{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:CB3ZIAWSEVD6EFT66Q2FYUJ3EW","short_pith_number":"pith:CB3ZIAWS","schema_version":"1.0","canonical_sha256":"10779402d22547e2167ef4345c513b259fa86e0a134b70d8649fc5dfb921ebd6","source":{"kind":"arxiv","id":"2412.15102","version":1},"attestation_state":"computed","paper":{"title":"Circle compactifications of Minkowski$_D$ solutions, flux vacua and solitonic branes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Niall T. Macpherson, Paul Merrikin, Ricardo Stuardo","submitted_at":"2024-12-19T17:48:45Z","abstract_excerpt":"G-structure techniques are used to construct broad classes of circle compactifications of Mink$_{D+1}$ solutions to Mink$_{D}$ embedded into type II supergravity for $D=1,...5$. Under a certain assumptions we show that the conditions that imply supersymmetry for Mink$_{D+1}$ imply those of the Mink$_{D}$ solution, but that Bianchi identities of the fluxes must be modified. This realises an off shell solution generating technique for supersymmetric solutions or a \"supersymmetry generating\" technique. Along the way it is necessary for us to derive G structure conditions for general ${\\cal N}=(1,"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"2412.15102","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-12-19T17:48:45Z","cross_cats_sorted":[],"title_canon_sha256":"c45ab63b545b2e4c4f6adb0acd98ce64cf3deeb16589d5be89cfbc9ab727fa53","abstract_canon_sha256":"beb69cae15ac89ed87971307b8faa55a82d281bb4084c94537be882f9900233d"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:51:57.918951Z","signature_b64":"x8k0Nl5jO0lpu22f1KhcL+KM4qlmusqj7bXhzAyclxlaMf7J5x1XVQclxEqID+tBD/ZLpV+DcQcxIveUdxfPAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"10779402d22547e2167ef4345c513b259fa86e0a134b70d8649fc5dfb921ebd6","last_reissued_at":"2026-07-05T09:51:57.918485Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:51:57.918485Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Circle compactifications of Minkowski$_D$ solutions, flux vacua and solitonic branes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Niall T. Macpherson, Paul Merrikin, Ricardo Stuardo","submitted_at":"2024-12-19T17:48:45Z","abstract_excerpt":"G-structure techniques are used to construct broad classes of circle compactifications of Mink$_{D+1}$ solutions to Mink$_{D}$ embedded into type II supergravity for $D=1,...5$. Under a certain assumptions we show that the conditions that imply supersymmetry for Mink$_{D+1}$ imply those of the Mink$_{D}$ solution, but that Bianchi identities of the fluxes must be modified. This realises an off shell solution generating technique for supersymmetric solutions or a \"supersymmetry generating\" technique. Along the way it is necessary for us to derive G structure conditions for general ${\\cal N}=(1,"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.15102","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/2412.15102/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":"2412.15102","created_at":"2026-07-05T09:51:57.918547+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.15102v1","created_at":"2026-07-05T09:51:57.918547+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.15102","created_at":"2026-07-05T09:51:57.918547+00:00"},{"alias_kind":"pith_short_12","alias_value":"CB3ZIAWSEVD6","created_at":"2026-07-05T09:51:57.918547+00:00"},{"alias_kind":"pith_short_16","alias_value":"CB3ZIAWSEVD6EFT6","created_at":"2026-07-05T09:51:57.918547+00:00"},{"alias_kind":"pith_short_8","alias_value":"CB3ZIAWS","created_at":"2026-07-05T09:51:57.918547+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.04586","citing_title":"Bound states and deconfinement from Romans supergravity with magnetic flux","ref_index":118,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18942","citing_title":"Covariant unification of holographic c-functions","ref_index":76,"is_internal_anchor":false},{"citing_arxiv_id":"2511.18128","citing_title":"Supersymmetric AdS Solitons, Coulomb Branch Flows and Twisted Compactifications","ref_index":29,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW","json":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW.json","graph_json":"https://pith.science/api/pith-number/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/graph.json","events_json":"https://pith.science/api/pith-number/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/events.json","paper":"https://pith.science/paper/CB3ZIAWS"},"agent_actions":{"view_html":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW","download_json":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW.json","view_paper":"https://pith.science/paper/CB3ZIAWS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.15102&json=true","fetch_graph":"https://pith.science/api/pith-number/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/graph.json","fetch_events":"https://pith.science/api/pith-number/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/action/storage_attestation","attest_author":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/action/author_attestation","sign_citation":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/action/citation_signature","submit_replication":"https://pith.science/pith/CB3ZIAWSEVD6EFT66Q2FYUJ3EW/action/replication_record"}},"created_at":"2026-07-05T09:51:57.918547+00:00","updated_at":"2026-07-05T09:51:57.918547+00:00"}