{"bundle_type":"pith_open_graph_bundle","bundle_version":"1.0","pith_number":"pith:2003:WQ6UTEVIZSQDFMV6WUQPAKNA6X","short_pith_number":"pith:WQ6UTEVI","canonical_record":{"source":{"id":"hep-th/0312285","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2003-12-24T05:04:00Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"1b00152047324c61e3323ac170dd8c06d59eec21074b52edc2ad31f90d0a34f5","abstract_canon_sha256":"c92bf046e70478e50d4ee53acb0fa63efa1fc2714e39c9f13597cadcf8b8c159"},"schema_version":"1.0"},"canonical_sha256":"b43d4992a8cca032b2beb520f029a0f5e4bbc4d78347a6a43c39f00e07238d23","source":{"kind":"arxiv","id":"hep-th/0312285","version":2},"source_aliases":[{"alias_kind":"arxiv","alias_value":"hep-th/0312285","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0312285v2","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0312285","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"pith_short_12","alias_value":"WQ6UTEVIZSQD","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"pith_short_16","alias_value":"WQ6UTEVIZSQDFMV6","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"pith_short_8","alias_value":"WQ6UTEVI","created_at":"2026-07-04T16:41:30Z"}],"events":[{"event_type":"record_created","subject_pith_number":"pith:2003:WQ6UTEVIZSQDFMV6WUQPAKNA6X","target":"record","payload":{"canonical_record":{"source":{"id":"hep-th/0312285","kind":"arxiv","version":2},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2003-12-24T05:04:00Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"1b00152047324c61e3323ac170dd8c06d59eec21074b52edc2ad31f90d0a34f5","abstract_canon_sha256":"c92bf046e70478e50d4ee53acb0fa63efa1fc2714e39c9f13597cadcf8b8c159"},"schema_version":"1.0"},"canonical_sha256":"b43d4992a8cca032b2beb520f029a0f5e4bbc4d78347a6a43c39f00e07238d23","receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:41:30.940082Z","signature_b64":"Wcwigfi9sO0ZB4lT+yyr/WLLIWf8HQ+R+HNXneKnJZ2Sw4BABWMTeMZgA8PnKMkdPDV3YOmvRJZcLQaFnX/LBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b43d4992a8cca032b2beb520f029a0f5e4bbc4d78347a6a43c39f00e07238d23","last_reissued_at":"2026-07-04T16:41:30.939709Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:41:30.939709Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"source_kind":"arxiv","source_id":"hep-th/0312285","source_version":2,"attestation_state":"computed"},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:41:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"eqvJfwJKr/rejnGTe5sS2odgV2qsxJzdVjrBoBmumkPRHPu1v4AJtg8DmPe7K7ictEH/p+nUQ4NOVALT779HBg==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T12:39:31.125763Z"},"content_sha256":"573d91098532f0e34e5456408fdbbbf6de20c178273c9d870b19e77d12872d0a","schema_version":"1.0","event_id":"sha256:573d91098532f0e34e5456408fdbbbf6de20c178273c9d870b19e77d12872d0a"},{"event_type":"graph_snapshot","subject_pith_number":"pith:2003:WQ6UTEVIZSQDFMV6WUQPAKNA6X","target":"graph","payload":{"graph_snapshot":{"paper":{"title":"Nuttier (A)dS Black Holes in Higher Dimensions","license":"","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Cristian Stelea, Robert Mann","submitted_at":"2003-12-24T05:04:00Z","abstract_excerpt":"We construct new solutions of the vacuum Einstein field equations with cosmological constant. These solutions describe spacetimes with non-trivial topology that are asymptotically dS, AdS or flat. For a negative cosmological constant these solutions are NUT charged generalizations of the topological black hole solutions in higher dimensions. We also point out the existence of such NUT charged spacetimes in odd dimensions and we explicitly construct such spaces in 5 and 7 dimensions. The existence of such spacetimes with non-trivial topology is closely related to the existence of the cosmologic"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0312285","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/0312285/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"},"verdict_id":null},"signer":{"signer_id":"pith.science","signer_type":"pith_registry","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"created_at":"2026-07-04T16:41:30Z","supersedes":[],"prev_event":null,"signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"ASk7TNVWdx39QwuRE1Atn1dLHLYR8etiZ/XZe4L65x+w8NUuGNTrInziq44D0Sh99A6+0BS+z3bceKJDvQevCw==","signed_message":"open_graph_event_sha256_bytes","signed_at":"2026-08-04T12:39:31.126723Z"},"content_sha256":"129c0c12c48f31188d220e4fd9e2bb506fd049ba91758a29502696cb849ae911","schema_version":"1.0","event_id":"sha256:129c0c12c48f31188d220e4fd9e2bb506fd049ba91758a29502696cb849ae911"}],"timestamp_proofs":[],"mirror_hints":[{"mirror_type":"https","name":"Pith Resolver","base_url":"https://pith.science","bundle_url":"https://pith.science/pith/WQ6UTEVIZSQDFMV6WUQPAKNA6X/bundle.json","state_url":"https://pith.science/pith/WQ6UTEVIZSQDFMV6WUQPAKNA6X/state.json","well_known_bundle_url":"https://pith.science/.well-known/pith/WQ6UTEVIZSQDFMV6WUQPAKNA6X/bundle.json","status":"primary"}],"public_keys":[{"key_id":"pith-v1-2026-05","algorithm":"ed25519","format":"raw","public_key_b64":"stVStoiQhXFxp4s2pdzPNoqVNBMojDU/fJ2db5S3CbM=","public_key_hex":"b2d552b68890857171a78b36a5dccf368a953413288c353f7c9d9d6f94b709b3","fingerprint_sha256_b32_first128bits":"RVFV5Z2OI2J3ZUO7ERDEBCYNKS","fingerprint_sha256_hex":"8d4b5ee74e4693bcd1df2446408b0d54","rotates_at":null,"url":"https://pith.science/pith-signing-key.json","notes":"Pith uses this Ed25519 key to sign canonical record SHA-256 digests. Verify with: ed25519_verify(public_key, message=canonical_sha256_bytes, signature=base64decode(signature_b64))."