{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2009:BUIFVNV7U52BOQPJOLUKAGDO66","short_pith_number":"pith:BUIFVNV7","schema_version":"1.0","canonical_sha256":"0d105ab6bfa7741741e972e8a0186ef79190bda0aff4c2f9cb42607f807c7f57","source":{"kind":"arxiv","id":"0908.3918","version":2},"attestation_state":"computed","paper":{"title":"Black Holes in the Dilatonic Einstein-Gauss-Bonnet Theory in Various Dimensions IV - Topological Black Holes with and without Cosmological Term","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Nobuyoshi Ohta, Takashi Torii","submitted_at":"2009-08-26T23:57:25Z","abstract_excerpt":"We study black hole solutions in the Einstein gravity with Gauss-Bonnet term, the dilaton and a positive \"cosmological constant\" in various dimensions. Physically meaningful black holes with a positive cosmological term are obtained only for those in static spacetime with $(D-2)$-dimensional hyperbolic space of negative curvature and $D>4$. We construct such black hole solutions of various masses numerically in $D=5,6$ and 10 dimensional spacetime and discuss their properties. In spite of the positive cosmological constant the spacetime approach anti-de Sitter spacetime asymptotically. The bla"},"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":"0908.3918","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2009-08-26T23:57:25Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"c73ad6f5b8eda670c94d7d07816bdc505375c32ee390984a20aeb77f2a009be7","abstract_canon_sha256":"9cb67582b04fa044dd33808b6c2204f063b52c266cf24997ced46ed689492fd8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T02:34:37.334072Z","signature_b64":"FeZwGPCmPAuxFtNTt2KpgutarSNEwsHW3OXBc+83VJfme+UhtqfiJrhTQQW+5yDzKOqBuC30Y+f0ft4olBfHBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0d105ab6bfa7741741e972e8a0186ef79190bda0aff4c2f9cb42607f807c7f57","last_reissued_at":"2026-05-18T02:34:37.333424Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T02:34:37.333424Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Black Holes in the Dilatonic Einstein-Gauss-Bonnet Theory in Various Dimensions IV - Topological Black Holes with and without Cosmological Term","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Nobuyoshi Ohta, Takashi Torii","submitted_at":"2009-08-26T23:57:25Z","abstract_excerpt":"We study black hole solutions in the Einstein gravity with Gauss-Bonnet term, the dilaton and a positive \"cosmological constant\" in various dimensions. Physically meaningful black holes with a positive cosmological term are obtained only for those in static spacetime with $(D-2)$-dimensional hyperbolic space of negative curvature and $D>4$. We construct such black hole solutions of various masses numerically in $D=5,6$ and 10 dimensional spacetime and discuss their properties. In spite of the positive cosmological constant the spacetime approach anti-de Sitter spacetime asymptotically. The bla"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"0908.3918","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":""},"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":"0908.3918","created_at":"2026-05-18T02:34:37.333532+00:00"},{"alias_kind":"arxiv_version","alias_value":"0908.3918v2","created_at":"2026-05-18T02:34:37.333532+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.0908.3918","created_at":"2026-05-18T02:34:37.333532+00:00"},{"alias_kind":"pith_short_12","alias_value":"BUIFVNV7U52B","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_16","alias_value":"BUIFVNV7U52BOQPJ","created_at":"2026-05-18T12:25:58.837520+00:00"},{"alias_kind":"pith_short_8","alias_value":"BUIFVNV7","created_at":"2026-05-18T12:25:58.837520+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/BUIFVNV7U52BOQPJOLUKAGDO66","json":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66.json","graph_json":"https://pith.science/api/pith-number/BUIFVNV7U52BOQPJOLUKAGDO66/graph.json","events_json":"https://pith.science/api/pith-number/BUIFVNV7U52BOQPJOLUKAGDO66/events.json","paper":"https://pith.science/paper/BUIFVNV7"},"agent_actions":{"view_html":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66","download_json":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66.json","view_paper":"https://pith.science/paper/BUIFVNV7","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=0908.3918&json=true","fetch_graph":"https://pith.science/api/pith-number/BUIFVNV7U52BOQPJOLUKAGDO66/graph.json","fetch_events":"https://pith.science/api/pith-number/BUIFVNV7U52BOQPJOLUKAGDO66/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66/action/timestamp_anchor","attest_storage":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66/action/storage_attestation","attest_author":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66/action/author_attestation","sign_citation":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66/action/citation_signature","submit_replication":"https://pith.science/pith/BUIFVNV7U52BOQPJOLUKAGDO66/action/replication_record"}},"created_at":"2026-05-18T02:34:37.333532+00:00","updated_at":"2026-05-18T02:34:37.333532+00:00"}