{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:CG6VC5U4FFBPIHLKTWRAAWMP3F","short_pith_number":"pith:CG6VC5U4","schema_version":"1.0","canonical_sha256":"11bd51769c2942f41d6a9da200598fd967d797ec1eabbd7d4c11b9093dc0f520","source":{"kind":"arxiv","id":"2307.11348","version":2},"attestation_state":"computed","paper":{"title":"All holographic systems have scar states","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","quant-ph"],"primary_cat":"hep-th","authors_text":"Alexey Milekhin, Nikolay Sukhov","submitted_at":"2023-07-21T04:48:05Z","abstract_excerpt":"Scar states are special finite-energy density, but non-thermal states of chaotic Hamiltonians. We argue that all holographic quantum field theories, including $\\mathcal{N}=4$ super Yang--Mills, have scar states. Their presence is tied to the existence of non-topological, horizonless soliton solutions in gravity: oscillons and a novel family of excited boson stars. We demonstrate that these solutions have periodic oscillations in the correlation functions and posses low-entanglement entropy as expected for scar states. Also we find that they can be very easily prepared with Euclidean path integ"},"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":"2307.11348","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2023-07-21T04:48:05Z","cross_cats_sorted":["gr-qc","quant-ph"],"title_canon_sha256":"27a54caad666c8473c1adaacd490261d435857cbf343af1a52bcf19b1641733e","abstract_canon_sha256":"f711ae31372e00aebcb08ff94e377c4320a89acbcd4acdeb94a267f3ebfa457c"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T08:33:31.294748Z","signature_b64":"yoW5fR0neb+SUn234FJkBMysF5/FsZPVhBiP8+bGvUhg0f4uGJUC30EbJ0QSeZU0g5cu6Uqznjnh6aKyhrPIBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"11bd51769c2942f41d6a9da200598fd967d797ec1eabbd7d4c11b9093dc0f520","last_reissued_at":"2026-07-05T08:33:31.294205Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T08:33:31.294205Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"All holographic systems have scar states","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","quant-ph"],"primary_cat":"hep-th","authors_text":"Alexey Milekhin, Nikolay Sukhov","submitted_at":"2023-07-21T04:48:05Z","abstract_excerpt":"Scar states are special finite-energy density, but non-thermal states of chaotic Hamiltonians. We argue that all holographic quantum field theories, including $\\mathcal{N}=4$ super Yang--Mills, have scar states. Their presence is tied to the existence of non-topological, horizonless soliton solutions in gravity: oscillons and a novel family of excited boson stars. We demonstrate that these solutions have periodic oscillations in the correlation functions and posses low-entanglement entropy as expected for scar states. Also we find that they can be very easily prepared with Euclidean path integ"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2307.11348","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/2307.11348/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":"2307.11348","created_at":"2026-07-05T08:33:31.294268+00:00"},{"alias_kind":"arxiv_version","alias_value":"2307.11348v2","created_at":"2026-07-05T08:33:31.294268+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2307.11348","created_at":"2026-07-05T08:33:31.294268+00:00"},{"alias_kind":"pith_short_12","alias_value":"CG6VC5U4FFBP","created_at":"2026-07-05T08:33:31.294268+00:00"},{"alias_kind":"pith_short_16","alias_value":"CG6VC5U4FFBPIHLK","created_at":"2026-07-05T08:33:31.294268+00:00"},{"alias_kind":"pith_short_8","alias_value":"CG6VC5U4","created_at":"2026-07-05T08:33:31.294268+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":6,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2605.02446","citing_title":"Quantum scars from holographic boson stars","ref_index":10,"is_internal_anchor":false},{"citing_arxiv_id":"2406.19441","citing_title":"Moduli Spaces in CFT: Large Charge Operators","ref_index":90,"is_internal_anchor":false},{"citing_arxiv_id":"2508.20094","citing_title":"(Un)solvable Matrix Models for BPS Correlators","ref_index":9,"is_internal_anchor":false},{"citing_arxiv_id":"2605.15180","citing_title":"Wormholes and Averaging over N","ref_index":22,"is_internal_anchor":false},{"citing_arxiv_id":"2604.18675","citing_title":"All-order fluctuating hydrodynamics of the SYK lattice","ref_index":25,"is_internal_anchor":false},{"citing_arxiv_id":"2605.02446","citing_title":"Quantum scars from holographic boson stars","ref_index":10,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F","json":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F.json","graph_json":"https://pith.science/api/pith-number/CG6VC5U4FFBPIHLKTWRAAWMP3F/graph.json","events_json":"https://pith.science/api/pith-number/CG6VC5U4FFBPIHLKTWRAAWMP3F/events.json","paper":"https://pith.science/paper/CG6VC5U4"},"agent_actions":{"view_html":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F","download_json":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F.json","view_paper":"https://pith.science/paper/CG6VC5U4","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2307.11348&json=true","fetch_graph":"https://pith.science/api/pith-number/CG6VC5U4FFBPIHLKTWRAAWMP3F/graph.json","fetch_events":"https://pith.science/api/pith-number/CG6VC5U4FFBPIHLKTWRAAWMP3F/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F/action/timestamp_anchor","attest_storage":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F/action/storage_attestation","attest_author":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F/action/author_attestation","sign_citation":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F/action/citation_signature","submit_replication":"https://pith.science/pith/CG6VC5U4FFBPIHLKTWRAAWMP3F/action/replication_record"}},"created_at":"2026-07-05T08:33:31.294268+00:00","updated_at":"2026-07-05T08:33:31.294268+00:00"}