{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2004:623ZILF4LR62BK5JOJDYDN3VYK","short_pith_number":"pith:623ZILF4","schema_version":"1.0","canonical_sha256":"f6b7942cbc5c7da0aba9724781b775c283374b9e1dc6602263e4ba75d6e0de7f","source":{"kind":"arxiv","id":"hep-th/0412183","version":1},"attestation_state":"computed","paper":{"title":"Non-extremal instantons and wormholes in string theory","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"A. Collinucci, D. Roest, E. Bergshoeff, S. Vandoren, U. Gran","submitted_at":"2004-12-16T17:03:12Z","abstract_excerpt":"We construct the most general non-extremal spherically symmetric instanton solution of a gravity-dilaton-axion system with $SL(2,R)$ symmetry, for arbitrary euclidean spacetime dimension $D\\geq 3$. A subclass of these solutions describe completely regular wormhole geometries, whose size is determined by an invariant combination of the $SL(2,R)$ charges.\n  Our results can be applied to four-dimensional effective actions of type II strings compactified on a Calabi-Yau manifold, and in particular to the universal hypermultiplet coupled to gravity. We show that these models contain regular wormhol"},"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":"hep-th/0412183","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"hep-th","submitted_at":"2004-12-16T17:03:12Z","cross_cats_sorted":[],"title_canon_sha256":"9dfc79a4ed1c0812acb7079e4e48fbdcb038d1383195b63def63ec4bb853f7fb","abstract_canon_sha256":"28625d20fa6fce86576d8dca6adff4d66d85ebda6f12cd7960ff494f6f4fe75b"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T16:49:07.928819Z","signature_b64":"/8Uw/1TQFlzUN+uLh1UmSVlnHi8pqAOCRld/7Q16qH0LLzf6AhcrDkHmwaXo0MvBok2fpAKBWjajCe3utU35Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"f6b7942cbc5c7da0aba9724781b775c283374b9e1dc6602263e4ba75d6e0de7f","last_reissued_at":"2026-07-04T16:49:07.928470Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T16:49:07.928470Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-extremal instantons and wormholes in string theory","license":"","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"A. Collinucci, D. Roest, E. Bergshoeff, S. Vandoren, U. Gran","submitted_at":"2004-12-16T17:03:12Z","abstract_excerpt":"We construct the most general non-extremal spherically symmetric instanton solution of a gravity-dilaton-axion system with $SL(2,R)$ symmetry, for arbitrary euclidean spacetime dimension $D\\geq 3$. A subclass of these solutions describe completely regular wormhole geometries, whose size is determined by an invariant combination of the $SL(2,R)$ charges.\n  Our results can be applied to four-dimensional effective actions of type II strings compactified on a Calabi-Yau manifold, and in particular to the universal hypermultiplet coupled to gravity. We show that these models contain regular wormhol"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"hep-th/0412183","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/hep-th/0412183/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":"hep-th/0412183","created_at":"2026-07-04T16:49:07.928531+00:00"},{"alias_kind":"arxiv_version","alias_value":"hep-th/0412183v1","created_at":"2026-07-04T16:49:07.928531+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.hep-th/0412183","created_at":"2026-07-04T16:49:07.928531+00:00"},{"alias_kind":"pith_short_12","alias_value":"623ZILF4LR62","created_at":"2026-07-04T16:49:07.928531+00:00"},{"alias_kind":"pith_short_16","alias_value":"623ZILF4LR62BK5J","created_at":"2026-07-04T16:49:07.928531+00:00"},{"alias_kind":"pith_short_8","alias_value":"623ZILF4","created_at":"2026-07-04T16:49:07.928531+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":7,"internal_anchor_count":5,"sample":[{"citing_arxiv_id":"2606.26004","citing_title":"Non-invertible symmetries in the axiverse, and the imaginary wormholes","ref_index":122,"is_internal_anchor":true},{"citing_arxiv_id":"2607.01221","citing_title":"Type IIB Axion--Dilaton Wormholes and the BPS Limit Hessian","ref_index":20,"is_internal_anchor":true},{"citing_arxiv_id":"2605.16168","citing_title":"Supergravity flows, wormholes and their pseudo-Hermitian holographic duals","ref_index":36,"is_internal_anchor":true},{"citing_arxiv_id":"2605.22912","citing_title":"Sharpening the Supersymmetric Axion Weak Gravity Conjecture","ref_index":51,"is_internal_anchor":true},{"citing_arxiv_id":"2605.16168","citing_title":"Supergravity flows, wormholes and their pseudo-Hermitian holographic duals","ref_index":35,"is_internal_anchor":true},{"citing_arxiv_id":"2605.05336","citing_title":"Wormholes and the imaginary distance bound","ref_index":21,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05305","citing_title":"Positivity of the gravitational path integral implies the axionic weak gravity conjecture","ref_index":32,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK","json":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK.json","graph_json":"https://pith.science/api/pith-number/623ZILF4LR62BK5JOJDYDN3VYK/graph.json","events_json":"https://pith.science/api/pith-number/623ZILF4LR62BK5JOJDYDN3VYK/events.json","paper":"https://pith.science/paper/623ZILF4"},"agent_actions":{"view_html":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK","download_json":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK.json","view_paper":"https://pith.science/paper/623ZILF4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=hep-th/0412183&json=true","fetch_graph":"https://pith.science/api/pith-number/623ZILF4LR62BK5JOJDYDN3VYK/graph.json","fetch_events":"https://pith.science/api/pith-number/623ZILF4LR62BK5JOJDYDN3VYK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK/action/storage_attestation","attest_author":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK/action/author_attestation","sign_citation":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK/action/citation_signature","submit_replication":"https://pith.science/pith/623ZILF4LR62BK5JOJDYDN3VYK/action/replication_record"}},"created_at":"2026-07-04T16:49:07.928531+00:00","updated_at":"2026-07-04T16:49:07.928531+00:00"}