{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:WBCZ3SJL6JHVHYDIAUPSOF4AFF","short_pith_number":"pith:WBCZ3SJL","schema_version":"1.0","canonical_sha256":"b0459dc92bf24f53e068051f27178029555bf205e5aba9aea74f5dfae13cddf9","source":{"kind":"arxiv","id":"2408.04001","version":1},"attestation_state":"computed","paper":{"title":"Holographic Gubser flow: A combined analytic and numerical study","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Alexander Soloviev, Ayan Mukhopadhyay, Sukrut Mondkar, Toshali Mitra","submitted_at":"2024-08-07T18:00:03Z","abstract_excerpt":"Gubser flow is an evolution with cylindrical and boost symmetries, which can be best studied by mapping the future wedge of Minkowski space (R$^{3,1}$) to dS$_3$ $\\times$ $\\mathbb{R}$ in a conformal relativistic theory. Here, we sharpen our previous analytic results and validate them via the first numerical exploration of the Gubser flow in a holographic conformal field theory.\n  Remarkably, the leading generic behavior at large de Sitter time is free-streaming in transverse directions and the sub-leading behavior is that of a color glass condensate. We also show that Gubser flow can be smooth"},"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":"2408.04001","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-th","submitted_at":"2024-08-07T18:00:03Z","cross_cats_sorted":["gr-qc","hep-ph"],"title_canon_sha256":"8543be2b4afced62c6cdd4561a919a83faab6f5a75d3001199dd371d0124ac0a","abstract_canon_sha256":"8eb9108330a0bbd44a57ba482cf71c3a18218841d8b981f775fe1943678b0146"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T09:28:53.927405Z","signature_b64":"dNk6gtwXCS9a0FpuAtIlb/7yCDvZ1z0nkWSj94dD8Fj0wsWOg/zMx9moNwPkuZt5PJaC4hd9mvk9RBCeK4QuBQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"b0459dc92bf24f53e068051f27178029555bf205e5aba9aea74f5dfae13cddf9","last_reissued_at":"2026-07-05T09:28:53.926909Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T09:28:53.926909Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Holographic Gubser flow: A combined analytic and numerical study","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["gr-qc","hep-ph"],"primary_cat":"hep-th","authors_text":"Alexander Soloviev, Ayan Mukhopadhyay, Sukrut Mondkar, Toshali Mitra","submitted_at":"2024-08-07T18:00:03Z","abstract_excerpt":"Gubser flow is an evolution with cylindrical and boost symmetries, which can be best studied by mapping the future wedge of Minkowski space (R$^{3,1}$) to dS$_3$ $\\times$ $\\mathbb{R}$ in a conformal relativistic theory. Here, we sharpen our previous analytic results and validate them via the first numerical exploration of the Gubser flow in a holographic conformal field theory.\n  Remarkably, the leading generic behavior at large de Sitter time is free-streaming in transverse directions and the sub-leading behavior is that of a color glass condensate. We also show that Gubser flow can be smooth"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2408.04001","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/2408.04001/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":"2408.04001","created_at":"2026-07-05T09:28:53.926968+00:00"},{"alias_kind":"arxiv_version","alias_value":"2408.04001v1","created_at":"2026-07-05T09:28:53.926968+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2408.04001","created_at":"2026-07-05T09:28:53.926968+00:00"},{"alias_kind":"pith_short_12","alias_value":"WBCZ3SJL6JHV","created_at":"2026-07-05T09:28:53.926968+00:00"},{"alias_kind":"pith_short_16","alias_value":"WBCZ3SJL6JHVHYDI","created_at":"2026-07-05T09:28:53.926968+00:00"},{"alias_kind":"pith_short_8","alias_value":"WBCZ3SJL","created_at":"2026-07-05T09:28:53.926968+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2410.01892","citing_title":"Superfluids in expanding backgrounds and attractor times","ref_index":48,"is_internal_anchor":false},{"citing_arxiv_id":"2604.07463","citing_title":"Decoding multiway gravitational junctions in AdS in terms of holographic quantum maps","ref_index":45,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF","json":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF.json","graph_json":"https://pith.science/api/pith-number/WBCZ3SJL6JHVHYDIAUPSOF4AFF/graph.json","events_json":"https://pith.science/api/pith-number/WBCZ3SJL6JHVHYDIAUPSOF4AFF/events.json","paper":"https://pith.science/paper/WBCZ3SJL"},"agent_actions":{"view_html":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF","download_json":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF.json","view_paper":"https://pith.science/paper/WBCZ3SJL","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2408.04001&json=true","fetch_graph":"https://pith.science/api/pith-number/WBCZ3SJL6JHVHYDIAUPSOF4AFF/graph.json","fetch_events":"https://pith.science/api/pith-number/WBCZ3SJL6JHVHYDIAUPSOF4AFF/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF/action/timestamp_anchor","attest_storage":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF/action/storage_attestation","attest_author":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF/action/author_attestation","sign_citation":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF/action/citation_signature","submit_replication":"https://pith.science/pith/WBCZ3SJL6JHVHYDIAUPSOF4AFF/action/replication_record"}},"created_at":"2026-07-05T09:28:53.926968+00:00","updated_at":"2026-07-05T09:28:53.926968+00:00"}