{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2010:U6T5GKFKO6P2FEPITLDQ4PBJDP","short_pith_number":"pith:U6T5GKFK","schema_version":"1.0","canonical_sha256":"a7a7d328aa779fa291e89ac70e3c291beb38136462a8a7d7b3c20b75bd8c079e","source":{"kind":"arxiv","id":"1011.3990","version":2},"attestation_state":"computed","paper":{"title":"Interplay between scintillation and ionization in liquid xenon Dark Matter searches","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.IM","authors_text":"Fedor Bezrukov, Felix Kahlhoefer, Manfred Lindner","submitted_at":"2010-11-17T16:20:30Z","abstract_excerpt":"We provide a new way of constraining the relative scintillation efficiency L_eff for liquid xenon. Using a simple estimate for the electronic and nuclear stopping powers together with an analysis of recombination processes we predict both the ionization and the scintillation yields. Using presently available data for the ionization yield, we can use the correlation between these two quantities to constrain L_eff from below. Moreover, we argue that more reliable data on the ionization yield would allow to verify our assumptions on the atomic cross sections and to predict the value of L_eff. We "},"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":"1011.3990","kind":"arxiv","version":2},"metadata":{"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"astro-ph.IM","submitted_at":"2010-11-17T16:20:30Z","cross_cats_sorted":["hep-ph"],"title_canon_sha256":"af7083c9b20587e6fb6053e2fdde6b88c9734ed896cf09bbea544dd97e08dbc5","abstract_canon_sha256":"829c4f84db7ed6107a6b69d110e08162348d74e916e242df20e55188880086d2"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-05-18T04:15:04.277616Z","signature_b64":"KA6NLsYFfJRp20Lr8zZB11ejPHFW48Gx8Lmf14HL+L05ken/hk0R/b+4c/W3zpa9rz36h97ZXvIdNeMG78PfBA==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"a7a7d328aa779fa291e89ac70e3c291beb38136462a8a7d7b3c20b75bd8c079e","last_reissued_at":"2026-05-18T04:15:04.276782Z","signature_status":"signed_v1","first_computed_at":"2026-05-18T04:15:04.276782Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"Interplay between scintillation and ionization in liquid xenon Dark Matter searches","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","headline":"","cross_cats":["hep-ph"],"primary_cat":"astro-ph.IM","authors_text":"Fedor Bezrukov, Felix Kahlhoefer, Manfred Lindner","submitted_at":"2010-11-17T16:20:30Z","abstract_excerpt":"We provide a new way of constraining the relative scintillation efficiency L_eff for liquid xenon. Using a simple estimate for the electronic and nuclear stopping powers together with an analysis of recombination processes we predict both the ionization and the scintillation yields. Using presently available data for the ionization yield, we can use the correlation between these two quantities to constrain L_eff from below. Moreover, we argue that more reliable data on the ionization yield would allow to verify our assumptions on the atomic cross sections and to predict the value of L_eff. We "},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1011.3990","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":""},"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":"1011.3990","created_at":"2026-05-18T04:15:04.276921+00:00"},{"alias_kind":"arxiv_version","alias_value":"1011.3990v2","created_at":"2026-05-18T04:15:04.276921+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1011.3990","created_at":"2026-05-18T04:15:04.276921+00:00"},{"alias_kind":"pith_short_12","alias_value":"U6T5GKFKO6P2","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_16","alias_value":"U6T5GKFKO6P2FEPI","created_at":"2026-05-18T12:26:15.391820+00:00"},{"alias_kind":"pith_short_8","alias_value":"U6T5GKFK","created_at":"2026-05-18T12:26:15.391820+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":1,"internal_anchor_count":1,"sample":[{"citing_arxiv_id":"2511.13629","citing_title":"Sensitivity to low-mass WIMPs with an improved liquid argon ionization response model within the DarkSide programme","ref_index":8,"is_internal_anchor":true}]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP","json":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP.json","graph_json":"https://pith.science/api/pith-number/U6T5GKFKO6P2FEPITLDQ4PBJDP/graph.json","events_json":"https://pith.science/api/pith-number/U6T5GKFKO6P2FEPITLDQ4PBJDP/events.json","paper":"https://pith.science/paper/U6T5GKFK"},"agent_actions":{"view_html":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP","download_json":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP.json","view_paper":"https://pith.science/paper/U6T5GKFK","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=1011.3990&json=true","fetch_graph":"https://pith.science/api/pith-number/U6T5GKFKO6P2FEPITLDQ4PBJDP/graph.json","fetch_events":"https://pith.science/api/pith-number/U6T5GKFKO6P2FEPITLDQ4PBJDP/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP/action/timestamp_anchor","attest_storage":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP/action/storage_attestation","attest_author":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP/action/author_attestation","sign_citation":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP/action/citation_signature","submit_replication":"https://pith.science/pith/U6T5GKFKO6P2FEPITLDQ4PBJDP/action/replication_record"}},"created_at":"2026-05-18T04:15:04.276921+00:00","updated_at":"2026-05-18T04:15:04.276921+00:00"}