Scintillation properties of pure CaF2

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 566:2 (2006) 522-525

Authors:

VB Mikhailik, H Kraus, J Imber, D Wahl

Abstract:

The temperature dependence of the decay time and scintillation light yield of pure CaF2 crystal was measured over the temperature range 8-305 K using the multiphoton coincidence counting technique. Pure CaF2 exhibits emission of triplet self-trapped excitons at 280 nm with a slow decay, the time constant of which changes significantly with temperature. The main decay time constant increases by three orders of magnitude when cooled, from 0.96±0.06 μs at 295 K to 930±40 μs at 8 K. The results obtained demonstrate that the scintillation light yield of pure CaF2 increases with decreasing temperature down to 20 K below which it is roughly constant. At low temperatures the light yield of CaF2 is estimated to be 60% relative to that of pure CaWO4. It is concluded that undoped calcium fluoride is a very attractive target material for experimental searches for rare events based on the detection of phonon and scintillation signals. © 2006 Elsevier B.V. All rights reserved.

Fracture processes observed with a cryogenic detector

Physics Letters Section A General Atomic and Solid State Physics 356:4-5 (2006) 262-266

Authors:

J Åström, PCF Di Stefano, F Pröbst, L Stodolsky, J Timonen, C Bucci, S Cooper, C Cozzini, FV Feilitzsch, H Kraus, J Marchese, O Meier, U Nagel, Y Ramachers, W Seidel, M Sisti, S Uchaikin, L Zerle

Abstract:

In the early stages of running of the CRESST dark matter search using sapphire detectors at very low temperature, an unexpectedly high rate of signal pulses appeared. Their origin was finally traced to fracture events in the sapphire due to the very tight clamping of the detectors. During extensive runs the energy and time of each event was recorded, providing large data sets for such phenomena. We believe this is the first time the energy release in fracture has been directly and accurately measured on a microscopic event-by-event basis. The energy threshold corresponds to the breaking of only a few hundred covalent bonds, a sensitivity some orders of magnitude greater than that of previous technique. We report some features of the data, including energy distributions, waiting time distributions, autocorrelations and the Hurst exponent. The energy distribution appear to follow a power law, d N / d E ∝ E- β, similar to the power law for earthquake magnitudes, and after appropriate translation, with a similar exponent. In the time domain, the waiting time w or gap distribution between events has a power law behavior at small w and an exponential fall-off at large w, and can be fit ∝ w- α e -w / w0. The autocorrelation function shows time correlations lasting for substantial parts of an hour. An asymmetry is found around large events, with higher count rates after, as opposed to before, the large event. © 2006 Elsevier B.V. All rights reserved.

Optical and luminescence studies of ZnMoO4 using vacuum ultraviolet synchrotron radiation

Nuclear Instruments and Methods in Physics Research Section A Accelerators Spectrometers Detectors and Associated Equipment 562:1 (2006) 513-516

Authors:

VB Mikhailik, H Kraus, D Wahl, H Ehrenberg, MS Mykhaylyk

Abstract:

In this paper we present a characterisation of ZnMoO4 using spectroscopic techniques. Reflection, luminescence and luminescence excitation spectra were measured over the temperature range 8-295 K using VUV synchrotron radiation. The emission spectrum of the crystal exhibits a broad band with a maximum around 1.95 eV at 80 K that is attributed to the radiative transitions within MO42- oxyanion complex. An interpretation of the observed features of the electronic excitations in the crystal is given based on present knowledge of the electronic structure and emission properties of molybdate crystals. The results of this study suggest that ZnMoO4 is a suitable candidate for further testing for implementation as a target material in cryogenic scintillation searches for rare events. © 2006 Elsevier B.V. All rights reserved.

Constraints on Cosmic Neutrino Fluxes from the Antarctic Impulsive Transient Antenna Experiment

Physical Review Letters American Physical Society (APS) 96:17 (2006) 171101

Authors:

SW Barwick, JJ Beatty, DZ Besson, WR Binns, B Cai, JM Clem, A Connolly, DF Cowen, PF Dowkontt, MA DuVernois, PA Evenson, D Goldstein, PW Gorham, CL Hebert, MH Israel, JG Learned, KM Liewer, JT Link, S Matsuno, P Miočinović, J Nam, CJ Naudet, R Nichol, K Palladino, M Rosen, D Saltzberg, D Seckel, A Silvestri, BT Stokes, GS Varner, F Wu

Dark-matter search with CRESST

CZECH J PHYS 56:5 (2006) 535-542

Authors:

W Westphal, C Coppi, F von Feilitzsch, C Isaila, J Konig, W Potzel, W Rau, M Razeti, M Stark, H Wulandari, G Angloher, I Bavykina, P Christ, D Hauff, J Ninkovic, E Pantic, F Petricca, F Probst, W Seidel, L Stodolsky, M Bauer, T Jagemann, J JocHum, K Rottler, S Scholl, C Bucci, C Cozzini, S Henry, H Kraus, B Majorovits, R McGowan, V Mikhailik, AJB Tolhurst, Y Ramachers

Abstract:

The CRESST experiment is looking for non-baryonic particle dark matter via nuclear scattering in CaWO4. The simultaneous measurement of the heat and the scintillation light generated by an event in a CaWO4 single crystal is used to discriminate between electron and nuclear recoils thanks to their different light output. This allows an efficient suppression of the electron recoil background. The set-up consists of modules with a 300 g CaWO4 crystal mounted in a reflective housing together with a light detector. The heat signal is read out using a superconducting transition-edge sensor (TES) made of tungsten evaporated directly onto the crystal that is operated at a few mK. Currently the second phase of the experiment is being set up at the Laboratori Nazionali del Gran Sasso in which it is planned to run 33 detector modules providing a total target mass of 10 kg. First test runs with prototype detectors have been successfully performed.