{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2015:DBOWA7FEHO3ZOAR6TCT26UDFTD","short_pith_number":"pith:DBOWA7FE","schema_version":"1.0","canonical_sha256":"185d607ca43bb797023e98a7af506598cd2495ff4d2a3e6c2359b1e2ca8266d5","source":{"kind":"arxiv","id":"1510.08176","version":1},"attestation_state":"computed","paper":{"title":"Thermodynamical Analysis of a Black Hole with a Global Monopole Within a Class of a f(R) Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Cristine N. Ferreira, F. B. Lustosa, J. L. Neto, M.E.X. Guimar\\~aes","submitted_at":"2015-10-28T03:16:06Z","abstract_excerpt":"We analyze the thermodynamics of a black hole in a region that contains a global monopole in the framework of a particular class of a f(R) gravity. Specifically, we study the case in which df(R)/dR = F(R) is a power law function of the radial coordinate of the monopole spacetime, i.e., F(r) = 1 + \\psi_n r^n, where \\psi_n is the fine-tuned parameter corresponding to the f(R) gravity. We obtain explicit expressions for the local thermodynamic quantities of the black hole as a function of the event horizon, the parameter describing the monopole and the measurable corrections due to the f(R) theor"},"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":"1510.08176","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2015-10-28T03:16:06Z","cross_cats_sorted":[],"title_canon_sha256":"85eef817417ffede24c51e602d241da808a6bd696adec6205414e6504fa7f66b","abstract_canon_sha256":"5b8b05313b576b229ecf9eb3112702d5d5d7e2c90b705d765127b831305e9eeb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T01:28:37.012242Z","signature_b64":"QoDGxUoPnC/dknrx50HEyGjyWl4Gl0pPB3vSupPUpjOmSzbBVUkT6yc48mEJwgAJK7+ROuhtSKp4k1/eRGrcAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"185d607ca43bb797023e98a7af506598cd2495ff4d2a3e6c2359b1e2ca8266d5","last_reissued_at":"2026-05-18T01:28:37.011618Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T01:28:37.011618Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Thermodynamical Analysis of a Black Hole with a Global Monopole Within a Class of a f(R) Gravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Cristine N. Ferreira, F. B. Lustosa, J. L. Neto, M.E.X. Guimar\\~aes","submitted_at":"2015-10-28T03:16:06Z","abstract_excerpt":"We analyze the thermodynamics of a black hole in a region that contains a global monopole in the framework of a particular class of a f(R) gravity. Specifically, we study the case in which df(R)/dR = F(R) is a power law function of the radial coordinate of the monopole spacetime, i.e., F(r) = 1 + \\psi_n r^n, where \\psi_n is the fine-tuned parameter corresponding to the f(R) gravity. We obtain explicit expressions for the local thermodynamic quantities of the black hole as a function of the event horizon, the parameter describing the monopole and the measurable corrections due to the f(R) theor"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1510.08176","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":"1510.08176","created_at":"2026-05-18T01:28:37.011719+00:00"},{"alias_kind":"arxiv_version","alias_value":"1510.08176v1","created_at":"2026-05-18T01:28:37.011719+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1510.08176","created_at":"2026-05-18T01:28:37.011719+00:00"},{"alias_kind":"pith_short_12","alias_value":"DBOWA7FEHO3Z","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_16","alias_value":"DBOWA7FEHO3ZOAR6","created_at":"2026-05-18T12:29:17.054201+00:00"},{"alias_kind":"pith_short_8","alias_value":"DBOWA7FE","created_at":"2026-05-18T12:29:17.054201+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.08201","citing_title":"The instability of a black hole with $f(R)$ global monopole under extended uncertainty principle","ref_index":15,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD","json":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD.json","graph_json":"https://pith.science/api/pith-number/DBOWA7FEHO3ZOAR6TCT26UDFTD/graph.json","events_json":"https://pith.science/api/pith-number/DBOWA7FEHO3ZOAR6TCT26UDFTD/events.json","paper":"https://pith.science/paper/DBOWA7FE"},"agent_actions":{"view_html":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD","download_json":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD.json","view_paper":"https://pith.science/paper/DBOWA7FE","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1510.08176&json=true","fetch_graph":"https://pith.science/api/pith-number/DBOWA7FEHO3ZOAR6TCT26UDFTD/graph.json","fetch_events":"https://pith.science/api/pith-number/DBOWA7FEHO3ZOAR6TCT26UDFTD/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD/action/timestamp_anchor","attest_storage":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD/action/storage_attestation","attest_author":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD/action/author_attestation","sign_citation":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD/action/citation_signature","submit_replication":"https://pith.science/pith/DBOWA7FEHO3ZOAR6TCT26UDFTD/action/replication_record"}},"created_at":"2026-05-18T01:28:37.011719+00:00","updated_at":"2026-05-18T01:28:37.011719+00:00"}