Final results of the EDELWEISS-I dark matter search with cryogenic heat-and-ionization Ge detectors
| dc.creator | Sanglard, V. | |
| dc.creator | Benoit, A. | |
| dc.creator | Berge, L. | |
| dc.creator | Blumer, J. | |
| dc.creator | Broniatowski, A. | |
| dc.creator | Censier, B. | |
| dc.creator | Chabert, L. | |
| dc.creator | Chapellier, M. | |
| dc.creator | Chardin, G. | |
| dc.creator | Charvin, P. | |
| dc.creator | Collin, S. | |
| dc.creator | De Jesus, M. | |
| dc.creator | Deschamps, H. | |
| dc.creator | Di Stefano, P. | |
| dc.creator | Dolgorouky, Y. | |
| dc.creator | Drain, D. | |
| dc.creator | Dumoulin, L. | |
| dc.creator | Eitel, K. | |
| dc.creator | Fesquet, M. | |
| dc.creator | Fiorucci, S. | |
| dc.creator | Gascon, J. | |
| dc.creator | Gerbier, G. | |
| dc.creator | Gerlic, E. | |
| dc.creator | Goldbach, C. | |
| dc.creator | Goyot, M. | |
| dc.creator | Gros, M. | |
| dc.creator | Herve, S. | |
| dc.creator | Horn, M. | |
| dc.creator | Juillard, A. | |
| dc.creator | Karolak, M. | |
| dc.creator | Kikuchi, C. | |
| dc.creator | de Lesquen, A. | |
| dc.creator | Luca, M. | |
| dc.creator | Mallet, J. | |
| dc.creator | Marnieros, S. | |
| dc.creator | Mosca, L. | |
| dc.creator | Navick, X. -F. | |
| dc.creator | Nollez, G. | |
| dc.creator | Pari, P. | |
| dc.creator | Schoeffel, L. | |
| dc.creator | Stern, M. | |
| dc.creator | Vagneron, L. | |
| dc.creator | Villar, V. | |
| dc.date | 2005-03-11 | |
| dc.date | 2005-05-26 | |
| dc.date.accessioned | 2026-07-07T10:27:26Z | |
| dc.date.available | 2026-07-07T10:27:26Z | |
| dc.description | The final results of the EDELWEISS-I dark matter search using cryogenic heat-and-ionization Ge detectors are presented. The final data sample corresponds to an increase by a factor five in exposure relative to the previously published results. A recoil energy threshold of 13 keV or better was achieved with three 320g detectors working simultaneously over four months of stable operation. Limits on the spin-independent cross-section for the scattering of a WIMP on a nucleon are derived from an accumulated fiducial exposure of 62 kg.d. | |
| dc.description | 42 pages, 16 figures, submitted to Physical Review D, 1 figure and 2 references added, some little changes in the text | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0503265 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0503265 | |
| dc.identifier | Phys.Rev.D71:122002,2005 | |
| dc.identifier | doi:10.1103/PhysRevD.71.122002 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/177149 | |
| dc.subject | Astrophysics | |
| dc.title | Final results of the EDELWEISS-I dark matter search with cryogenic heat-and-ionization Ge detectors | |
| dc.type | text |