{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:GNAPMZFS7DB5K4OH5VJFBKVHYZ","short_pith_number":"pith:GNAPMZFS","schema_version":"1.0","canonical_sha256":"3340f664b2f8c3d571c7ed5250aaa7c653a6e37d2306acb6484fa7117dffa344","source":{"kind":"arxiv","id":"2503.12227","version":1},"attestation_state":"computed","paper":{"title":"Ordinary wormholes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alexander Maloney, Mark Van Raamsdonk, Viraj Meruliya","submitted_at":"2025-03-15T18:45:31Z","abstract_excerpt":"Euclidean wormholes have played a key role in the recent ``disorder averaged\" approaches to quantum gravity and holography, but are typically only considered in somewhat special theories of gravity, such as theories in low dimensions or theories with exotic matter content (such as axions). These exotic theories have advantage that both the matter and gravitational sectors can be treated completely classically. However, once this constraint is relaxed we find that Euclidean wormholes arise generically, with no special constraints on the matter content. The key point is that there is a self-cons"},"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":"2503.12227","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2025-03-15T18:45:31Z","cross_cats_sorted":["gr-qc"],"title_canon_sha256":"3b4706a24b31b3877c944410fccfdf17d2b329279da8ac68774a359c3254748b","abstract_canon_sha256":"b49b49be8696e27ee4b365da79b4a93d1e0f493ebb7eab0198d74c80339e53fe"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:32:07.847250Z","signature_b64":"HYtuXMJUF3RbtHoiFZonvM9j7xyD3oqiOVLE2GuJvTKDWytv5fcOVzr0lygvSpu9f6WN8s8FVpY81WqiH20dCA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3340f664b2f8c3d571c7ed5250aaa7c653a6e37d2306acb6484fa7117dffa344","last_reissued_at":"2026-07-05T10:32:07.846625Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:32:07.846625Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Ordinary wormholes","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc"],"primary_cat":"hep-th","authors_text":"Alexander Maloney, Mark Van Raamsdonk, Viraj Meruliya","submitted_at":"2025-03-15T18:45:31Z","abstract_excerpt":"Euclidean wormholes have played a key role in the recent ``disorder averaged\" approaches to quantum gravity and holography, but are typically only considered in somewhat special theories of gravity, such as theories in low dimensions or theories with exotic matter content (such as axions). These exotic theories have advantage that both the matter and gravitational sectors can be treated completely classically. However, once this constraint is relaxed we find that Euclidean wormholes arise generically, with no special constraints on the matter content. The key point is that there is a self-cons"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2503.12227","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/2503.12227/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":"2503.12227","created_at":"2026-07-05T10:32:07.846695+00:00"},{"alias_kind":"arxiv_version","alias_value":"2503.12227v1","created_at":"2026-07-05T10:32:07.846695+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2503.12227","created_at":"2026-07-05T10:32:07.846695+00:00"},{"alias_kind":"pith_short_12","alias_value":"GNAPMZFS7DB5","created_at":"2026-07-05T10:32:07.846695+00:00"},{"alias_kind":"pith_short_16","alias_value":"GNAPMZFS7DB5K4OH","created_at":"2026-07-05T10:32:07.846695+00:00"},{"alias_kind":"pith_short_8","alias_value":"GNAPMZFS","created_at":"2026-07-05T10:32:07.846695+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":5,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.13777","citing_title":"Before the Bang: Wormholes at the Dawn of the Universe","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2601.10906","citing_title":"Menagerie of Euclidean constructions for 3D holographic cosmologies","ref_index":1,"is_internal_anchor":false},{"citing_arxiv_id":"2602.23432","citing_title":"A Menagerie of Wormholes and Cosmologies in the Gravitational Path Integral","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13777","citing_title":"Before the Bang: Wormholes at the Dawn of the Universe","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2605.05336","citing_title":"Wormholes and the imaginary distance bound","ref_index":43,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ","json":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ.json","graph_json":"https://pith.science/api/pith-number/GNAPMZFS7DB5K4OH5VJFBKVHYZ/graph.json","events_json":"https://pith.science/api/pith-number/GNAPMZFS7DB5K4OH5VJFBKVHYZ/events.json","paper":"https://pith.science/paper/GNAPMZFS"},"agent_actions":{"view_html":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ","download_json":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ.json","view_paper":"https://pith.science/paper/GNAPMZFS","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2503.12227&json=true","fetch_graph":"https://pith.science/api/pith-number/GNAPMZFS7DB5K4OH5VJFBKVHYZ/graph.json","fetch_events":"https://pith.science/api/pith-number/GNAPMZFS7DB5K4OH5VJFBKVHYZ/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ/action/timestamp_anchor","attest_storage":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ/action/storage_attestation","attest_author":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ/action/author_attestation","sign_citation":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ/action/citation_signature","submit_replication":"https://pith.science/pith/GNAPMZFS7DB5K4OH5VJFBKVHYZ/action/replication_record"}},"created_at":"2026-07-05T10:32:07.846695+00:00","updated_at":"2026-07-05T10:32:07.846695+00:00"}