{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2022:SQORSS33BVTRLMOXDYSXE6YQLK","short_pith_number":"pith:SQORSS33","schema_version":"1.0","canonical_sha256":"941d194b7b0d6715b1d71e25727b105aa9d5f78a96d7d6997083ff7d8745ea9c","source":{"kind":"arxiv","id":"2205.02857","version":2},"attestation_state":"computed","paper":{"title":"Non-Gaussianities in Collider Energy Flux","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Hao Chen, Hua Xing Zhu, Ian Moult, Jesse Thaler","submitted_at":"2022-05-05T18:00:01Z","abstract_excerpt":"The microscopic dynamics of particle collisions is imprinted into the statistical properties of asymptotic energy flux, much like the dynamics of inflation is imprinted into the cosmic microwave background. This energy flux is characterized by correlation functions $\\langle \\mathcal{E}(\\vec n_1)\\cdots \\mathcal{E}(\\vec n_k) \\rangle$ of energy flow operators $ \\mathcal{E}(\\vec n)$. There has been significant recent progress in studying energy flux, including the calculation of multi-point correlation functions and their direct measurement inside high-energy jets at the Large Hadron Collider (LHC"},"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":"2205.02857","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-ph","submitted_at":"2022-05-05T18:00:01Z","cross_cats_sorted":["hep-ex","hep-th"],"title_canon_sha256":"fd3aaf485bc8aa2c18b3097f831f7dd157b51719b6097506ae437ba6dc9468a4","abstract_canon_sha256":"a7ffbbe5ac1997a74fc199e0fe7f5d2e37fd9686407fc345f0003d6a2c252d47"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T04:50:56.669652Z","signature_b64":"REcRQBqshv+LAoO6tmwDBJ8tZqYzVlh7L68sjwVse/fIs6ESZmZ1dLy7X7WJzdAKMIM3M8/KTVjmYQ+fvlm1Bw==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"941d194b7b0d6715b1d71e25727b105aa9d5f78a96d7d6997083ff7d8745ea9c","last_reissued_at":"2026-07-05T04:50:56.669118Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T04:50:56.669118Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Non-Gaussianities in Collider Energy Flux","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ex","hep-th"],"primary_cat":"hep-ph","authors_text":"Hao Chen, Hua Xing Zhu, Ian Moult, Jesse Thaler","submitted_at":"2022-05-05T18:00:01Z","abstract_excerpt":"The microscopic dynamics of particle collisions is imprinted into the statistical properties of asymptotic energy flux, much like the dynamics of inflation is imprinted into the cosmic microwave background. This energy flux is characterized by correlation functions $\\langle \\mathcal{E}(\\vec n_1)\\cdots \\mathcal{E}(\\vec n_k) \\rangle$ of energy flow operators $ \\mathcal{E}(\\vec n)$. There has been significant recent progress in studying energy flux, including the calculation of multi-point correlation functions and their direct measurement inside high-energy jets at the Large Hadron Collider (LHC"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2205.02857","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/2205.02857/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":"2205.02857","created_at":"2026-07-05T04:50:56.669186+00:00"},{"alias_kind":"arxiv_version","alias_value":"2205.02857v2","created_at":"2026-07-05T04:50:56.669186+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2205.02857","created_at":"2026-07-05T04:50:56.669186+00:00"},{"alias_kind":"pith_short_12","alias_value":"SQORSS33BVTR","created_at":"2026-07-05T04:50:56.669186+00:00"},{"alias_kind":"pith_short_16","alias_value":"SQORSS33BVTRLMOX","created_at":"2026-07-05T04:50:56.669186+00:00"},{"alias_kind":"pith_short_8","alias_value":"SQORSS33","created_at":"2026-07-05T04:50:56.669186+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":2,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2607.07792","citing_title":"Dissecting Parton Showers with Multi-Point Energy Correlators","ref_index":34,"is_internal_anchor":true},{"citing_arxiv_id":"2604.21971","citing_title":"Hydrodynamics and Energy Correlators","ref_index":19,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK","json":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK.json","graph_json":"https://pith.science/api/pith-number/SQORSS33BVTRLMOXDYSXE6YQLK/graph.json","events_json":"https://pith.science/api/pith-number/SQORSS33BVTRLMOXDYSXE6YQLK/events.json","paper":"https://pith.science/paper/SQORSS33"},"agent_actions":{"view_html":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK","download_json":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK.json","view_paper":"https://pith.science/paper/SQORSS33","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2205.02857&json=true","fetch_graph":"https://pith.science/api/pith-number/SQORSS33BVTRLMOXDYSXE6YQLK/graph.json","fetch_events":"https://pith.science/api/pith-number/SQORSS33BVTRLMOXDYSXE6YQLK/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK/action/timestamp_anchor","attest_storage":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK/action/storage_attestation","attest_author":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK/action/author_attestation","sign_citation":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK/action/citation_signature","submit_replication":"https://pith.science/pith/SQORSS33BVTRLMOXDYSXE6YQLK/action/replication_record"}},"created_at":"2026-07-05T04:50:56.669186+00:00","updated_at":"2026-07-05T04:50:56.669186+00:00"}