Where will supersymmetric dark matter first be seen? Liang Gao National observatories of China, CAS.
The XENON Project A 1 tonne Liquid Xenon experiment for a sensitive Dark Matter Search Elena Aprile Columbia University.
Dark Matter Direct Detection roadmap strategy
Gaitskell XENON Experiment - SAGENAP Factors Affecting Detector Performance Goals and Alternative Photo-detectors Rick Gaitskell Department of Physics.
Dark Matter G. Chardin CEA/Saclay, DAPNIA. Motivations for non-baryonic Dark Matter Search - 1 Astrophysical measurements –“Dark” matter halo around the.
Low background techniques from XMASS Low Radioactivity Techniques 2013 Laboratori Nazionali del Gran Sasso Assergi (AQ), Italy, April 10-12, 2013 Hiroshi.
