First test of a cryogenic scintillation module with a CaWO4 scintillator and a low-temperature photomultiplier down to 6 K

Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 621:1-3 (2010) 395-400

Authors:

H Kraus, VB Mikhailik

Abstract:

Future cryogenic experiments searching for rare events require reliable, efficient and robust techniques for the detection of photons at temperatures well below that to which low-temperature photomultipliers (PMT) were characterised. Motivated by this, we investigated the feasibility of a low-temperature PMT for the detection of scintillation from crystalline scintillators at T=6 K. The scintillation module was composed of a CaWO 4 scintillator and a low-temperature PMT D745B from ET Enterprises. The PMT responsivity was studied at T=290, 77 and 6 K using γ-quanta from 241Am (60 keV) and 57Co (122 and 136 keV) sources. We have shown that the low-temperature PMT retains its single photon counting ability even at cryogenic temperatures. At T=6 K, the response of the PMT decreases to 51±13% and 27±6%, when assessed in photon counting and pulse height mode, respectively. Due to the light yield increase of the CaWO 4 scintillating crystal, the overall responsivity of the scintillation modules CaWO4PMT is 94±15% (photon counting) and 48±8% (pulse height) when cooling to T=6 K. The dark count rate was found to be 20 s-1. The energy resolution of the module remains similar to that measured at room temperature using either of the detection modes. It is concluded that commercially available low-temperature PMT are well suited for detection of scintillation light at cryogenic temperatures. © 2010 Elsevier B.V. All rights reserved.

Observation of Ultra-high-energy Cosmic Rays with the ANITA Balloon-borne Radio Interferometer

(2010)

Authors:

S Hoover, J Nam, PW Gorham, E Grashorn, P Allison, SW Barwick, JJ Beatty, K Belov, DZ Besson, WR Binns, C Chen, P Chen, JM Clem, A Connolly, PF Dowkontt, MA DuVernois, RC Field, D Goldstein, AG Vieregg, C Hast, CL Hebert, MH Israel, A Javaid, J Kowalski, JG Learned, KM Liewer, JT Link, E Lusczek, S Matsuno, BC Mercurio, C Miki, P Miočinović, CJ Naudet, J Ng, RJ Nichol, K Palladino, K Reil, A Romero-Wolf, M Rosen, L Ruckman, D Saltzberg, D Seckel, GS Varner, D Walz, F Wu

Direct dark matter search with CRESST and EURECA

Progress in Particle and Nuclear Physics 64:2 (2010) 457-459

Authors:

S Roth, G Angloher, M Bauer, I Bavykina, A Bento, A Brown, C Bucci, C Ciemniak, C Coppi, G Deuter, A Erb, FV Feilitzsch, A Gütlein, D Hauff, S Henry, M Hofmann, P Huff, J Imber, S Ingelby, C Isaila, J Jochum, M Kiefer, M Kimmerle, H Kraus, T Lachenmaier, JC Lanfranchi, RF Lang, B Majorovits, M Malek, R McGowan, V Mikhailik, E Pantic, F Petricca, S Pfister, W Potzel, F Pröbst, K Rottler, C Sailer, K Schäffner, J Schmaler, S Scholl, W Seidel, MV Sivers, L Stodolsky, R Strauss, AJB Tolhurst, I Usherov, W Westphal

Abstract:

The current status of the direct Dark Matter experiments CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) and the planned EURECA (European Underground Rare Event Calorimeter Array) is presented. Both experiments are aimed at the direct detection of WIMPs (Weakly Interacting Massive Particles), potential candidates for the Dark Matter in the universe. New design developments of the cryogenic detectors operated at mK temperatures are investigated to optimize detector performance and to simplify mass production. Thus, CRESST is also providing a basis for the EURECA project, aimed at a ton of cryogenic detectors with a multi-material target. © 2010 Elsevier B.V. All rights reserved.

Observational Constraints on the Ultra-high Energy Cosmic Neutrino Flux from the Second Flight of the ANITA Experiment

(2010)

Authors:

The ANITA Collaboration, PW Gorham, P Allison, BM Baughman, JJ Beatty, K Belov, DZ Besson, S Bevan, WR Binns, C Chen, P Chen, JM Clem, A Connolly, M Detrixhe, D De Marco, PF Dowkontt, M DuVernois, EW Grashorn, B Hill, S Hoover, M Huang, MH Israel, A Javaid, KM Liewer, S Matsuno, BC Mercurio, C Miki, M Mottram, J Nam, RJ Nichol, K Palladino, A Romero-Wolf, L Ruckman, D Saltzberg, D Seckel, GS Varner, AG Vieregg, Y Wang

First test of a cryogenic scintillation module with a CaWO4 scintillator and a low-temperature photomultiplier down to 6 K

(2010)

Authors:

H Kraus, VB Mikhailik