{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:432MECFGDU5HWUFG4YD2PMZOWW","short_pith_number":"pith:432MECFG","schema_version":"1.0","canonical_sha256":"e6f4c208a61d3a7b50a6e607a7b32eb5a5642e797788ba1ed2d8b49d168deaf3","source":{"kind":"arxiv","id":"2309.04880","version":2},"attestation_state":"computed","paper":{"title":"Holographic CFTs on $AdS_d\\times S^n$ and conformal defects","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Ahmad Ghodsi, Elias Kiritsis, Francesco Nitti","submitted_at":"2023-09-09T21:53:29Z","abstract_excerpt":"We consider ($d+n+1$)-dimensional solutions of Einstein gravity with constant negative curvature. Regular solutions of this type are expected to be dual to the ground states of ($d+n$)-dimensional holographic CFTs on $AdS_d\\times S^n$. Their only dimensionless parameter is the ratio of radii of curvatures of $AdS_d$ and $S^n$. The same solutions may also be dual to $(d-1)$-dimensional conformal defects in holographic QFT$_{d+n}$. We solve the gravity equations with an associated conifold ansatz, and we classify all solutions both singular and regular by a combination of analytical and numerica"},"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":"2309.04880","kind":"arxiv","version":2},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2023-09-09T21:53:29Z","cross_cats_sorted":[],"title_canon_sha256":"a23f3463174aa9acb8b6fa07b28416fc3161bf85d2835c21c4d724077d946f47","abstract_canon_sha256":"49c06fe5d43f2db66b0d41e5bf220c10151d93357524238c5c86884b8b52a1a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T07:15:37.438090Z","signature_b64":"nBzQ+/2jqRBTg4pSPJt+gSg1iY1m/CetezUMyLbd/LanhNwadtwQmjGIxzY1XaRqoSPExTFChfBMxnzaYODbCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e6f4c208a61d3a7b50a6e607a7b32eb5a5642e797788ba1ed2d8b49d168deaf3","last_reissued_at":"2026-07-05T07:15:37.437608Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T07:15:37.437608Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holographic CFTs on $AdS_d\\times S^n$ and conformal defects","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Ahmad Ghodsi, Elias Kiritsis, Francesco Nitti","submitted_at":"2023-09-09T21:53:29Z","abstract_excerpt":"We consider ($d+n+1$)-dimensional solutions of Einstein gravity with constant negative curvature. Regular solutions of this type are expected to be dual to the ground states of ($d+n$)-dimensional holographic CFTs on $AdS_d\\times S^n$. Their only dimensionless parameter is the ratio of radii of curvatures of $AdS_d$ and $S^n$. The same solutions may also be dual to $(d-1)$-dimensional conformal defects in holographic QFT$_{d+n}$. We solve the gravity equations with an associated conifold ansatz, and we classify all solutions both singular and regular by a combination of analytical and numerica"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.04880","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/2309.04880/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":"2309.04880","created_at":"2026-07-05T07:15:37.437660+00:00"},{"alias_kind":"arxiv_version","alias_value":"2309.04880v2","created_at":"2026-07-05T07:15:37.437660+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2309.04880","created_at":"2026-07-05T07:15:37.437660+00:00"},{"alias_kind":"pith_short_12","alias_value":"432MECFGDU5H","created_at":"2026-07-05T07:15:37.437660+00:00"},{"alias_kind":"pith_short_16","alias_value":"432MECFGDU5HWUFG","created_at":"2026-07-05T07:15:37.437660+00:00"},{"alias_kind":"pith_short_8","alias_value":"432MECFG","created_at":"2026-07-05T07:15:37.437660+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.03106","citing_title":"Holographic reconstruction for defect CFTs from $\\mathrm{AdS}_p \\times S^q$ spacetimes","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW","json":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW.json","graph_json":"https://pith.science/api/pith-number/432MECFGDU5HWUFG4YD2PMZOWW/graph.json","events_json":"https://pith.science/api/pith-number/432MECFGDU5HWUFG4YD2PMZOWW/events.json","paper":"https://pith.science/paper/432MECFG"},"agent_actions":{"view_html":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW","download_json":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW.json","view_paper":"https://pith.science/paper/432MECFG","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2309.04880&json=true","fetch_graph":"https://pith.science/api/pith-number/432MECFGDU5HWUFG4YD2PMZOWW/graph.json","fetch_events":"https://pith.science/api/pith-number/432MECFGDU5HWUFG4YD2PMZOWW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW/action/storage_attestation","attest_author":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW/action/author_attestation","sign_citation":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW/action/citation_signature","submit_replication":"https://pith.science/pith/432MECFGDU5HWUFG4YD2PMZOWW/action/replication_record"}},"created_at":"2026-07-05T07:15:37.437660+00:00","updated_at":"2026-07-05T07:15:37.437660+00:00"}