{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:TWYNZYDHB6LVO6L445KNN7NB53","short_pith_number":"pith:TWYNZYDH","schema_version":"1.0","canonical_sha256":"9db0dce0670f9757797ce754d6fda1eecb111eff0aa757be0fce8afa0d659d90","source":{"kind":"arxiv","id":"2309.16542","version":1},"attestation_state":"computed","paper":{"title":"Anisotropic scale-separated AdS$_4$ flux vacua","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"George Tringas","submitted_at":"2023-09-28T15:53:53Z","abstract_excerpt":"We present minimally supersymmetric AdS$_4$ flux vacua derived from massive type IIA compactified on $T^6/\\mathbb{Z}_3\\times \\mathbb{Z}_3$ orbifold, characterized by unconstrained fluxes with general scaling. We discover anisotropic scaling solutions where scale separation is realized in the supergravity limit and the subvolumes of the internal space become large and anisotropic for large values of unconstrained fluxes. Additionally, we identify regimes where subvolumes are either shrinking or remain constant while scale separation is either broken or realized. Then we employ a probe anti-D4-b"},"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":"2309.16542","kind":"arxiv","version":1},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2023-09-28T15:53:53Z","cross_cats_sorted":[],"title_canon_sha256":"69d16830657df29123073b0801964f463f75173afdde0534860e5885041b828e","abstract_canon_sha256":"4b61a7e76c9a3b8645e01414a71f12a9080363594da3ce23a1061f9f41cc42a2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:55:17.979735Z","signature_b64":"WUKH3ip+LDNxHubG6sUzVj+1t0V4fRzMG++wuCQiNuUpvwS9cYrXfgVRvNENujplBqFzR+a9Ry7PMOJ5uu2dAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9db0dce0670f9757797ce754d6fda1eecb111eff0aa757be0fce8afa0d659d90","last_reissued_at":"2026-07-05T06:55:17.979262Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:55:17.979262Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Anisotropic scale-separated AdS$_4$ flux vacua","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"George Tringas","submitted_at":"2023-09-28T15:53:53Z","abstract_excerpt":"We present minimally supersymmetric AdS$_4$ flux vacua derived from massive type IIA compactified on $T^6/\\mathbb{Z}_3\\times \\mathbb{Z}_3$ orbifold, characterized by unconstrained fluxes with general scaling. We discover anisotropic scaling solutions where scale separation is realized in the supergravity limit and the subvolumes of the internal space become large and anisotropic for large values of unconstrained fluxes. Additionally, we identify regimes where subvolumes are either shrinking or remain constant while scale separation is either broken or realized. Then we employ a probe anti-D4-b"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2309.16542","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/2309.16542/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":"2309.16542","created_at":"2026-07-05T06:55:17.979344+00:00"},{"alias_kind":"arxiv_version","alias_value":"2309.16542v1","created_at":"2026-07-05T06:55:17.979344+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2309.16542","created_at":"2026-07-05T06:55:17.979344+00:00"},{"alias_kind":"pith_short_12","alias_value":"TWYNZYDHB6LV","created_at":"2026-07-05T06:55:17.979344+00:00"},{"alias_kind":"pith_short_16","alias_value":"TWYNZYDHB6LVO6L4","created_at":"2026-07-05T06:55:17.979344+00:00"},{"alias_kind":"pith_short_8","alias_value":"TWYNZYDH","created_at":"2026-07-05T06:55:17.979344+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2507.17802","citing_title":"Instabilities in scale-separated Casimir vacua","ref_index":90,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53","json":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53.json","graph_json":"https://pith.science/api/pith-number/TWYNZYDHB6LVO6L445KNN7NB53/graph.json","events_json":"https://pith.science/api/pith-number/TWYNZYDHB6LVO6L445KNN7NB53/events.json","paper":"https://pith.science/paper/TWYNZYDH"},"agent_actions":{"view_html":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53","download_json":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53.json","view_paper":"https://pith.science/paper/TWYNZYDH","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2309.16542&json=true","fetch_graph":"https://pith.science/api/pith-number/TWYNZYDHB6LVO6L445KNN7NB53/graph.json","fetch_events":"https://pith.science/api/pith-number/TWYNZYDHB6LVO6L445KNN7NB53/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53/action/storage_attestation","attest_author":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53/action/author_attestation","sign_citation":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53/action/citation_signature","submit_replication":"https://pith.science/pith/TWYNZYDHB6LVO6L445KNN7NB53/action/replication_record"}},"created_at":"2026-07-05T06:55:17.979344+00:00","updated_at":"2026-07-05T06:55:17.979344+00:00"}