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The theory is formulated in the metric-affine (or Palatini) formalism and exact analytical solutions are obtained. For $\\lambda<0$, one finds that the solution has the same characteristics as the Schwarzschild black hole with a monopole charge in Einstein's GR. For $\\lambda>0$, instead, the metric is more closely related to the Reissner-Nordstr\\\"{o}m metric with a monopole charge and, in addition, it possesses a wormhole-lik"},"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":"1812.00471","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"gr-qc","submitted_at":"2018-12-02T21:40:57Z","cross_cats_sorted":[],"title_canon_sha256":"5398817cdf5bef13aaf6c4c88ac32bd9c3d3cc6679262cf057308e1f22e5b632","abstract_canon_sha256":"d86efc9d78053d27252af3bdc1303987dcc9609f8a7287b7bb45fcc28a7506b9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-17T23:49:40.277641Z","signature_b64":"eXADLrozCVpQYl1WUc6+wgKYxs9ajobQtD7nUEDD9/6AUcQo2HM34HUPuRxl2fH2PcCjlSgRqGpIgxHssP0SCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"041fe06e738134fb7b019ddb355c4a0a2e943d003173e7dcc95c8bc90e33fffc","last_reissued_at":"2026-05-17T23:49:40.277094Z","signature_status":"signed_v1","first_computed_at":"2026-05-17T23:49:40.277094Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Global Monopole in Palatini f(R) gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"gr-qc","authors_text":"A. 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