The XENON100 Dark Matter Experiment

Details The XENON100 Dark Matter Experiment The XENON100 Dark Matter Experiment

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1241..458t&link_type=abstract

INVISIBLE UNIVERSE: Proceedings of the Conference. AIP Conference Proceedings, Volume 1241, pp. 458-462 (2010).

Computer Science

Performance

Dark Matter, Clusters Of Galaxies, Cosmic Background Radiation, Supersymmetry, Dark Matter, Galaxy Clusters, Background Radiations, Supersymmetry

Scientific paper

The XENON100 experiment is searching for WIMPs, which are particles that may consist dark matter. It is located in the underground laboratory of Gran Sasso (LNGS) in Italy at a depth of ~3600 m.w.e.. The experiment description, its performance and the expected background based on Monte Carlo simulations and material screening along with the projected sensitivities of the experiment are presented. In addition, a brief description of the upgrade XENON100 detector is given.

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