{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:5OMHHVC23V5LB6ZKBYGJZUFC4N","short_pith_number":"pith:5OMHHVC2","schema_version":"1.0","canonical_sha256":"eb9873d45add7ab0fb2a0e0c9cd0a2e373762f661194e8e4958efdbb097e87fa","source":{"kind":"arxiv","id":"2408.12330","version":5},"attestation_state":"computed","paper":{"title":"Pole-skipping in two-dimensional de Sitter spacetime and double-scaled SYK model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Haiming Yuan, Keun-Young Kim, Xian-Hui Ge","submitted_at":"2024-08-22T12:17:45Z","abstract_excerpt":"We develop the pole-skipping structure in de Sitter (dS) spacetime and find that their leading frequencies satisfy the relation $\\omega_{dS}=i2\\pi T_{dS}(1-s)$, where $T_{dS}=1/2\\pi L$ and $s$ denotes spin. In the two-dimensional dS spacetime, the pole-skipping points near the cosmic horizon $r=L$ for the scalar field of spin-0 and the fermionic field of spin-$\\frac{1}{2}$ correspond one-to-one with those in the classical limit as $\\lambda\\rightarrow 0$ in double-scaled Sachdev-Ye-Kitaev model when the temperature is infinite (DSSYK$_\\infty$). This provides a numerical correspondence between q"},"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":"2408.12330","kind":"arxiv","version":5},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-08-22T12:17:45Z","cross_cats_sorted":[],"title_canon_sha256":"4eed99c974a00662f37b9d6794bc344e50d50d4a8ea3eab2013419a6eaf95c9d","abstract_canon_sha256":"8198a6a3be96f5431bb49d7edf9aaaa7c2ab16a03cb0f5847ae64695f782074c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:39:42.799908Z","signature_b64":"rzmuAuHItXUP387Xoujsfu+0uIj0qO8jPgLWzCpVynwG/yMsdj019l7yJLASfdgAEKdyWircQgVnj2uMXFO5Ag==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"eb9873d45add7ab0fb2a0e0c9cd0a2e373762f661194e8e4958efdbb097e87fa","last_reissued_at":"2026-07-05T11:39:42.799402Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:39:42.799402Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Pole-skipping in two-dimensional de Sitter spacetime and double-scaled SYK model","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Haiming Yuan, Keun-Young Kim, Xian-Hui Ge","submitted_at":"2024-08-22T12:17:45Z","abstract_excerpt":"We develop the pole-skipping structure in de Sitter (dS) spacetime and find that their leading frequencies satisfy the relation $\\omega_{dS}=i2\\pi T_{dS}(1-s)$, where $T_{dS}=1/2\\pi L$ and $s$ denotes spin. In the two-dimensional dS spacetime, the pole-skipping points near the cosmic horizon $r=L$ for the scalar field of spin-0 and the fermionic field of spin-$\\frac{1}{2}$ correspond one-to-one with those in the classical limit as $\\lambda\\rightarrow 0$ in double-scaled Sachdev-Ye-Kitaev model when the temperature is infinite (DSSYK$_\\infty$). This provides a numerical correspondence between q"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.12330","kind":"arxiv","version":5},"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/2408.12330/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":"2408.12330","created_at":"2026-07-05T11:39:42.799461+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.12330v5","created_at":"2026-07-05T11:39:42.799461+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.12330","created_at":"2026-07-05T11:39:42.799461+00:00"},{"alias_kind":"pith_short_12","alias_value":"5OMHHVC23V5L","created_at":"2026-07-05T11:39:42.799461+00:00"},{"alias_kind":"pith_short_16","alias_value":"5OMHHVC23V5LB6ZK","created_at":"2026-07-05T11:39:42.799461+00:00"},{"alias_kind":"pith_short_8","alias_value":"5OMHHVC2","created_at":"2026-07-05T11:39:42.799461+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.13956","citing_title":"q-Askey Deformations of Double-Scaled SYK","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2511.03779","citing_title":"Cosmological Entanglement Entropy from the von Neumann Algebra of Double-Scaled SYK & Its Connection with Krylov Complexity","ref_index":98,"is_internal_anchor":false},{"citing_arxiv_id":"2601.09801","citing_title":"Probing the Chaos to Integrability Transition in Double-Scaled SYK","ref_index":71,"is_internal_anchor":false},{"citing_arxiv_id":"2602.06113","citing_title":"Deforming the Double-Scaled SYK & Reaching the Stretched Horizon From Finite Cutoff Holography","ref_index":131,"is_internal_anchor":false},{"citing_arxiv_id":"2605.13956","citing_title":"q-Askey Deformations of Double-Scaled SYK","ref_index":38,"is_internal_anchor":false},{"citing_arxiv_id":"2604.14638","citing_title":"Probing bulk geometry via pole skipping: from static to rotating spacetimes","ref_index":27,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N","json":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N.json","graph_json":"https://pith.science/api/pith-number/5OMHHVC23V5LB6ZKBYGJZUFC4N/graph.json","events_json":"https://pith.science/api/pith-number/5OMHHVC23V5LB6ZKBYGJZUFC4N/events.json","paper":"https://pith.science/paper/5OMHHVC2"},"agent_actions":{"view_html":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N","download_json":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N.json","view_paper":"https://pith.science/paper/5OMHHVC2","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.12330&json=true","fetch_graph":"https://pith.science/api/pith-number/5OMHHVC23V5LB6ZKBYGJZUFC4N/graph.json","fetch_events":"https://pith.science/api/pith-number/5OMHHVC23V5LB6ZKBYGJZUFC4N/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N/action/timestamp_anchor","attest_storage":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N/action/storage_attestation","attest_author":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N/action/author_attestation","sign_citation":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N/action/citation_signature","submit_replication":"https://pith.science/pith/5OMHHVC23V5LB6ZKBYGJZUFC4N/action/replication_record"}},"created_at":"2026-07-05T11:39:42.799461+00:00","updated_at":"2026-07-05T11:39:42.799461+00:00"}