The XENON10 WIMP Direct Detection Search at the Gran Sasso Underground Laboratory

Details The XENON10 WIMP Direct Detection Search at the Gran Sasso Underground Laboratory The XENON10 WIMP Direct Detection Search at the Gran Sasso Underground Laboratory

Sep 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1166..212m&link_type=abstract

SOURCES AND DETECTION OF DARK MATTER AND DARK ENERGY IN THE UNIVERSE: Proceedings of the 8th UCLA Symposium. AIP Conference Pro

Other

Dark Matter, Tracking And Position-Sensitive Detectors, Neutrino, Muon, Pion, And Other Elementary Particle Detectors, Cosmic Ray Detectors

Scientific paper

The direct detection search for WIMPs with the XENON10 detector has produced among the best results in the field to date. The detector is a dual-phase liquid xenon time projection chamber, capable of 3-D position reconstruction and nuclear recoil discrimination. We summarize 58.6 live-days of WIMP search data collected at the Gran Sasso Underground Laboratory (LNGS) in Italy. With this data we have been able to set stringent upper limits on the spin-dependent and spin-independent WIMP scattering cross sections, in addition to a lower limit of 2.2 TeV/c2 on the mass of the heavy Majorana neutrino.

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