Current status of the ANITA experiment

Annual Meeting of the Division of Particles and Fields of the American Physical Society, DPF 2006, and the Annual Fall Meeting of the Japan Particle Physics Community (2006)

Authors:

S Matsuno, J Clem, D Seckel, S Barwick, D Goldstein, K Kuehn, J Nam, A Connolly, D Saltsberg, D Williams, P Gorham, C Hebert, J Learned, J Kowalski, S Matsuno, R Milincic, P Miocinovic, M Rosen, A Romero-Wolf, G Verner, K Liewer, C Naudet, F Wu, D Besson, M DuVernois, E Lusczek, D Gregory, J Link, J Beatty, B Mercurino, R Nichol, K Palladino, P Chen, C Field, C Hast, J Ng, K Reil, R Binns, P Dowkontt, M Isreal, M Olevitch

Abstract:

• ANITA project has been progressing in amazing pace • instrument is well tested, understood, and calibrated with SLAC electron beam • ANITA is now ready to detect UHE neutrinos - collaborators heading for Antarctica - two calibration radio sources scheduled to be set up. • a nominal 15 days flight should cut into expected GZK flux • hope to have a longer flight (like 42 days CREAM '0405 flight) and a positive detection of GZK neutrinos.

Development of multiple photon counting coincidence (MPCC) technique for characterisation of scintillators for cryogenic applications

Astroparticle, Particle and Space Physics, Detectors and Medical Physics Applications - Proceedings of the 9th Conference (2006) 277-281

Authors:

H Kraus, V Mikhailik, D Wahl

Abstract:

A new method for measurements of the scintillation characteristics of materials has been developed. This method, called multiple photon counting coincidence (MPCC) technique, is based on the recording of a sequence of individual photon pulses resulting from a scintillation event. The distribution of the arrival times of these individual photon pulses provides information about the decay characteristic of the scintillation process and the number of photons recorded per scintillation event is proportional to the scintillation light yield. The ability to reject spurious events through off-line analysis is an important advantage of the MPCC method since it allows cleaning of the data set from pile-up events. It is shown that the MPCC technique is particularly well suited for the analysis of slow scintillation processes in the investigation of temperature-dependant scintillator properties. It is now used extensively by our group for the identification and optimisation of scintillating targets for cryogenic low-background rare event searches, such as Dark Matter and 0-v double beta decay experiments.

EURECA -- the European future of cryogenic dark matter searches

J PHYS CONF SER 39 (2006) 139-141

Authors:

H Kraus, M Bauer, A Benoit, J Blumer, A Broniatowski, P Camus, A Chantelauze, M Chapellier, G Chardin, P Christ, C Coppi, M De Jesus, A De Lesquen, H Deschamps, P Di Stefano, L Dumoulin, K Eitel, F von Feilitzsch, M Fesquet, J Gascon, G Gerbier, C Goldbach, M Gros, D Hauff, S Henry, M Horn, C Isaila, M Kimmerle, J Jochum, A Juillard, R Lemrani, M Luca, S Marnieros, R McGowan, V Mikhailik, XF Navick, T Niinikoski, G Nollez, E Pantic, P Pari, F Petricca, W Potzel, F Probst, W Rau, F Ritter, K Rottler, S Scholl, W Seidel, V Sanglard, M Stern, F Schwamm, M Teshima, B Tolhurst, W Westphal, P Wikus, J Wolf

Abstract:

EURECA (European Underground Rare Event Calorimeter Array) is a new project, searching for dark matter, with largely the present groups of the CRESST and EDELWEISS experiments and already a few new groups. The aim is to explore scalar cross sections in the 10(-9) - 10(-10) pico-barn region with a target mass of up to one tonne. A major advantage of EURECA is our planned use of more that just one target material (multi target experiment for WIMP identification). In preparation for this large-scale experiment, R&D for EURECA is provided through the current phases of CRESST and EDELWEISS.

Radiative decay of self-trapped excitons in CaMoO4 and MgMoO4 crystals

Journal of Physics Condensed Matter 17:46 (2005) 7209-7218

Authors:

VB Mikhailik, H Kraus, M Itoh, D Iri, M Uchida

Abstract:

Spectroscopic properties of CaMoO4 and MgMoO4 crystals were studied in view of their application to cryogenic scintillation detectors. Luminescence spectra and the luminescence decay kinetics were measured over a wide range of temperatures (8-300 K). For the first time we measured time-resolved luminescence spectra of CaMoO4. In addition to the green emission arising from the triplet state of self-trapped excitons (STEs), a new band at around 430 nm with a decay time constant 10 ± 3 ns was observed at T ≤ 8 K. This emission is assigned to the radiative decay of a singlet STE. The relaxation of electronic excitations in the crystals under study is discussed on the basis of our current understanding of their electronic structures and a configuration coordinate model for the radiative decay of STEs. The model includes adiabatic potential energy surfaces (APESs) associated with singlet and triplet states and explains the variation of the luminescence kinetics with temperature as a result of a re-distribution in the population of these states. Thus, judging from the change of the singlet STE emission due to temperature variation, we infer the existence of an energy barrier between the singlet and triplet APESs. The multi-exponential character of the decay of the triplet emission can be understood assuming that the relevant radiative transitions originate from different minima of the triplet APES. Non-radiative energy transfer processes control the population of these states, resulting in thermal variation of the intensities of the different emission components. © 2005 IOP Publishing Ltd.

Characterization of CaWO4 scintillator at room and liquid nitrogen temperatures

Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 553:3 (2005) 578-591

Authors:

M Moszyński, M Balcerzyk, W Czarnacki, A Nassalski, T Szczȩśniak, H Kraus, VB Mikhailik, IM Solskii

Abstract:

The properties of CaWO4 (CaWO) crystals in γ-spectrometry were studied at room and liquid nitrogen(LN2) temperatures. Two small samples of 10×10×4 mm3 and 10×10×8 mm 3 size were tested, coupled to a Photonis XP3212 photomultiplier at room temperature and a large area avalanche photodiode at LN2 temperature. Light pulse shape and light output at room and LN2 temperatures were measured. Energy resolution and non-proportionality of the CaWO response versus γ-ray energy were studied and compared with those of small BGO and CdWO4 crystals to discuss further the origin of the intrinsic resolution of undoped scintillating crystals. A high light output of 4800±200 phe/MeV and a good energy resolution of 6.6±0.2% for 662 keV γ-rays from a 137Cs source were measured for the small samples coupled to the XP3212 photomultiplier. © 2005 Elsevier B.V. All rights reserved.