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Insertion of STC into TRT at the Department of Physics, Oxford
Credit: CERN

Hans Kraus

Professor of Physics

Research theme

  • Particle astrophysics & cosmology

Sub department

  • Particle Physics

Research groups

  • LUX-ZEPLIN
Hans.Kraus@physics.ox.ac.uk
Telephone: 01865 (2)73361
Denys Wilkinson Building, room 623
  • About
  • Publications

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 Pr枚bst, K Sch盲ffner, 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 Bl眉mer, 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 J茅sus, 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).

The cresst dark matter search

Proceedings of the 6th International Workshop on the Identification of Dark Matter, IDM 2006 (2007) 192-197

Authors:

I Bawkina, A Bento, D Hauff, P Huff, R Lang, B Majorovits, E Pantic, F Petricca, F Prbst, W Seidel, L Stodolsky, S Henry, J Imber, S Ingleby, H Kraus, M Malek, R McGowan, V Mikhailik, B Tolhurst, C Ciemniak, C Coppi, F Von Feilitzsch, C Isaila, J Lanfranchi, S Pfister, W Potzel, W Westphal, M Bauer, J Jochum, M Kimmerle, K Rottler, S Scholl, C Bucci

Abstract:

CRESST I1 is a WIMP search experiment using cryogenic detectors to detect heat and scintillation signals in Caw04 crystals simultaneously. Competitive limits on the coherent WIMP-nucleon scattering cross section and other results from runs from the upgrade to CRESST I1 are shown. New features and upgrades installed on the CRESST I1 setup are described and the status of the experiment is presented.

CRESST - status and future

NUCL PHYS B-PROC SUP 173 (2007) 104-107

Authors:

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

Abstract:

We present results on WIMP dark matter interaction, obtained using cryogenic phonon-scintillation detectors. The targets are CaWO4 scintillating crystals with phonon sensors, while scintillation is detected with an associated cryogenic light detector. The combination of phonon and light signals leads to a strong suppression of nonnuclear recoil backgrounds. Results obtained before the upgrade of CRESST are presented and a status report on the upgrade itself is given.

EURECA - the European future of dark matter searches with cryogenic detectors

NUCL PHYS B-PROC SUP 173 (2007) 168-171

Authors:

H Kraus, M Bauer, I Bavykina, A Benoit, J Blumer, A Broniatowski, V Brudanin, G Burghart, P Camus, A Chantelauze, M Chapellier, G Chardin, P Christ, C Ciemniak, 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, J Imber, C Isaila, J Jochum, A Juillard, M Kimmerle, JC Lanfranchi, R Lemrani, A Lubashevsky, M Luca, M Malek, S Marnieros, R McGowan, V Mikhailik, XF Navick, T Niinikoski, G Nollez, E Pantic, P Pari, L Perevoshchikov, F Petricca, S Pfister, W Potzel, F Probst, W Rau, F Ritter, K Rottler, V Sanglard, S Scholl, F Schwamm, W Seidel, A Smolnikov, M Stern, M Teshima, B Tolhurst, W Westphal, P Wikus, J Wolf, E Yakushev

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) picobarn 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.

Temperature dependence of CaMoO4 scintillation properties

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment (2007)

Authors:

SA Henry, V B Mikhailik, H Kraus, I Solskii

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