/ Astrophysics


EURECA – The Future of Cryogenic Dark Matter Detection in Europe


Kraus, H. (Oxford U.) ; Armengaud, E. (IRFU, Saclay) ; Bauer, M. (Tubingen U.) ; Bavykina, I. (Munich, Max Planck Inst.) ; Benoit, A. (Neel Lab, Grenoble) ; Bento, A. (Munich, Max Planck Inst.) ; Blümer, J. (Karlsruhe, Forschungszentrum) ; Bornschein, L. (Karlsruhe U., EKP) ; Broniatowski, A. (CSNSM, Orsay) ; Burghart, G. (CERN) ; Camus, P. (Neel Lab, Grenoble) ; Chantelauze, A. (Karlsruhe, Forschungszentrum) ; Chapellier, M. (IRFU, Saclay) ; Chardin, G. (CSNSM, Orsay) ; Ciemniak, C. (Munich, Tech. U.) ; Coppi, C. (Munich, Tech. U.) ; Coron, N. (Orsay, IAS) ; Crauste, O. (CSNSM, Orsay) ; Danevich, F.A. (Kiev, INR) ; Jésus, M. De (Lyon, IPN) ; Marcillac, P. de (Orsay, IAS) ; Daw, E. (Sheffield U.) ; Defay, X. (CSNSM, Orsay) ; Deuter, G. (Tubingen U.) ; Domange, J. (IRFU, Saclay) ; Stefano, P. Di (Lyon, IPN) ; Drexlin, G. (Karlsruhe U., EKP) ; Dumoulin, L. (CSNSM, Orsay) ; Eitel, K. (Karlsruhe, Forschungszentrum) ; Feilitzsch, F. von (Munich, Tech. U.) ; Filosofov, D. (Dubna, JINR) ; Gandit, P. (Neel Lab, Grenoble) ; Garcia, E. (Zaragoza U.) ; Gascon, J. (Lyon, IPN) ; Gerbier, G. (IRFU, Saclay) ; Gironnet, J. (Orsay, IAS) ; Godfrin, H. (Neel Lab, Grenoble) ; Grohmann, S. (Karlsruhe, Forschungszentrum) ; Gros, M. (IRFU, Saclay) ; Hannewald, M. (IRFU, Saclay) ; Hauff, D. (Munich, Max Planck Inst.) ; Haug, F. (CERN) ; Henry, S. (Oxford U.) ; Huff, P. (Munich, Max Planck Inst.) ; Imber, J. (Oxford U.) ; Ingleby, S. (Oxford U.) ; Isaila, C. (Munich, Tech. U.) ; Jochum, J. (Tubingen U.) ; Juillard, A. (CSNSM, Orsay) ; Kiefer, M. (Munich, Max Planck Inst.) ; Kimmerle, M. (Tubingen U.) ; Kluck, H. (Karlsruhe, Forschungszentrum) ; Kobychev, V.V. (Kiev, INR) ; Kozlov, V. (Karlsruhe, Forschungszentrum) ; Kudovbenko, V.M. (Kiev, INR) ; Kudryavtsev, V.A. (Sheffield U.) ; Lachenmaier, T. (Munich, Tech. U.) ; Lanfranchi, J.C. (Munich, Tech. U.) ; Lang, R.F. (Munich, Max Planck Inst.) ; Loaiza, P. (Modane, Lab. Souterrain) ; Lubashevsky, A. (Dubna, JINR) ; Malek, M. (Oxford U.) ; Marnieros, S. (CSNSM, Orsay) ; McGowan, R. (Oxford U.) ; Mikhailik, V. (Oxford U.) ; Monfardini, A. (Neel Lab, Grenoble) ; Navick, X.F. (IRFU, Saclay) ; Niinikoski, T. (CERN) ; Nikolaiko, A.S. (Kiev, INR) ; Oberauer, L. (Munich, Tech. U.) ; Olivieri, E. (CSNSM, Orsay) ; Ortigoza, Y. (Zaragoza U.) ; Pantic, E. (Munich, Max Planck Inst.) ; Pari, P. (IRFU, Saclay) ; Paul, B. (IRFU, Saclay) ; Perinic, G. (CERN) ; Petricca, F. (Munich, Max Planck Inst.) ; Pfister, S. (Munich, Tech. U.) ; Pobes, C. (Zaragoza U.) ; Poda, D.V. (Kiev, INR) ; Podviyanuk, R.B. (Kiev, INR) ; Polischuk, O.G. (Kiev, INR) ; Potzel, W. (Munich, Tech. U.) ; Pröbst, F. (Munich, Max Planck Inst.) ; Puimedon, J. (Zaragoza U.) ; Robinson, M. (Sheffield U.) ; Roth, S. (Munich, Tech. U.) ; Rottler, K. (Tubingen U.) ; Rozov, S. (Dubna, JINR) ; Sailer, C. (Tubingen U.) ; Salinas, A. (Zaragoza U.) ; Sanglard, V. (Lyon, IPN) ; Sarsa, M.L. (Zaragoza U.) ; Schäffner, K. (Munich, Max Planck Inst.) ; Scholl, S. (Tubingen U.) ; Scorza, S. (Lyon, IPN) ; Smolnikov, A. (Dubna, JINR) ; Seidel, W. (Munich, Max Planck Inst.) ; Semikh, S. (Dubna, JINR) ; Stern, M. (Lyon, IPN) ; Stodolsky, L. (Munich, Max Planck Inst.) ; Teshima, M. (Munich, Max Planck Inst.) ; Tomasello, V. (Sheffield U.) ; Torrento, A. (CERN) ; Torres, L. (Zaragoza U.) ; Tretyak, V.I. (Kiev, INR) ; Villar, J.A. (Zaragoza U.) ; Verdier, M.A. (Lyon, IPN) ; Usherov, I. (Tubingen U.) ; Wolf, J. (Karlsruhe U., EKP) ; Yakushev, E. (Dubna, JINR)

Published in: EAS Publ.Ser.
Year: 2009
Vol.: 36
Page No: 249-255
Pages: 7
Year: 2009-05-30 published

Abstract: EURECA (European Underground Rare Event Calorimeter Array) is anastro-particle physics facility aiming to directly detect galactic darkmatter. The Laboratoire Souterrain de Modane has been selected as hostlaboratory. The EURECA collaboration unites CRESST, EDELWEISS and theSpanish-French experiment ROSEBUD, thus concentrating and focussing efforton cryogenic detector research in Europe into a single facility. EURECA willuse a target mass of up to one ton, enough to explore WIMP - nucleon scalarscattering cross sections in the region of 10^-9 - 10^-10 picobarn.A major advantage of EURECA is the planned use of more than just one targetmaterial (multi target experiment for WIMP identification).

Total numbers of views: 652
Numbers of unique views: 346
DOI: 10.1051/eas/0936035
 Record created 2015-03-03, last modified 2015-03-03



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