2006/02/21 by S. Balestra, Balestra, S., S. Cecchini +46
Physics and Astronomy · #Astrophysics and Cosmic Phenomena #Dark Matter and Cosmic Phenomena #Solar and Space Plasma Dynamics #hep-ex
paper · pdf · doi:10.48550/arxiv.hep-ex/0602036
Paper presented by G. Giacomelli at the European Conference on High Energy Physics, July 21-27 2005, Lisboa, Portugal
arxiv created 2006/02/21 · arxiv updated 2009/12/01
The search for rare particles in the cosmic radiation remains one of the main aims of non-accelerator particle astrophysics. Experiments at high altitude allow lower mass thresholds with respect to detectors at sea level or underground. The SLIM experiment is a large array of nuclear track detectors located at the Chacaltaya High Altitude Laboratory (5290 m a.s.l.). The preliminary results from the analysis of a part of the first 236 sq.m exposed for more than 3.6 y are here reported. The detector is sensitive to Intermediate Mass Magnetic Monopoles and to SQM nuggets and Q-balls, which are possible Dark Matter candidates.