{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2024:FTDKILVW4P6EDE5U7NT2QSEJZH","short_pith_number":"pith:FTDKILVW","schema_version":"1.0","canonical_sha256":"2cc6a42eb6e3fc4193b4fb67a84889c9ea99f97e19ecd5316695f34922c6ca86","source":{"kind":"arxiv","id":"2412.02917","version":2},"attestation_state":"computed","paper":{"title":"Probability Distribution for Vacuum Energy Flux Fluctuations in Two Spacetime Dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","math-ph","math.MP"],"primary_cat":"hep-th","authors_text":"Christopher J. Fewster, L. H. Ford","submitted_at":"2024-12-04T00:08:15Z","abstract_excerpt":"The probability distribution for vacuum fluctuations of the energy flux in two dimensions will be constructed, along with the joint distribution of energy flux and energy density. Our approach will be based on previous work on probability distributions for the energy density in two dimensional conformal field theory. In both cases, the relevant stress tensor component must be averaged in time, and the results are sensitive to the form of the averaging function. Here we present results for two classes of such functions, which include the Gaussian and Lorentzian functions. The distribution for t"},"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":"2412.02917","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"hep-th","submitted_at":"2024-12-04T00:08:15Z","cross_cats_sorted":["gr-qc","math-ph","math.MP"],"title_canon_sha256":"80ca7eaf9c92a79940f6ff0a087fa1c82578f855472f62f95b5e38d7c188c5e0","abstract_canon_sha256":"5933d5d9ac9f274502c90149a0eba2480f54e2d583c14ef1cf6e694dbac8869a"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T10:47:20.683837Z","signature_b64":"EzSD3zzmvdPZCg4f3NK+eGSoJvFgaWynPRE6b+s/wH+8+7yzT5YMdGS3D2tX0m90sluqepy2LEVrnAjIWbD8Bg==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"2cc6a42eb6e3fc4193b4fb67a84889c9ea99f97e19ecd5316695f34922c6ca86","last_reissued_at":"2026-07-05T10:47:20.683363Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T10:47:20.683363Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Probability Distribution for Vacuum Energy Flux Fluctuations in Two Spacetime Dimensions","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["gr-qc","math-ph","math.MP"],"primary_cat":"hep-th","authors_text":"Christopher J. Fewster, L. H. Ford","submitted_at":"2024-12-04T00:08:15Z","abstract_excerpt":"The probability distribution for vacuum fluctuations of the energy flux in two dimensions will be constructed, along with the joint distribution of energy flux and energy density. Our approach will be based on previous work on probability distributions for the energy density in two dimensional conformal field theory. In both cases, the relevant stress tensor component must be averaged in time, and the results are sensitive to the form of the averaging function. Here we present results for two classes of such functions, which include the Gaussian and Lorentzian functions. The distribution for t"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2412.02917","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/2412.02917/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":"2412.02917","created_at":"2026-07-05T10:47:20.683429+00:00"},{"alias_kind":"arxiv_version","alias_value":"2412.02917v2","created_at":"2026-07-05T10:47:20.683429+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2412.02917","created_at":"2026-07-05T10:47:20.683429+00:00"},{"alias_kind":"pith_short_12","alias_value":"FTDKILVW4P6E","created_at":"2026-07-05T10:47:20.683429+00:00"},{"alias_kind":"pith_short_16","alias_value":"FTDKILVW4P6EDE5U","created_at":"2026-07-05T10:47:20.683429+00:00"},{"alias_kind":"pith_short_8","alias_value":"FTDKILVW","created_at":"2026-07-05T10:47:20.683429+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH","json":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH.json","graph_json":"https://pith.science/api/pith-number/FTDKILVW4P6EDE5U7NT2QSEJZH/graph.json","events_json":"https://pith.science/api/pith-number/FTDKILVW4P6EDE5U7NT2QSEJZH/events.json","paper":"https://pith.science/paper/FTDKILVW"},"agent_actions":{"view_html":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH","download_json":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH.json","view_paper":"https://pith.science/paper/FTDKILVW","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2412.02917&json=true","fetch_graph":"https://pith.science/api/pith-number/FTDKILVW4P6EDE5U7NT2QSEJZH/graph.json","fetch_events":"https://pith.science/api/pith-number/FTDKILVW4P6EDE5U7NT2QSEJZH/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH/action/timestamp_anchor","attest_storage":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH/action/storage_attestation","attest_author":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH/action/author_attestation","sign_citation":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH/action/citation_signature","submit_replication":"https://pith.science/pith/FTDKILVW4P6EDE5U7NT2QSEJZH/action/replication_record"}},"created_at":"2026-07-05T10:47:20.683429+00:00","updated_at":"2026-07-05T10:47:20.683429+00:00"}