{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2019:R6W3KFHKUH4YMMFNMO2HJP73CH","short_pith_number":"pith:R6W3KFHK","schema_version":"1.0","canonical_sha256":"8fadb514eaa1f98630ad63b474bffb11cf2e3d910f0bb73dc59a36dcecd2ff81","source":{"kind":"arxiv","id":"1907.12764","version":2},"attestation_state":"computed","paper":{"title":"${\\mathcal{N}=(8,0)}$ AdS vacua of three-dimensional supergravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Camille Eloy, Henning Samtleben, Nihat Sadik Deger","submitted_at":"2019-07-30T07:31:10Z","abstract_excerpt":"We give a classification of fully supersymmetric chiral ${\\cal N}=(8,0)$ AdS$_3$ vacua in general three-dimensional half-maximal gauged supergravities coupled to matter. These theories exhibit a wealth of supersymmetric vacua with background isometries given by the supergroups OSp$(8|2,\\mathbb{R})$, F(4), SU$(4|1,1)$, and OSp$(4^*|4)$, respectively. We identify the associated embedding tensors and the structure of the associated gauge groups. We furthermore compute the mass spectra around these vacua. As an off-spin we include results for a number of ${\\cal N}=(7,0)$ vacua with supergroups OSp"},"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":"1907.12764","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2019-07-30T07:31:10Z","cross_cats_sorted":[],"title_canon_sha256":"3feac87f3f9388bb6b5e063378a0c4d41ccdee08ca51d4c1f77fd377741e3f65","abstract_canon_sha256":"b6fe928870d5ac2eadfe1f5ceb79d8d35638bf797901148dcd86f37cb0fdd602"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T00:14:20.432625Z","signature_b64":"KtWKQMHcAaAfQpHkw4Ua7/xesWRwPG9xpr4h01sX2dc3bQR1WKSO36ZcxRE4/T/xmBQpc46FM9wH2dHjawEhAg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"8fadb514eaa1f98630ad63b474bffb11cf2e3d910f0bb73dc59a36dcecd2ff81","last_reissued_at":"2026-07-05T00:14:20.432282Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T00:14:20.432282Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"${\\mathcal{N}=(8,0)}$ AdS vacua of three-dimensional supergravity","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Camille Eloy, Henning Samtleben, Nihat Sadik Deger","submitted_at":"2019-07-30T07:31:10Z","abstract_excerpt":"We give a classification of fully supersymmetric chiral ${\\cal N}=(8,0)$ AdS$_3$ vacua in general three-dimensional half-maximal gauged supergravities coupled to matter. These theories exhibit a wealth of supersymmetric vacua with background isometries given by the supergroups OSp$(8|2,\\mathbb{R})$, F(4), SU$(4|1,1)$, and OSp$(4^*|4)$, respectively. We identify the associated embedding tensors and the structure of the associated gauge groups. We furthermore compute the mass spectra around these vacua. As an off-spin we include results for a number of ${\\cal N}=(7,0)$ vacua with supergroups OSp"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1907.12764","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/1907.12764/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":"1907.12764","created_at":"2026-07-05T00:14:20.432344+00:00"},{"alias_kind":"arxiv_version","alias_value":"1907.12764v2","created_at":"2026-07-05T00:14:20.432344+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1907.12764","created_at":"2026-07-05T00:14:20.432344+00:00"},{"alias_kind":"pith_short_12","alias_value":"R6W3KFHKUH4Y","created_at":"2026-07-05T00:14:20.432344+00:00"},{"alias_kind":"pith_short_16","alias_value":"R6W3KFHKUH4YMMFN","created_at":"2026-07-05T00:14:20.432344+00:00"},{"alias_kind":"pith_short_8","alias_value":"R6W3KFHK","created_at":"2026-07-05T00:14:20.432344+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"1908.09851","citing_title":"AdS$_3$ solutions in Massive IIA with small $\\mathcal{N}=(4,0)$ supersymmetry","ref_index":40,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH","json":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH.json","graph_json":"https://pith.science/api/pith-number/R6W3KFHKUH4YMMFNMO2HJP73CH/graph.json","events_json":"https://pith.science/api/pith-number/R6W3KFHKUH4YMMFNMO2HJP73CH/events.json","paper":"https://pith.science/paper/R6W3KFHK"},"agent_actions":{"view_html":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH","download_json":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH.json","view_paper":"https://pith.science/paper/R6W3KFHK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1907.12764&json=true","fetch_graph":"https://pith.science/api/pith-number/R6W3KFHKUH4YMMFNMO2HJP73CH/graph.json","fetch_events":"https://pith.science/api/pith-number/R6W3KFHKUH4YMMFNMO2HJP73CH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH/action/storage_attestation","attest_author":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH/action/author_attestation","sign_citation":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH/action/citation_signature","submit_replication":"https://pith.science/pith/R6W3KFHKUH4YMMFNMO2HJP73CH/action/replication_record"}},"created_at":"2026-07-05T00:14:20.432344+00:00","updated_at":"2026-07-05T00:14:20.432344+00:00"}