{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:AGMOWVJJGNITW7NDC7ZX7PTJNN","short_pith_number":"pith:AGMOWVJJ","schema_version":"1.0","canonical_sha256":"0198eb552933513b7da317f37fbe696b43a445015d1cc4427b806df0a618b726","source":{"kind":"arxiv","id":"2212.01697","version":1},"attestation_state":"computed","paper":{"title":"Pure Supersymmetric AdS and the Swampland","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Cumrun Vafa, Martin Rocek, Miguel Montero","submitted_at":"2022-12-03T21:39:30Z","abstract_excerpt":"We point out that pure supergravity theories in $AdS$ with enough supersymmetry lead, upon taking the large radius limit, to flat space quantum gravities with a nonperturbatively exact global symmetry, and are therefore in the Swampland. The argument applies to any $AdS$ supergravity with gauged R-symmetry group, including truncations of most well known examples, such as $AdS_5$ without the $S^5$ or $AdS_4$ without the $S^7$. This demonstrates that extreme scale separation, at least with enough supersymmetry, is not realizable. Moreover pure $AdS$ theories are also in conflict with some other "},"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":"2212.01697","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-12-03T21:39:30Z","cross_cats_sorted":[],"title_canon_sha256":"a9fe360fbc80bb5e1d329d076e137029f99e01622f33a9d4226ff2537dbcd5b6","abstract_canon_sha256":"e669594f18aa082139cfe9872b95e22d711192d71bdfb851103dce361d5dd498"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:39:26.696699Z","signature_b64":"rZgwLFYjrE5CwysD4Vf69u8GBKlpUVA1DnD3QDluH2oWVWArfQ7y+u4VjNOawmKx/a9oJ+TcK/5PkqHy9eQrCg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"0198eb552933513b7da317f37fbe696b43a445015d1cc4427b806df0a618b726","last_reissued_at":"2026-07-05T05:39:26.696288Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:39:26.696288Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pure Supersymmetric AdS and the Swampland","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Cumrun Vafa, Martin Rocek, Miguel Montero","submitted_at":"2022-12-03T21:39:30Z","abstract_excerpt":"We point out that pure supergravity theories in $AdS$ with enough supersymmetry lead, upon taking the large radius limit, to flat space quantum gravities with a nonperturbatively exact global symmetry, and are therefore in the Swampland. The argument applies to any $AdS$ supergravity with gauged R-symmetry group, including truncations of most well known examples, such as $AdS_5$ without the $S^5$ or $AdS_4$ without the $S^7$. This demonstrates that extreme scale separation, at least with enough supersymmetry, is not realizable. Moreover pure $AdS$ theories are also in conflict with some other "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2212.01697","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/2212.01697/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":"2212.01697","created_at":"2026-07-05T05:39:26.696356+00:00"},{"alias_kind":"arxiv_version","alias_value":"2212.01697v1","created_at":"2026-07-05T05:39:26.696356+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2212.01697","created_at":"2026-07-05T05:39:26.696356+00:00"},{"alias_kind":"pith_short_12","alias_value":"AGMOWVJJGNIT","created_at":"2026-07-05T05:39:26.696356+00:00"},{"alias_kind":"pith_short_16","alias_value":"AGMOWVJJGNITW7ND","created_at":"2026-07-05T05:39:26.696356+00:00"},{"alias_kind":"pith_short_8","alias_value":"AGMOWVJJ","created_at":"2026-07-05T05:39:26.696356+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.30341","citing_title":"A note on the holographic consistency of DGKT-type vacua with $h^{2,1}=0$","ref_index":5,"is_internal_anchor":false},{"citing_arxiv_id":"2507.17802","citing_title":"Instabilities in scale-separated Casimir vacua","ref_index":107,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26755","citing_title":"Scale-separated vacua with extended supersymmetry","ref_index":11,"is_internal_anchor":false},{"citing_arxiv_id":"2605.07464","citing_title":"Broken and restored: a holographic constraint for AdS vacua with orbifolds","ref_index":15,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN","json":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN.json","graph_json":"https://pith.science/api/pith-number/AGMOWVJJGNITW7NDC7ZX7PTJNN/graph.json","events_json":"https://pith.science/api/pith-number/AGMOWVJJGNITW7NDC7ZX7PTJNN/events.json","paper":"https://pith.science/paper/AGMOWVJJ"},"agent_actions":{"view_html":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN","download_json":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN.json","view_paper":"https://pith.science/paper/AGMOWVJJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2212.01697&json=true","fetch_graph":"https://pith.science/api/pith-number/AGMOWVJJGNITW7NDC7ZX7PTJNN/graph.json","fetch_events":"https://pith.science/api/pith-number/AGMOWVJJGNITW7NDC7ZX7PTJNN/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN/action/timestamp_anchor","attest_storage":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN/action/storage_attestation","attest_author":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN/action/author_attestation","sign_citation":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN/action/citation_signature","submit_replication":"https://pith.science/pith/AGMOWVJJGNITW7NDC7ZX7PTJNN/action/replication_record"}},"created_at":"2026-07-05T05:39:26.696356+00:00","updated_at":"2026-07-05T05:39:26.696356+00:00"}