{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2025:HK3OLZFAHL6BOQBGDPUXGH5PF7","short_pith_number":"pith:HK3OLZFA","schema_version":"1.0","canonical_sha256":"3ab6e5e4a03afc1740261be9731faf2febb9980030fa89bea963ec3557be7201","source":{"kind":"arxiv","id":"2502.03031","version":3},"attestation_state":"computed","paper":{"title":"On the Underlying Nonrelativistic Nature of Relativistic Holography","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Alberto Guijosa","submitted_at":"2025-02-05T09:34:37Z","abstract_excerpt":"Over the past quarter century, considerable effort has been invested in the study of nonrelativistic (NR) string theory, its U-dual NR brane theories, and their geometric foundations in (generalized) Newton-Cartan geometry. Many interesting results have been obtained, both for their intrinsic value and in the hope that they hold useful lessons for relativistic string/M theory. By synthesizing two strands of recent developments (especially, arXiv:2312.13243 and arXiv:2410.03591), we argue that this hope has already come to fruition, because standard, relativistic holography can now be recognize"},"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":"2502.03031","kind":"arxiv","version":3},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2025-02-05T09:34:37Z","cross_cats_sorted":[],"title_canon_sha256":"de787cc8cefb60bf75b93268d108a9c7b1f169dec718db878b71ecc44f817d49","abstract_canon_sha256":"3ef35cdcb3df32834f410828cfae6062be6d04e0bedffeff401453db863133bb"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T11:38:26.820580Z","signature_b64":"Wr8LFOw7xOn+NMEtnOO14CXO90cyTkJMHtVnabU1BD96MCu6PSWeDK0LJmQ1cPWjRCluq+E1utWm3/ks8pGpDg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"3ab6e5e4a03afc1740261be9731faf2febb9980030fa89bea963ec3557be7201","last_reissued_at":"2026-07-05T11:38:26.820029Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T11:38:26.820029Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the Underlying Nonrelativistic Nature of Relativistic Holography","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":[],"primary_cat":"hep-th","authors_text":"Alberto Guijosa","submitted_at":"2025-02-05T09:34:37Z","abstract_excerpt":"Over the past quarter century, considerable effort has been invested in the study of nonrelativistic (NR) string theory, its U-dual NR brane theories, and their geometric foundations in (generalized) Newton-Cartan geometry. Many interesting results have been obtained, both for their intrinsic value and in the hope that they hold useful lessons for relativistic string/M theory. By synthesizing two strands of recent developments (especially, arXiv:2312.13243 and arXiv:2410.03591), we argue that this hope has already come to fruition, because standard, relativistic holography can now be recognize"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2502.03031","kind":"arxiv","version":3},"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/2502.03031/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":"2502.03031","created_at":"2026-07-05T11:38:26.820098+00:00"},{"alias_kind":"arxiv_version","alias_value":"2502.03031v3","created_at":"2026-07-05T11:38:26.820098+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2502.03031","created_at":"2026-07-05T11:38:26.820098+00:00"},{"alias_kind":"pith_short_12","alias_value":"HK3OLZFAHL6B","created_at":"2026-07-05T11:38:26.820098+00:00"},{"alias_kind":"pith_short_16","alias_value":"HK3OLZFAHL6BOQBG","created_at":"2026-07-05T11:38:26.820098+00:00"},{"alias_kind":"pith_short_8","alias_value":"HK3OLZFA","created_at":"2026-07-05T11:38:26.820098+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":3,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2604.27449","citing_title":"Phase-Space Contractions of Carrollian Black-Hole Thermodynamics","ref_index":42,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27449","citing_title":"Phase-Space Contractions of Carrollian Black-Hole Thermodynamics","ref_index":39,"is_internal_anchor":false},{"citing_arxiv_id":"2604.27449","citing_title":"Phase-Space Contractions of Carrollian Black-Hole Thermodynamics","ref_index":39,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7","json":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7.json","graph_json":"https://pith.science/api/pith-number/HK3OLZFAHL6BOQBGDPUXGH5PF7/graph.json","events_json":"https://pith.science/api/pith-number/HK3OLZFAHL6BOQBGDPUXGH5PF7/events.json","paper":"https://pith.science/paper/HK3OLZFA"},"agent_actions":{"view_html":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7","download_json":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7.json","view_paper":"https://pith.science/paper/HK3OLZFA","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2502.03031&json=true","fetch_graph":"https://pith.science/api/pith-number/HK3OLZFAHL6BOQBGDPUXGH5PF7/graph.json","fetch_events":"https://pith.science/api/pith-number/HK3OLZFAHL6BOQBGDPUXGH5PF7/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7/action/timestamp_anchor","attest_storage":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7/action/storage_attestation","attest_author":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7/action/author_attestation","sign_citation":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7/action/citation_signature","submit_replication":"https://pith.science/pith/HK3OLZFAHL6BOQBGDPUXGH5PF7/action/replication_record"}},"created_at":"2026-07-05T11:38:26.820098+00:00","updated_at":"2026-07-05T11:38:26.820098+00:00"}