{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2012:CSDRU7WJLIGQXIPPHGSXPE3GF3","short_pith_number":"pith:CSDRU7WJ","schema_version":"1.0","canonical_sha256":"14871a7ec95a0d0ba1ef39a57793662efcbbef5d918c7be49c64020f5880f657","source":{"kind":"arxiv","id":"1206.4738","version":3},"attestation_state":"computed","paper":{"title":"Quasi-topological Reissner-Nordstr\\\"om Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"R. B. Mann, W. G. Brenna","submitted_at":"2012-06-20T23:16:32Z","abstract_excerpt":"We consider Reissner-Nordstrom solutions in quasi-topological gravity, obtaining exact solutions to the field equations yielding charged quasi-topological black holes. We study their thermodynamic behaviour over a range of parameters that yield ghost-free and stable space times. We find that a sufficiently negative quasi-topological parameter can yield black holes with 2 horizons, even for zero charge. We discuss the thermodynamic stability for the class of solutions we obtain. We also describe the structure of exact charged solutions to $k^{th}$ order quasi-topological gravity."},"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":"1206.4738","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2012-06-20T23:16:32Z","cross_cats_sorted":[],"title_canon_sha256":"c0703d8cfef0ce240b44a79e1a39c5715247ac45512a621cecda82f9e3fe99b8","abstract_canon_sha256":"8424f27a72704d728822086734fa8fe69f449d660dcadb18bc59242df86e6da9"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T03:43:20.346018Z","signature_b64":"5+p427V1g5NPb44CtK7hNEoGXxfmoeqG548oj8D2O4tEkjEpHgotuXE4tAnjOs/lXpZSAjNudAbomsiMrrvhDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"14871a7ec95a0d0ba1ef39a57793662efcbbef5d918c7be49c64020f5880f657","last_reissued_at":"2026-05-18T03:43:20.345489Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T03:43:20.345489Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Quasi-topological Reissner-Nordstr\\\"om Black Holes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"R. B. Mann, W. G. Brenna","submitted_at":"2012-06-20T23:16:32Z","abstract_excerpt":"We consider Reissner-Nordstrom solutions in quasi-topological gravity, obtaining exact solutions to the field equations yielding charged quasi-topological black holes. We study their thermodynamic behaviour over a range of parameters that yield ghost-free and stable space times. We find that a sufficiently negative quasi-topological parameter can yield black holes with 2 horizons, even for zero charge. We discuss the thermodynamic stability for the class of solutions we obtain. We also describe the structure of exact charged solutions to $k^{th}$ order quasi-topological gravity."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1206.4738","kind":"arxiv","version":3},"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":"1206.4738","created_at":"2026-05-18T03:43:20.345569+00:00"},{"alias_kind":"arxiv_version","alias_value":"1206.4738v3","created_at":"2026-05-18T03:43:20.345569+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1206.4738","created_at":"2026-05-18T03:43:20.345569+00:00"},{"alias_kind":"pith_short_12","alias_value":"CSDRU7WJLIGQ","created_at":"2026-05-18T12:27:01.376967+00:00"},{"alias_kind":"pith_short_16","alias_value":"CSDRU7WJLIGQXIPP","created_at":"2026-05-18T12:27:01.376967+00:00"},{"alias_kind":"pith_short_8","alias_value":"CSDRU7WJ","created_at":"2026-05-18T12:27:01.376967+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2608.05268","citing_title":"Living on the Edge of Effective Field Theory: Near-Extremal Black Holes in Quadratic Gravity","ref_index":37,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3","json":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3.json","graph_json":"https://pith.science/api/pith-number/CSDRU7WJLIGQXIPPHGSXPE3GF3/graph.json","events_json":"https://pith.science/api/pith-number/CSDRU7WJLIGQXIPPHGSXPE3GF3/events.json","paper":"https://pith.science/paper/CSDRU7WJ"},"agent_actions":{"view_html":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3","download_json":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3.json","view_paper":"https://pith.science/paper/CSDRU7WJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1206.4738&json=true","fetch_graph":"https://pith.science/api/pith-number/CSDRU7WJLIGQXIPPHGSXPE3GF3/graph.json","fetch_events":"https://pith.science/api/pith-number/CSDRU7WJLIGQXIPPHGSXPE3GF3/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3/action/storage_attestation","attest_author":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3/action/author_attestation","sign_citation":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3/action/citation_signature","submit_replication":"https://pith.science/pith/CSDRU7WJLIGQXIPPHGSXPE3GF3/action/replication_record"}},"created_at":"2026-05-18T03:43:20.345569+00:00","updated_at":"2026-05-18T03:43:20.345569+00:00"}