出版社：SISSA, Scuola Internazionale Superiore di Studi Avanzati
摘要：The direct search for dark matter experiment, XENON100, using liquid xenon, has been in the process of taking data since January 2010 and will continue to do so for another year to reach a never yet achieved sensitivity on the WIMP nucleon cross section and may ultimately detect WIMPs. In addition, the experiment is already being pushed towards its next phase, XENON1T, which will be much larger with a fiducial mass of about 1 ton of liquid xenon. Reducing the background, it should be a hundred times more sensitive. While the previous phases were located at the LaboratoriNazionali del Gran Sasso (LNGS), in Italy, XENON1T could be hosted in the Laboratoire Souterrain de Modane (LSM), in France. The LSM site and its different level of gamma, neutron and muon background with an emphasis on the muon induced neutrons coming from the environmental rocks, have been investigated. Considering the available space at LSM and the final background level necessary for a dark matter search, an efficient and optimal shielding design has been established. All the results of these studies will be presented hereafter.
