EURECA - The future of cryogenic dark matter detection in Europe

Proceedings of Science (2008)

Authors:

H Kraus, E Armengaud, M Bauer, I Bavykina, A Benoit, A Bento, J Blümer, L Bornschein, A Broniatowski, G Burghart, P Camus, A Chantelauze, M Chapellier, G Chardin, C Ciemniak, C Coppi, N Coron, O Crauste, FA Danevich, M De Jésus, P Marcillac, E Daw, X Defay, G Deuter, J Domange, P Di Stefano, G Drexlin, L Dumoulin, K Eitel, F Von Feilitzsch, D Filosofov, P Gandit, E Garcia, J Gascon, G Gerbier, J Gironnet, H Godfrin, S Grohmann, M Gros, M Hannewald, D Hauff, F Haug, S Henry, P Huff, J Imber, S Ingleby, C Isaila, J Jochum, A Juillard, M Kiefer, M Kimmerle, H Kluck, VV Kobychev, V Kozlov, VA Kudryavtsev, T Lachenmaier, JC Lanfranchi, RF Lang, P Loaiza, A Lubashevsky, M Malek, S Marnieros, R McGowan, V Mikhailik, VM Mokina, A Monfardini, XF Navick, T Niinikoski, AS Nikolaiko, L Oberauer, E Olivieri, Y Ortigoza, E Pantic, P Pari, B Paul, G Perinic, F Petricca, S Pfister, C Pobes, DV Poda, RB Podviyanuk, OG Polischuk, W Potzel, F Pröbst, J Puimedon, M Robinson, S Roth, K Rottler, S Rozov, C Sailer, A Salinas, V Sanglard, ML Sarsa, K Schäffner, S Scholl, S Scorza, A Smolnikov, W Seidel, S Semikh, M Stern

Abstract:

European Underground Rare Event Calorimeter Array (EURECA) will be an astro-particle physics facility in the Laboratoire Souterrain de Modane, aiming to directly detect galactic dark matter. The EURECA collaboration unites CRESST, EDELWEISS and the Spanish-French experiment ROSEBUD, thus concentrating and focussing effort on cryogenic detector research in Europe into a single facility. The aim is to explore WIMP - nucleon scalar cross sections in the 10-9 - 10-10 picobarn region with a target mass of up to one ton. A major advantage of EURECA is the planned use of more than just one target material (multi target experiment for WIMP identification).

Results of the CRESST commissioning run 2007

Proceedings of the 4th Patras Workshop on Axions, WIMPs and WISPs, PATRAS 2008 (2008) 95-98

Authors:

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

Abstract:

CRESST (Cryogenic Rare Event Search with Superconducting Thermometers) is a low temperature experiment dedicated to the direct dark matter detection via nuclear recoil. It is located in Hall A of the Laboratori Nazionali del Gran Sasso, Italy. Scintillating CaWO4 crystals operated at a few mK are utilized as target forWIMPs (Weakly Interacting Massive Particles), which are expected to scatter predominantly on the heavy tungsten nuclei. As for background rejection, CRESST uses the phonon-light technique, where two different quantities of an interaction are recorded: the heat production in the CaWO4crystal and the simultaneous emission of scintillation light, which is monitored by a second low-temperature detector, the light detector. The information provided by both detectors allows a powerful background discrimination on an event by event basis. After a major upgrade phase, CRESST-II has now successfully completed a commissioning run during 2007, the results of which are presented in this article.

Scintillation properties of pure and ca-doped ZnWO4 crystals

Physica Status Solidi (A) Applications and Materials Science 205:2 (2008) 335-339

Authors:

FA Danevich, S Henry, H Kraus, R McGowan, VB Mikhailik, OG Shkulkova, J Telfer

Abstract:

Following the investigations of the structure and scintillation properties of Ca-doped zinc tungstate powder [phys. stat. sol. (a) 204. 730 (2007)] a single-crystal of ZnWO4-Ca (0.5 mol%) was grown and characterised. The relative light output, energy resolution and decay characteristics were measured for pure and Ca-doped ZnWO4 scintillators. An increase in the light yield of ~40% compared with the undoped crystal, and an energy resolution 9.6% (137Cs) were obtained for Ca-doped ZnWO4. The observed improvement is attributed to the reduction of self-absorption (bleaching) of the crystal. The cause of bleaching as well as the possible contribution of scattering is discussed. © 2008 WILEY-VCH Verlag GmbH & Co. KGaA.

