{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:1998:I4OYW45GGOE6CDYGIXKH74ANWZ","short_pith_number":"pith:I4OYW45G","schema_version":"1.0","canonical_sha256":"471d8b73a63389e10f0645d47ff00db66662e98edc05146d5063540ab38710cd","source":{"kind":"arxiv","id":"hep-th/9811107","version":1},"attestation_state":"computed","paper":{"title":"Decoupling Limit, Lens Spaces and Taub-NUT: D=4 Black Hole Microscopics from D=5 Black Holes","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"C.N. Pope, H. Lu, M. Cvetic","submitted_at":"1998-11-12T23:29:38Z","abstract_excerpt":"We study the space-times of non-extremal intersecting p-brane configurations in M-theory, where one of the components in the intersection is a ``NUT,'' i.e. a configuration of the Taub-NUT type. Such a Taub-NUT configuration corresponds, upon compactification to D=4, to a Gross-Perry-Sorkin (GPS) monopole. We show that in the decoupling limit of the CFT/AdS correspondence, the 4-dimensional transverse space of the NUT configuration in D=5 is foliated by surfaces that are cyclic lens spaces S^3/Z_N, where N is the quantised monopole charge. By contrast, in D=4 the 3-dimensional transverse space"},"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/9811107","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"1998-11-12T23:29:38Z","cross_cats_sorted":[],"title_canon_sha256":"2a917c6cfa7a6f43fb2d3b7410f85dcdd5694d255b241ae371c596056bf12d3e","abstract_canon_sha256":"57bd26fd65393ccfdb422eb3118d8ab9e1325ce9f37a3be8a96033669b0f2fdf"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T15:49:59.724007Z","signature_b64":"CdRR/IOgGXI4uFmM+6hSojP2GyfI0Nt7XKj6xc0jmQrEjfxJLhQgWf6DgnaeS3xrMjplHSL47Eu9Z4hLhxPlBg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"471d8b73a63389e10f0645d47ff00db66662e98edc05146d5063540ab38710cd","last_reissued_at":"2026-07-04T15:49:59.723585Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T15:49:59.723585Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Decoupling Limit, Lens Spaces and Taub-NUT: D=4 Black Hole Microscopics from D=5 Black Holes","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"C.N. Pope, H. Lu, M. Cvetic","submitted_at":"1998-11-12T23:29:38Z","abstract_excerpt":"We study the space-times of non-extremal intersecting p-brane configurations in M-theory, where one of the components in the intersection is a ``NUT,'' i.e. a configuration of the Taub-NUT type. Such a Taub-NUT configuration corresponds, upon compactification to D=4, to a Gross-Perry-Sorkin (GPS) monopole. We show that in the decoupling limit of the CFT/AdS correspondence, the 4-dimensional transverse space of the NUT configuration in D=5 is foliated by surfaces that are cyclic lens spaces S^3/Z_N, where N is the quantised monopole charge. By contrast, in D=4 the 3-dimensional transverse space"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/9811107","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":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/hep-th/9811107/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/9811107","created_at":"2026-07-04T15:49:59.723653+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/9811107v1","created_at":"2026-07-04T15:49:59.723653+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/9811107","created_at":"2026-07-04T15:49:59.723653+00:00"},{"alias_kind":"pith_short_12","alias_value":"I4OYW45GGOE6","created_at":"2026-07-04T15:49:59.723653+00:00"},{"alias_kind":"pith_short_16","alias_value":"I4OYW45GGOE6CDYG","created_at":"2026-07-04T15:49:59.723653+00:00"},{"alias_kind":"pith_short_8","alias_value":"I4OYW45G","created_at":"2026-07-04T15:49:59.723653+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2411.11096","citing_title":"An extremal black hole with a unique ground state","ref_index":34,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ","json":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ.json","graph_json":"https://pith.science/api/pith-number/I4OYW45GGOE6CDYGIXKH74ANWZ/graph.json","events_json":"https://pith.science/api/pith-number/I4OYW45GGOE6CDYGIXKH74ANWZ/events.json","paper":"https://pith.science/paper/I4OYW45G"},"agent_actions":{"view_html":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ","download_json":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ.json","view_paper":"https://pith.science/paper/I4OYW45G","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/9811107&json=true","fetch_graph":"https://pith.science/api/pith-number/I4OYW45GGOE6CDYGIXKH74ANWZ/graph.json","fetch_events":"https://pith.science/api/pith-number/I4OYW45GGOE6CDYGIXKH74ANWZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ/action/storage_attestation","attest_author":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ/action/author_attestation","sign_citation":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ/action/citation_signature","submit_replication":"https://pith.science/pith/I4OYW45GGOE6CDYGIXKH74ANWZ/action/replication_record"}},"created_at":"2026-07-04T15:49:59.723653+00:00","updated_at":"2026-07-04T15:49:59.723653+00:00"}