{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2023:OWO4ERJU6BVBFFR6OCEB2ZPFIA","short_pith_number":"pith:OWO4ERJU","schema_version":"1.0","canonical_sha256":"759dc24534f06a12963e70881d65e5400b57631ebfd21b70e5d3a39d0f7df9ef","source":{"kind":"arxiv","id":"2306.10896","version":1},"attestation_state":"computed","paper":{"title":"Dilaton-induced open quantum dynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th","quant-ph"],"primary_cat":"hep-ph","authors_text":"Caroline Voith, Christian K\\\"ading, Mario Pitschmann","submitted_at":"2023-06-19T12:49:59Z","abstract_excerpt":"In modern cosmology, scalar fields with screening mechanisms are often used as explanations for phenomena like dark energy or dark matter. Amongst a zoo of models, the environment dependent dilaton, screened by the Polyakov-Damour mechanism, is one of the least constrained ones. Using recently developed path integral tools for directly computing reduced density matrices, we study the open quantum dynamics of a probe, modelled by another real scalar field, induced by interactions with an environment comprising fluctuations of a dilaton. As the leading effect, we extract a correction to the prob"},"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":"2306.10896","kind":"arxiv","version":1},"metadata":{"license":"http://creativecommons.org/licenses/by/4.0/","primary_cat":"hep-ph","submitted_at":"2023-06-19T12:49:59Z","cross_cats_sorted":["astro-ph.CO","gr-qc","hep-th","quant-ph"],"title_canon_sha256":"2a1729f068da1691682f254f0d024e8e9faedf45e3ea444f0d4325ca975bcfa7","abstract_canon_sha256":"1c7d7ca8a0076216e97759b60b3b299d56fe5a64f7bba1936a62fbfe71327692"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-05T06:46:33.255798Z","signature_b64":"u2TcN+H9YozM0Cb7dzREqPdJ19BStzm7Qde4z4PfJ9pw9flbxnjvIq1/weoKcQlxgssftwsd4qFNDoeoDRvpDA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"759dc24534f06a12963e70881d65e5400b57631ebfd21b70e5d3a39d0f7df9ef","last_reissued_at":"2026-07-05T06:46:33.255208Z","signature_status":"signed_v1","first_computed_at":"2026-07-05T06:46:33.255208Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Dilaton-induced open quantum dynamics","license":"http://creativecommons.org/licenses/by/4.0/","headline":"","cross_cats":["astro-ph.CO","gr-qc","hep-th","quant-ph"],"primary_cat":"hep-ph","authors_text":"Caroline Voith, Christian K\\\"ading, Mario Pitschmann","submitted_at":"2023-06-19T12:49:59Z","abstract_excerpt":"In modern cosmology, scalar fields with screening mechanisms are often used as explanations for phenomena like dark energy or dark matter. Amongst a zoo of models, the environment dependent dilaton, screened by the Polyakov-Damour mechanism, is one of the least constrained ones. Using recently developed path integral tools for directly computing reduced density matrices, we study the open quantum dynamics of a probe, modelled by another real scalar field, induced by interactions with an environment comprising fluctuations of a dilaton. As the leading effect, we extract a correction to the prob"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"2306.10896","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/2306.10896/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":"2306.10896","created_at":"2026-07-05T06:46:33.255270+00:00"},{"alias_kind":"arxiv_version","alias_value":"2306.10896v1","created_at":"2026-07-05T06:46:33.255270+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.2306.10896","created_at":"2026-07-05T06:46:33.255270+00:00"},{"alias_kind":"pith_short_12","alias_value":"OWO4ERJU6BVB","created_at":"2026-07-05T06:46:33.255270+00:00"},{"alias_kind":"pith_short_16","alias_value":"OWO4ERJU6BVBFFR6","created_at":"2026-07-05T06:46:33.255270+00:00"},{"alias_kind":"pith_short_8","alias_value":"OWO4ERJU","created_at":"2026-07-05T06:46:33.255270+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":4,"internal_anchor_count":0,"sample":[{"citing_arxiv_id":"2606.03440","citing_title":"Experimental test of symmetron-field based dark energy model using neutron interferometry","ref_index":23,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26941","citing_title":"Schwinger-Keldysh Path Integral for Gauge theories","ref_index":145,"is_internal_anchor":false},{"citing_arxiv_id":"2512.01590","citing_title":"Directly computing Wigner functions for open quantum systems","ref_index":60,"is_internal_anchor":false},{"citing_arxiv_id":"2604.26941","citing_title":"Schwinger-Keldysh Path Integral for Gauge theories","ref_index":145,"is_internal_anchor":false}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA","json":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA.json","graph_json":"https://pith.science/api/pith-number/OWO4ERJU6BVBFFR6OCEB2ZPFIA/graph.json","events_json":"https://pith.science/api/pith-number/OWO4ERJU6BVBFFR6OCEB2ZPFIA/events.json","paper":"https://pith.science/paper/OWO4ERJU"},"agent_actions":{"view_html":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA","download_json":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA.json","view_paper":"https://pith.science/paper/OWO4ERJU","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=2306.10896&json=true","fetch_graph":"https://pith.science/api/pith-number/OWO4ERJU6BVBFFR6OCEB2ZPFIA/graph.json","fetch_events":"https://pith.science/api/pith-number/OWO4ERJU6BVBFFR6OCEB2ZPFIA/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA/action/timestamp_anchor","attest_storage":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA/action/storage_attestation","attest_author":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA/action/author_attestation","sign_citation":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA/action/citation_signature","submit_replication":"https://pith.science/pith/OWO4ERJU6BVBFFR6OCEB2ZPFIA/action/replication_record"}},"created_at":"2026-07-05T06:46:33.255270+00:00","updated_at":"2026-07-05T06:46:33.255270+00:00"}