{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:CWE4DQGPIALAR6U25HMTGPBV7H","short_pith_number":"pith:CWE4DQGP","schema_version":"1.0","canonical_sha256":"1589c1c0cf401608fa9ae9d9333c35f9e113cefdebafe54fbddb2efc4ef661d9","source":{"kind":"arxiv","id":"2205.12968","version":2},"attestation_state":"computed","paper":{"title":"A precision test of averaging in AdS/CFT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.dis-nn","gr-qc"],"primary_cat":"hep-th","authors_text":"Jordan Cotler, Kristan Jensen","submitted_at":"2022-05-25T18:00:00Z","abstract_excerpt":"We reconsider the role of wormholes in the AdS/CFT correspondence. We focus on Euclidean wormholes that connect two asymptotically AdS or hyperbolic regions with $\\mathbb{S}^1\\times \\mathbb{S}^{d-1}$ boundary. There is no solution to Einstein's equations of this sort, as the wormholes possess a modulus that runs to infinity. To find on-shell wormholes we must stabilize this modulus, which we can do by fixing the total energy on the two boundaries. Such a wormhole gives the saddle point approximation to a non-standard problem in quantum gravity, where we fix two asymptotic boundaries and constr"},"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":"2205.12968","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2022-05-25T18:00:00Z","cross_cats_sorted":["cond-mat.dis-nn","gr-qc"],"title_canon_sha256":"ecc35beec43dbb48852ade872be4801a206efc30261ec6b216b620e6fa717af0","abstract_canon_sha256":"daf4ba02e8fde16b15b3ef4d2aa33cc2db2bd9edaea89924e05789a55d9ac6f3"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T05:20:11.794227Z","signature_b64":"ufvu4yaXDdBiQ5SikHGeI+PogGlKqa23JTWrA+prw3uIHApmHP/T78BTEQIdU2xNrASeUGmdNEnqZKVOx+BDCw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"1589c1c0cf401608fa9ae9d9333c35f9e113cefdebafe54fbddb2efc4ef661d9","last_reissued_at":"2026-07-05T05:20:11.793789Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T05:20:11.793789Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"A precision test of averaging in AdS/CFT","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["cond-mat.dis-nn","gr-qc"],"primary_cat":"hep-th","authors_text":"Jordan Cotler, Kristan Jensen","submitted_at":"2022-05-25T18:00:00Z","abstract_excerpt":"We reconsider the role of wormholes in the AdS/CFT correspondence. We focus on Euclidean wormholes that connect two asymptotically AdS or hyperbolic regions with $\\mathbb{S}^1\\times \\mathbb{S}^{d-1}$ boundary. There is no solution to Einstein's equations of this sort, as the wormholes possess a modulus that runs to infinity. To find on-shell wormholes we must stabilize this modulus, which we can do by fixing the total energy on the two boundaries. Such a wormhole gives the saddle point approximation to a non-standard problem in quantum gravity, where we fix two asymptotic boundaries and constr"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.12968","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/2205.12968/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":"2205.12968","created_at":"2026-07-05T05:20:11.793854+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.12968v2","created_at":"2026-07-05T05:20:11.793854+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.12968","created_at":"2026-07-05T05:20:11.793854+00:00"},{"alias_kind":"pith_short_12","alias_value":"CWE4DQGPIALA","created_at":"2026-07-05T05:20:11.793854+00:00"},{"alias_kind":"pith_short_16","alias_value":"CWE4DQGPIALAR6U2","created_at":"2026-07-05T05:20:11.793854+00:00"},{"alias_kind":"pith_short_8","alias_value":"CWE4DQGP","created_at":"2026-07-05T05:20:11.793854+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.25251","citing_title":"Some universalities in the partition functions of low-dimensional gravity models","ref_index":34,"is_internal_anchor":false},{"citing_arxiv_id":"2605.18725","citing_title":"Signatures of Quantum Chaos in the D1D5 System","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15180","citing_title":"Wormholes and Averaging over N","ref_index":19,"is_internal_anchor":false},{"citing_arxiv_id":"2604.12784","citing_title":"Quantum chaos and the holographic principle","ref_index":30,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H","json":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H.json","graph_json":"https://pith.science/api/pith-number/CWE4DQGPIALAR6U25HMTGPBV7H/graph.json","events_json":"https://pith.science/api/pith-number/CWE4DQGPIALAR6U25HMTGPBV7H/events.json","paper":"https://pith.science/paper/CWE4DQGP"},"agent_actions":{"view_html":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H","download_json":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H.json","view_paper":"https://pith.science/paper/CWE4DQGP","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.12968&json=true","fetch_graph":"https://pith.science/api/pith-number/CWE4DQGPIALAR6U25HMTGPBV7H/graph.json","fetch_events":"https://pith.science/api/pith-number/CWE4DQGPIALAR6U25HMTGPBV7H/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H/action/storage_attestation","attest_author":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H/action/author_attestation","sign_citation":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H/action/citation_signature","submit_replication":"https://pith.science/pith/CWE4DQGPIALAR6U25HMTGPBV7H/action/replication_record"}},"created_at":"2026-07-05T05:20:11.793854+00:00","updated_at":"2026-07-05T05:20:11.793854+00:00"}