{"state_type":"pith_open_graph_state","state_version":"1.0","pith_number":"pith:2013:FVMCBTLOV62WLSALVXXULK5Z2T","merge_version":"pith-open-graph-merge-v1","event_count":2,"valid_event_count":2,"invalid_event_count":0,"equivocation_count":0,"current":{"canonical_record":{"metadata":{"abstract_canon_sha256":"ed44ecc00434d834142dffafef23a18fa2b6c727571ecd8f5ba9a34af78442e4","cross_cats_sorted":["hep-ex","nucl-ex","physics.optics"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2013-08-12T21:00:54Z","title_canon_sha256":"2a1db9700055c51395740a09da2feeca5aa73070665f1da19f10995ce67f4440"},"schema_version":"1.0","source":{"id":"1308.2699","kind":"arxiv","version":1}},"source_aliases":[{"alias_kind":"arxiv","alias_value":"1308.2699","created_at":"2026-05-18T01:48:16Z"},{"alias_kind":"arxiv_version","alias_value":"1308.2699v1","created_at":"2026-05-18T01:48:16Z"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.1308.2699","created_at":"2026-05-18T01:48:16Z"},{"alias_kind":"pith_short_12","alias_value":"FVMCBTLOV62W","created_at":"2026-05-18T12:27:45Z"},{"alias_kind":"pith_short_16","alias_value":"FVMCBTLOV62WLSAL","created_at":"2026-05-18T12:27:45Z"},{"alias_kind":"pith_short_8","alias_value":"FVMCBTLO","created_at":"2026-05-18T12:27:45Z"}],"graph_snapshots":[{"event_id":"sha256:64027cc45203456bde087544156b2a175e1780659ab386d387e58546ec6407c2","target":"graph","created_at":"2026-05-18T01:48:16Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"graph_snapshot":{"author_claims":{"count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","strong_count":0},"builder_version":"pith-number-builder-2026-05-17-v1","claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"paper":{"abstract_excerpt":"Radiation detectors with noble gasses as the active medium are becoming increasingly common in experimental programs searching for physics beyond the standard model. Nearly all of these experiments rely to some degree on collecting scintillation light from noble gasses. The VUV wavelengths associated with noble gas scintillation mean that most of these experiments use a fluorescent material to shift the direct scintillation light into the visible or near UV band. We present an overview of the R&D program at LBL related to noble gas detectors for neutrino physics, double beta decay, and dark ma","authors_text":"V. M. Gehman","cross_cats":["hep-ex","nucl-ex","physics.optics"],"headline":"","license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2013-08-12T21:00:54Z","title":"WLS R\\&D for the Detection of Noble Gas Scintillation at LBL: seeing the light from neutrinos, to dark matter, to double beta decay"},"references":{"count":0,"internal_anchors":0,"resolved_work":0,"sample":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"1308.2699","kind":"arxiv","version":1},"verdict":{"created_at":null,"id":null,"model_set":{},"one_line_summary":"","pipeline_version":null,"pith_extraction_headline":"","strongest_claim":"","weakest_assumption":""}},"verdict_id":null}}],"author_attestations":[],"timestamp_anchors":[],"storage_attestations":[],"citation_signatures":[],"replication_records":[],"corrections":[],"mirror_hints":[],"record_created":{"event_id":"sha256:24f348a16acb36727d565b6a28c7a2d2e3db38a2643e319ea4eb87d3bfe0ac74","target":"record","created_at":"2026-05-18T01:48:16Z","signer":{"key_id":"pith-v1-2026-05","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","signer_id":"pith.science","signer_type":"pith_registry"},"payload":{"attestation_state":"computed","canonical_record":{"metadata":{"abstract_canon_sha256":"ed44ecc00434d834142dffafef23a18fa2b6c727571ecd8f5ba9a34af78442e4","cross_cats_sorted":["hep-ex","nucl-ex","physics.optics"],"license":"http://arxiv.org/licenses/nonexclusive-distrib/1.0/","primary_cat":"physics.ins-det","submitted_at":"2013-08-12T21:00:54Z","title_canon_sha256":"2a1db9700055c51395740a09da2feeca5aa73070665f1da19f10995ce67f4440"},"schema_version":"1.0","source":{"id":"1308.2699","kind":"arxiv","version":1}},"canonical_sha256":"2d5820cd6eafb565c80badef45abb9d4d65985860631ce75a4fe427f248ae351","receipt":{"algorithm":"ed25519","builder_version":"pith-number-builder-2026-05-17-v1","canonical_sha256":"2d5820cd6eafb565c80badef45abb9d4d65985860631ce75a4fe427f248ae351","first_computed_at":"2026-05-18T01:48:16.137209Z","key_id":"pith-v1-2026-05","kind":"pith_receipt","last_reissued_at":"2026-05-18T01:48:16.137209Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54","receipt_version":"0.3","signature_b64":"fjc1zG1L5VD8LPBhWKqvMOGzohAU+ZpbP2n3r6JL6KR82Inp12fuk3APD0pfJQMJgr4vd7Qrsi4+M2j5RbaiBw==","signature_status":"signed_v1","signed_at":"2026-05-18T01:48:16.137658Z","signed_message":"canonical_sha256_bytes"},"source_id":"1308.2699","source_kind":"arxiv","source_version":1}}},"equivocations":[],"invalid_events":[],"applied_event_ids":["sha256:24f348a16acb36727d565b6a28c7a2d2e3db38a2643e319ea4eb87d3bfe0ac74","sha256:64027cc45203456bde087544156b2a175e1780659ab386d387e58546ec6407c2"],"state_sha256":"9cddcdc239975eee5a650b1f9103e59cbd53e7b8c82b349b6551dcd879ae1702"}