLTLTW4ROC","json":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC.json","graph_json":"https://pith.science/api/pith-number/A6C3CLCOZL45RVTSCLTLTW4ROC/graph.json","events_json":"https://pith.science/api/pith-number/A6C3CLCOZL45RVTSCLTLTW4ROC/events.json","paper":"https://pith.science/paper/A6C3CLCO"},"agent_actions":{"view_html":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC","download_json":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC.json","view_paper":"https://pith.science/paper/A6C3CLCO","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9409013&json=true","fetch_graph":"https://pith.science/api/pith-number/A6C3CLCOZL45RVTSCLTLTW4ROC/graph.json","fetch_events":"https://pith.science/api/pith-number/A6C3CLCOZL45RVTSCLTLTW4ROC/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC/action/timestamp_anchor","attest_storage":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC/action/storage_attestation","attest_author":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC/action/author_attestation","sign_citation":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC/action/citation_signature","submit_replication":"https://pith.science/pith/A6C3CLCOZL45RVTSCLTLTW4ROC/action/replication_record"}},"created_at":"2026-05-18T04:37:34.883739+00:00","updated_at":"2026-05-18T04:37:34.883739+00:00"}