{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:4F6AOC26UKGSCN3MLNSMY2BV5S","short_pith_number":"pith:4F6AOC26","schema_version":"1.0","canonical_sha256":"e17c070b5ea28d21376c5b64cc6835eca5899d45251bcce9396a82ab32a5483d","source":{"kind":"arxiv","id":"2101.08875","version":2},"attestation_state":"computed","paper":{"title":"AdS Euclidean wormholes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Donald Marolf, Jorge E. Santos","submitted_at":"2021-01-21T22:37:02Z","abstract_excerpt":"We explore the construction and stability of asymptotically anti-de Sitter Euclidean wormholes in a variety of models. In simple ad hoc low-energy models, it is not hard to construct two-boundary Euclidean wormholes that dominate over disconnected solutions and which are stable (lacking negative modes) in the usual sense of Euclidean quantum gravity. Indeed, the structure of such solutions turns out to strongly resemble that of the Hawking-Page phase transition for AdS-Schwarzschild black holes, in that for boundary sources above some threshold we find both a `large' and a `small' branch of wo"},"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":"2101.08875","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2021-01-21T22:37:02Z","cross_cats_sorted":[],"title_canon_sha256":"838f49812d04bfd4aa36e4fcc8a6b2eed030af1b6d74d09cdad13ecf2b42d6c9","abstract_canon_sha256":"0dd776e61833f0354da090c2420629e199f4e87d802730960237f3520b10ffa8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:31:56.914652Z","signature_b64":"71pcGXBB377xaEfsH0FYfOPPPupBCqmI0PgvqNYcAuX8HXtHYFGBpjVqcY4FuGGwdRG4ddkw96/MwRIpDHdzAA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"e17c070b5ea28d21376c5b64cc6835eca5899d45251bcce9396a82ab32a5483d","last_reissued_at":"2026-07-05T03:31:56.914150Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:31:56.914150Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"AdS Euclidean wormholes","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Donald Marolf, Jorge E. Santos","submitted_at":"2021-01-21T22:37:02Z","abstract_excerpt":"We explore the construction and stability of asymptotically anti-de Sitter Euclidean wormholes in a variety of models. In simple ad hoc low-energy models, it is not hard to construct two-boundary Euclidean wormholes that dominate over disconnected solutions and which are stable (lacking negative modes) in the usual sense of Euclidean quantum gravity. Indeed, the structure of such solutions turns out to strongly resemble that of the Hawking-Page phase transition for AdS-Schwarzschild black holes, in that for boundary sources above some threshold we find both a `large' and a `small' branch of wo"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2101.08875","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/2101.08875/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":"2101.08875","created_at":"2026-07-05T03:31:56.914209+00:00"},{"alias_kind":"arxiv_version","alias_value":"2101.08875v2","created_at":"2026-07-05T03:31:56.914209+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2101.08875","created_at":"2026-07-05T03:31:56.914209+00:00"},{"alias_kind":"pith_short_12","alias_value":"4F6AOC26UKGS","created_at":"2026-07-05T03:31:56.914209+00:00"},{"alias_kind":"pith_short_16","alias_value":"4F6AOC26UKGSCN3M","created_at":"2026-07-05T03:31:56.914209+00:00"},{"alias_kind":"pith_short_8","alias_value":"4F6AOC26","created_at":"2026-07-05T03:31:56.914209+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":8,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.16168","citing_title":"Supergravity flows, wormholes and their pseudo-Hermitian holographic duals","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13777","citing_title":"Before the Bang: Wormholes at the Dawn of the Universe","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.16168","citing_title":"Supergravity flows, wormholes and their pseudo-Hermitian holographic duals","ref_index":41,"is_internal_anchor":false},{"citing_arxiv_id":"2601.10906","citing_title":"Menagerie of Euclidean constructions for 3D holographic cosmologies","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2602.23432","citing_title":"A Menagerie of Wormholes and Cosmologies in the Gravitational Path Integral","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13777","citing_title":"Before the Bang: Wormholes at the Dawn of the Universe","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.10548","citing_title":"Birth of Inflationary Universes via Wineglass Wormholes and their No-Boundary Relatives","ref_index":36,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05336","citing_title":"Wormholes and the imaginary distance bound","ref_index":42,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S","json":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S.json","graph_json":"https://pith.science/api/pith-number/4F6AOC26UKGSCN3MLNSMY2BV5S/graph.json","events_json":"https://pith.science/api/pith-number/4F6AOC26UKGSCN3MLNSMY2BV5S/events.json","paper":"https://pith.science/paper/4F6AOC26"},"agent_actions":{"view_html":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S","download_json":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S.json","view_paper":"https://pith.science/paper/4F6AOC26","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2101.08875&json=true","fetch_graph":"https://pith.science/api/pith-number/4F6AOC26UKGSCN3MLNSMY2BV5S/graph.json","fetch_events":"https://pith.science/api/pith-number/4F6AOC26UKGSCN3MLNSMY2BV5S/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S/action/timestamp_anchor","attest_storage":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S/action/storage_attestation","attest_author":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S/action/author_attestation","sign_citation":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S/action/citation_signature","submit_replication":"https://pith.science/pith/4F6AOC26UKGSCN3MLNSMY2BV5S/action/replication_record"}},"created_at":"2026-07-05T03:31:56.914209+00:00","updated_at":"2026-07-05T03:31:56.914209+00:00"}