{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:3EDOHI33XAVI7XWJQ3UHFRM7N2","short_pith_number":"pith:3EDOHI33","schema_version":"1.0","canonical_sha256":"d906e3a37bb82a8fdec986e872c59f6eb4cff98833ae8c6c52ae866e6931f149","source":{"kind":"arxiv","id":"2510.11794","version":2},"attestation_state":"computed","paper":{"title":"4D de Sitter from 6D gauged supergravity with Green-Schwarz counterterm","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Ergin Sezgin, Xu Guo, Yi Pang","submitted_at":"2025-10-13T18:00:10Z","abstract_excerpt":"Taking into account the Green-Schwarz anomaly counterterm in R-symmetry gauged $N=(1,0)$ supergravity in six dimensions, and the associated modification in the Maxwell kinetic term and potential, the theory admits half-supersymmetric Mink$_4\\times S^2$ and non-supersymmetric dS$_4 \\times S^2$ solutions with or without a monopole on $S^2$. The monopole charge and the anomaly coefficients play key roles in the vacuum structure and a diagonal gauging in which an admixture of an external $U(1)$ with the R-symmetry $U(1)_R$ is needed for the de Sitter solutions to exist. We determine the full Kaluz"},"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":"2510.11794","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2025-10-13T18:00:10Z","cross_cats_sorted":[],"title_canon_sha256":"a4f1cac383f0e2ab04c268b7181d361627d663cf44066a3891bcda6cd5c5bc96","abstract_canon_sha256":"04b0692b0418d554cf15c70b9ddccdbb8e7f5be67b7dd8c6309a1d80447a6cb0"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-07T02:19:41.374927Z","signature_b64":"kbrbQzCULRrKAMWpbdBSxmn+jgb/qihcoQ2JtZ9QdF2cnOkMHnyH39zrC4VAe2JWcLOdLaKkgh5XdrFezqksDQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"d906e3a37bb82a8fdec986e872c59f6eb4cff98833ae8c6c52ae866e6931f149","last_reissued_at":"2026-07-07T02:19:41.374215Z","signature_status":"signed_v1","first_computed_at":"2026-07-07T02:19:41.374215Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"4D de Sitter from 6D gauged supergravity with Green-Schwarz counterterm","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Ergin Sezgin, Xu Guo, Yi Pang","submitted_at":"2025-10-13T18:00:10Z","abstract_excerpt":"Taking into account the Green-Schwarz anomaly counterterm in R-symmetry gauged $N=(1,0)$ supergravity in six dimensions, and the associated modification in the Maxwell kinetic term and potential, the theory admits half-supersymmetric Mink$_4\\times S^2$ and non-supersymmetric dS$_4 \\times S^2$ solutions with or without a monopole on $S^2$. The monopole charge and the anomaly coefficients play key roles in the vacuum structure and a diagonal gauging in which an admixture of an external $U(1)$ with the R-symmetry $U(1)_R$ is needed for the de Sitter solutions to exist. We determine the full Kaluz"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2510.11794","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/2510.11794/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":"2510.11794","created_at":"2026-07-07T02:19:41.374311+00:00"},{"alias_kind":"arxiv_version","alias_value":"2510.11794v2","created_at":"2026-07-07T02:19:41.374311+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2510.11794","created_at":"2026-07-07T02:19:41.374311+00:00"},{"alias_kind":"pith_short_12","alias_value":"3EDOHI33XAVI","created_at":"2026-07-07T02:19:41.374311+00:00"},{"alias_kind":"pith_short_16","alias_value":"3EDOHI33XAVI7XWJ","created_at":"2026-07-07T02:19:41.374311+00:00"},{"alias_kind":"pith_short_8","alias_value":"3EDOHI33","created_at":"2026-07-07T02:19:41.374311+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2603.25797","citing_title":"Dark energy from string theory: an introductory review","ref_index":117,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2","json":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2.json","graph_json":"https://pith.science/api/pith-number/3EDOHI33XAVI7XWJQ3UHFRM7N2/graph.json","events_json":"https://pith.science/api/pith-number/3EDOHI33XAVI7XWJQ3UHFRM7N2/events.json","paper":"https://pith.science/paper/3EDOHI33"},"agent_actions":{"view_html":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2","download_json":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2.json","view_paper":"https://pith.science/paper/3EDOHI33","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2510.11794&json=true","fetch_graph":"https://pith.science/api/pith-number/3EDOHI33XAVI7XWJQ3UHFRM7N2/graph.json","fetch_events":"https://pith.science/api/pith-number/3EDOHI33XAVI7XWJQ3UHFRM7N2/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2/action/timestamp_anchor","attest_storage":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2/action/storage_attestation","attest_author":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2/action/author_attestation","sign_citation":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2/action/citation_signature","submit_replication":"https://pith.science/pith/3EDOHI33XAVI7XWJQ3UHFRM7N2/action/replication_record"}},"created_at":"2026-07-07T02:19:41.374311+00:00","updated_at":"2026-07-07T02:19:41.374311+00:00"}