DM - LArTPC DocDB - Fermilab

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Introduction Neutrino & Dark Matter Synergies Technical Issues for Multi-ton Argon Neutrino detector: • Chemical purity to allow electron drift (10’s ppt O2 equivalent), • Chemical purity to allow light production and propagation • Cryostat and Cryogenics and associated safety issues • TPC design • TPC readout electronics • HV feedthroughs (>100 kV) and distribution • Light Detection • Data Acquisition • Detector Materials Qualification 6 Fermilab Institutional Review, June 6-9, 2011
Introduction Neutrino & Dark Matter Synergies Technical Issues for Neutrino or DM Argon detector: • Chemical purity to allow electron drift (10’s ppt O2), (ν and DM) • Chemical purity to allow light production and propagation (ν and DM) • Cryostat and Cryogenics and associated safety issues (ν and DM) • TPC design (ν and DM) • TPC readout electronics (ν) • HV feedthroughs (>100 kV) and distribution (ν and DM) • Light Detection (ν and DM) • Data Acquisition (ν and DM) • Detector Materials Qualification (ν and DM) • Shielding from environment radiation (DM) • Radio-purity of detector materials (DM) • Radio purity of Argon (DM) 7 Fermilab Institutional Review, June 6-9, 2011
Page 1 and 2: Work on Liquid Argon at Fermilab St
Page 3 and 4: Introduction Liquid Argon - Why Liq
Page 5: Introduction - Some Context (2) Ins
Page 9 and 10: Facilities - Schematic of Materials
Page 11 and 12: Measurement Features of Material
Page 13 and 14: Materials Test Stand Typical data S
Page 15 and 16: LAr TPC Electronics Test Stand MSU
Page 17 and 18: Example of use of TPC data - for el
Page 19 and 20: 1 st in-liquid CMOS electronics on
Page 21 and 22: ArgoNeuT-T962: LArTPC exposed to Nu
Page 23 and 24: Achieving good lifetime in an uneva
Page 25 and 26: Some steps on the path to the LBNE
Page 27 and 28: First steps with the Membrane Techn
Page 29 and 30: Light Readout R & D (M.I.T & Indian
Page 31 and 32: Distillation Column Design and Real
Page 33 and 34: One Slide on Software It is recogni
Page 35 and 36: Conclusions Vigorous and broad rang
Page 37 and 38: Introduction Neutrino & Dark Matter

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