The EDELWEISS Dark Matter search uses low-temperature Ge detectors with heat and ionisation read-out to identify nuclear recoils induced by elastic collisions with WIMPS from the galactic halo. Results from the operation of 70 g and 320 g Ge detectors in the low-background environment of the Modane Underground Laboratory (LSM) are presented.
The EDELWEISS experiment: Status and outlook / A. Benoit, A. Bonnevaux, L. Berge, A. Broniatowski, B. Chambon, M. Chapellier, G. Chardin, P. Charvin, P. Cluzel, M. De Jesus, P. Di Stefano, D. Drain, L. Dumoulin, J. Gascon, G. Gerbier, C. Goldbach, M. Goyot, M. Gros, J.P. Hadjout, S. Herve, A. Juillard, A. de Lesquen, M. Loidl, J. Mallet, S. Marnieros, O. Martineau, N. Mirabolfathi, L. Miramonti, L. Mosca, X.F. Navick, G. Nollez, P. Pari, C. Pastor, E. Simon, M. Stern, L. Vagneron, L. Miramonti. ((Intervento presentato al convegno 3rd International Conference on Dark Matter in Astro- and Particle Physics (DARK 2000) tenutosi a HEIDELBERG nel 2000.
The EDELWEISS experiment: Status and outlook
L. Miramonti;
2001
Abstract
The EDELWEISS Dark Matter search uses low-temperature Ge detectors with heat and ionisation read-out to identify nuclear recoils induced by elastic collisions with WIMPS from the galactic halo. Results from the operation of 70 g and 320 g Ge detectors in the low-background environment of the Modane Underground Laboratory (LSM) are presented.
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