{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:FZ42JSCX2TNGQKOFHKCDC6LGLL","short_pith_number":"pith:FZ42JSCX","schema_version":"1.0","canonical_sha256":"2e79a4c857d4da6829c53a843179665ac2023bd07ac03a72ab4db3cb8321dc70","source":{"kind":"arxiv","id":"hep-th/0602069","version":2},"attestation_state":"computed","paper":{"title":"Taub-NUT/Bolt Black Holes in Gauss-Bonnet-Maxwell Gravity","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"M. H. Dehghani, S. H. Hendi","submitted_at":"2006-02-07T12:24:29Z","abstract_excerpt":"We present a class of higher dimensional solutions to Gauss-Bonnet-Maxwell equations in $2k+2$ dimensions with a U(1) fibration over a $2k$-dimensional base space $\\mathcal{B}$. These solutions depend on two extra parameters, other than the mass and the NUT charge, which are the electric charge $q$ and the electric potential at infinity $V$. We find that the form of metric is sensitive to geometry of the base space, while the form of electromagnetic field is independent of $\\mathcal{B}$. We investigate the existence of Taub-NUT/bolt solutions and find that in addition to the two conditions of "},"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/0602069","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2006-02-07T12:24:29Z","cross_cats_sorted":[],"title_canon_sha256":"8ba9d60086920bab956e20b3c47f977d6cc87da3fdd45520806e3c1fa99a3140","abstract_canon_sha256":"50e7b3e4f49d6201fd6049ff70339413d253b79f2806920927503e903262b6ac"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:19:57.150522Z","signature_b64":"REi0k3ksvWPxmJpd0NhgGX9GzZFECmXDajSQL5EGrUpbxWY1awNAA6roHpG0rCyokqwtm4FeTcDl3V7+2ltZAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2e79a4c857d4da6829c53a843179665ac2023bd07ac03a72ab4db3cb8321dc70","last_reissued_at":"2026-07-04T15:19:57.150075Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:19:57.150075Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Taub-NUT/Bolt Black Holes in Gauss-Bonnet-Maxwell Gravity","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"M. H. Dehghani, S. H. Hendi","submitted_at":"2006-02-07T12:24:29Z","abstract_excerpt":"We present a class of higher dimensional solutions to Gauss-Bonnet-Maxwell equations in $2k+2$ dimensions with a U(1) fibration over a $2k$-dimensional base space $\\mathcal{B}$. These solutions depend on two extra parameters, other than the mass and the NUT charge, which are the electric charge $q$ and the electric potential at infinity $V$. We find that the form of metric is sensitive to geometry of the base space, while the form of electromagnetic field is independent of $\\mathcal{B}$. We investigate the existence of Taub-NUT/bolt solutions and find that in addition to the two conditions of "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0602069","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-th/0602069/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"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/0602069","created_at":"2026-07-04T15:19:57.150139+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0602069v2","created_at":"2026-07-04T15:19:57.150139+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0602069","created_at":"2026-07-04T15:19:57.150139+00:00"},{"alias_kind":"pith_short_12","alias_value":"FZ42JSCX2TNG","created_at":"2026-07-04T15:19:57.150139+00:00"},{"alias_kind":"pith_short_16","alias_value":"FZ42JSCX2TNGQKOF","created_at":"2026-07-04T15:19:57.150139+00:00"},{"alias_kind":"pith_short_8","alias_value":"FZ42JSCX","created_at":"2026-07-04T15:19:57.150139+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":2,"sample":[{"citing_arxiv_id":"2606.17784","citing_title":"Quasi-topological gravity for 4-dimensional Taub-NUT, near-horizon extreme Kerr, and swirling symmetries","ref_index":48,"is_internal_anchor":true},{"citing_arxiv_id":"2605.14668","citing_title":"$\\alpha'$ corrections to self-dual gravitational instantons","ref_index":47,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL","json":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL.json","graph_json":"https://pith.science/api/pith-number/FZ42JSCX2TNGQKOFHKCDC6LGLL/graph.json","events_json":"https://pith.science/api/pith-number/FZ42JSCX2TNGQKOFHKCDC6LGLL/events.json","paper":"https://pith.science/paper/FZ42JSCX"},"agent_actions":{"view_html":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL","download_json":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL.json","view_paper":"https://pith.science/paper/FZ42JSCX","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0602069&json=true","fetch_graph":"https://pith.science/api/pith-number/FZ42JSCX2TNGQKOFHKCDC6LGLL/graph.json","fetch_events":"https://pith.science/api/pith-number/FZ42JSCX2TNGQKOFHKCDC6LGLL/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL/action/storage_attestation","attest_author":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL/action/author_attestation","sign_citation":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL/action/citation_signature","submit_replication":"https://pith.science/pith/FZ42JSCX2TNGQKOFHKCDC6LGLL/action/replication_record"}},"created_at":"2026-07-04T15:19:57.150139+00:00","updated_at":"2026-07-04T15:19:57.150139+00:00"}