EURECA - The future of cryogenic dark matter detection in Europe

Proceedings of Science (2008)

Authors:

H Kraus, S Henry, J Imber, S Ingleby, M Malek, R McGowan, V Mikhailik, I Bavykina, A Bento, D Hauff, P Huff, M Kiefer, RF Lang, E Pantic, F Petricca, F Pröbst, K Schäffner, W Seidel, L Stodolsky, M Teshima, C Ciemniak, C Coppi, F Von Feilitzsch, C Isaila, T Lachenmaier, J-C Lanfranchi, L Oberauer, S Pfister, W Potzel, S Roth, M Bauer, G Deuter, J Jochum, M Kimmerle, K Rottler, C Sailer, S Scholl, I Usherov, J Blümer, L Bornschein, G Drexlin, J Wolf, A Chantelauze, K Eitel, S Grohmann, H Kluck, V Kozlov, E Armengaud, J Domange, G Gerbier, M Gros, M Hannewald, X-F Navick, B Paul, M Chapellier, P Pari, G Burghart, F Haug, T Niinikoski, G Perinic, A Torrento, A Broniatowski, G Chardin, O Crauste, X Defay, L Dumoulin, A Juillard, S Marnieros, E Olivieri, M De Jésus, P Di Stefano, J Gascon, V Sanglard, S Scorza, M Stern, MA Verdier, P Camus, N Coron, P Marcillac, J Gironnet, A Benoit, P Gandit, H Godfrin, A Monfardini, D Filosofov, A Lubashevsky, C Pobes, S Rozov, A Smolnikov, S Semikh, E Yakushev, E Garcia, Y Ortigoza, J Puimedon, A Salinas, ML Sarsa, L Torres, JA Villar, E Daw, VA Kudryavtsev, M Robinson, V Tomasello, FA Danevich, VV Kobychev, VM Mokina, AS Nikolaiko, DV Poda, RB Podviyanuk, OG Polischuk, VI Tretyak, P Loaiza

Abstract:

European Underground Rare Event Calorimeter Array (EURECA) will be an astro-particle physics facility in the Laboratoire Souterrain de Modane, aiming to directly detect galactic dark matter. The EURECA collaboration unites CRESST, EDELWEISS and the Spanish-French experiment ROSEBUD, thus concentrating and focussing effort on cryogenic detector research in Europe into a single facility. The aim is to explore WIMP - nucleon scalar cross sections in the 10 - 10 picobarn region with a target mass of up to one ton. A major advantage of EURECA is the planned use of more than just one target material (multi target experiment for WIMP identification).

Temperature dependence of CaMoO4 scintillation properties

583:2-3 (2007) 350-355

Authors:

VB Mikhallik, S Henry, H Kraus, I Solskii

Abstract:

The perspective of using CaMoO4 as a scintillation target in cryogenic rare event searches has provided strong motivation for the optimisation of this material. A single crystal of CaMoO4, exhibiting high optical quality, was produced and its scintillation light response to particle excitation and its decay time constant were investigated over the 7-300K temperature range. The scintillation at room temperature is strongly affected by thermal quenching. The main decay time constant is found to be 15.7 +/- 0.4 mu s at T= 300K; cooling to 7K increases the scintillation decay time constant to 380 +/- 20 mu s. The scintillation efficiency of the CaMoO4 crystal was evaluated by comparison with a reference CaWO4 crystal measured under the same conditions; we estimate the light output of CaMoO4 to be 55 +/- 20% that of CaWO4 at 294K and 95 +/- 30% at 7K. The study confirmed that calcium molybdate optimised for high light yield is a very attractive material for use in cryogenic phonon-scintillation detectors in rare event searches. (c) 2007 Elsevier B.V. All rights reserved.