{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2021:EFH5VACJN4LD7A5VL77AEEZDYP","short_pith_number":"pith:EFH5VACJ","schema_version":"1.0","canonical_sha256":"214fda80496f163f83b55ffe021323c3ff0a779cd0a81b48a9b6b0912b9d2d1c","source":{"kind":"arxiv","id":"2106.07649","version":1},"attestation_state":"computed","paper":{"title":"Non-Lorentzian Chaos and Cosmological Holography","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Aditya Sinha, Arjun Bagchi, Bharathkumar Radhakrishnan, Daniel Grumiller, Max Riegler, Shankhadeep Chakrabortty","submitted_at":"2021-06-14T18:00:00Z","abstract_excerpt":"We study chaos in non-Lorentzian field theories, specifically Galilean and Carrollian conformal field theories in two dimensions. In a large central charge limit, we find that the Lyapunov exponent saturates the bound on chaos, conjectured originally for relativistic field theories. We recover the same Lyapunov exponent holographically by a shock-wave calculation in three-dimensional flat space cosmologies, providing further evidence for flat space holography."},"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":"2106.07649","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2021-06-14T18:00:00Z","cross_cats_sorted":[],"title_canon_sha256":"d26137ba3711305b3edea4d851734cc451112da5c46492d1e5bad72a3957e63e","abstract_canon_sha256":"d6b502aa7e4e7bc410695daca1eec98153c3da4662fbb1bcf1854eddca26ebc8"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T03:34:27.303448Z","signature_b64":"xc8SlzHncm/B8xhbI61s3NcAPvuMyTI5eu68FAUrBjZkfnLb9RkcvH8WScEmgbcuxHjZY9r2JFp8lLm7idDOBw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"214fda80496f163f83b55ffe021323c3ff0a779cd0a81b48a9b6b0912b9d2d1c","last_reissued_at":"2026-07-05T03:34:27.303011Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T03:34:27.303011Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-Lorentzian Chaos and Cosmological Holography","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Aditya Sinha, Arjun Bagchi, Bharathkumar Radhakrishnan, Daniel Grumiller, Max Riegler, Shankhadeep Chakrabortty","submitted_at":"2021-06-14T18:00:00Z","abstract_excerpt":"We study chaos in non-Lorentzian field theories, specifically Galilean and Carrollian conformal field theories in two dimensions. In a large central charge limit, we find that the Lyapunov exponent saturates the bound on chaos, conjectured originally for relativistic field theories. We recover the same Lyapunov exponent holographically by a shock-wave calculation in three-dimensional flat space cosmologies, providing further evidence for flat space holography."},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2106.07649","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/2106.07649/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":"2106.07649","created_at":"2026-07-05T03:34:27.303065+00:00"},{"alias_kind":"arxiv_version","alias_value":"2106.07649v1","created_at":"2026-07-05T03:34:27.303065+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2106.07649","created_at":"2026-07-05T03:34:27.303065+00:00"},{"alias_kind":"pith_short_12","alias_value":"EFH5VACJN4LD","created_at":"2026-07-05T03:34:27.303065+00:00"},{"alias_kind":"pith_short_16","alias_value":"EFH5VACJN4LD7A5V","created_at":"2026-07-05T03:34:27.303065+00:00"},{"alias_kind":"pith_short_8","alias_value":"EFH5VACJ","created_at":"2026-07-05T03:34:27.303065+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.06826","citing_title":"BMS$_3$ invariant field theories","ref_index":39,"is_internal_anchor":true},{"citing_arxiv_id":"2506.16164","citing_title":"The Carrollian Kaleidoscope","ref_index":226,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP","json":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP.json","graph_json":"https://pith.science/api/pith-number/EFH5VACJN4LD7A5VL77AEEZDYP/graph.json","events_json":"https://pith.science/api/pith-number/EFH5VACJN4LD7A5VL77AEEZDYP/events.json","paper":"https://pith.science/paper/EFH5VACJ"},"agent_actions":{"view_html":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP","download_json":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP.json","view_paper":"https://pith.science/paper/EFH5VACJ","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2106.07649&json=true","fetch_graph":"https://pith.science/api/pith-number/EFH5VACJN4LD7A5VL77AEEZDYP/graph.json","fetch_events":"https://pith.science/api/pith-number/EFH5VACJN4LD7A5VL77AEEZDYP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP/action/storage_attestation","attest_author":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP/action/author_attestation","sign_citation":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP/action/citation_signature","submit_replication":"https://pith.science/pith/EFH5VACJN4LD7A5VL77AEEZDYP/action/replication_record"}},"created_at":"2026-07-05T03:34:27.303065+00:00","updated_at":"2026-07-05T03:34:27.303065+00:00"}