}],"merge_version":"pith-open-graph-merge-v1","built_at":"2026-08-04T12:39:31Z","links":{"resolver":"https://pith.science/pith/WQ6UTEVIZSQDFMV6WUQPAKNA6X","bundle":"https://pith.science/pith/WQ6UTEVIZSQDFMV6WUQPAKNA6X/bundle.json","state":"https://pith.science/pith/WQ6UTEVIZSQDFMV6WUQPAKNA6X/state.json","well_known_bundle":"https://pith.science/.well-known/pith/WQ6UTEVIZSQDFMV6WUQPAKNA6X/bundle.json"},"state":{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2003:WQ6UTEVIZSQDFMV6WUQPAKNA6X","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"c92bf046e70478e50d4ee53acb0fa63efa1fc2714e39c9f13597cadcf8b8c159","cross_cats_sorted":["gr-qc"],"license":"","primary_cat":"hep-th","submitted_at":"2003-12-24T05:04:00Z","title_canon_sha256":"1b00152047324c61e3323ac170dd8c06d59eec21074b52edc2ad31f90d0a34f5"},"schema_version":"1.0","source":{"id":"hep-th/0312285","kind":"arxiv","version":2}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"hep-th/0312285","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0312285v2","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0312285","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"pith_short_12","alias_value":"WQ6UTEVIZSQD","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"pith_short_16","alias_value":"WQ6UTEVIZSQDFMV6","created_at":"2026-07-04T16:41:30Z"},{"alias_kind":"pith_short_8","alias_value":"WQ6UTEVI","created_at":"2026-07-04T16:41:30Z"}],"graph_snapshots":[{"event_id":"sha256:129c0c12c48f31188d220e4fd9e2bb506fd049ba91758a29502696cb849ae911","target":"graph","created_at":"2026-07-04T16:41:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"integrity":{"available":true,"clean":true,"detectors_run":[],"endpoint":"/pith/hep-th/0312285/integrity.json","findings":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938","summary":{"advisory":0,"by_detector":{},"critical":0,"informational":0}},"paper":{"abstract_excerpt":"We construct new solutions of the vacuum Einstein field equations with cosmological constant. These solutions describe spacetimes with non-trivial topology that are asymptotically dS, AdS or flat. For a negative cosmological constant these solutions are NUT charged generalizations of the topological black hole solutions in higher dimensions. We also point out the existence of such NUT charged spacetimes in odd dimensions and we explicitly construct such spaces in 5 and 7 dimensions. The existence of such spacetimes with non-trivial topology is closely related to the existence of the cosmologic","authors_text":"Cristian Stelea, Robert Mann","cross_cats":["gr-qc"],"headline":"","license":"","primary_cat":"hep-th","submitted_at":"2003-12-24T05:04:00Z","title":"Nuttier (A)dS Black Holes in Higher Dimensions"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0312285","kind":"arxiv","version":2},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:573d91098532f0e34e5456408fdbbbf6de20c178273c9d870b19e77d12872d0a","target":"record","created_at":"2026-07-04T16:41:30Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"c92bf046e70478e50d4ee53acb0fa63efa1fc2714e39c9f13597cadcf8b8c159","cross_cats_sorted":["gr-qc"],"license":"","primary_cat":"hep-th","submitted_at":"2003-12-24T05:04:00Z","title_canon_sha256":"1b00152047324c61e3323ac170dd8c06d59eec21074b52edc2ad31f90d0a34f5"},"schema_version":"1.0","source":{"id":"hep-th/0312285","kind":"arxiv","version":2}},"canonical_sha256":"b43d4992a8cca032b2beb520f029a0f5e4bbc4d78347a6a43c39f00e07238d23","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"b43d4992a8cca032b2beb520f029a0f5e4bbc4d78347a6a43c39f00e07238d23","first_computed_at":"2026-07-04T16:41:30.939709Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-07-04T16:41:30.939709Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"Wcwigfi9sO0ZB4lT+yyr/WLLIWf8HQ+R+HNXneKnJZ2Sw4BABWMTeMZgA8PnKMkdPDV3YOmvRJZcLQaFnX/LBA==","signature_status":"signed_v1","signed_at":"2026-07-04T16:41:30.940082Z","signed_message":"canonical_sha256_bytes"},"source_id":"hep-th/0312285","source_kind":"arxiv","source_version":2}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:573d91098532f0e34e5456408fdbbbf6de20c178273c9d870b19e77d12872d0a","sha256:129c0c12c48f31188d220e4fd9e2bb506fd049ba91758a29502696cb849ae911"],"state_sha256":"b4cd2809cd20a84b58e25994b97f6cd211614156d5b45f67051c32f23ed20d35"},"bundle_signature":{"signature_status":"signed_v1","algorithm":"ed25519","key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signature_b64":"Q02k+VR8Yo/jwKJT9SsuT7rSEwFtU3pFexQPSY+Z6THDKEtfx2ksqVR+E0nukWUIdKd7pc9HLe5HrQMaVcD4AA==","signed_message":"bundle_sha256_bytes","signed_at":"2026-08-04T12:39:31.132425Z","bundle_sha256":"0da6d4e18cdce115a1bcb4d9018a43a791452099f63489447de11bfa0ecc850f"}}