Abstract
The XENON10 experiment at the Gran Sasso National Laboratory uses a 15 kg xenon dual phase time projection chamber to search for dark matter weakly interacting massive particles (WIMPs). The detector measures simultaneously the scintillation and the ionization produced by radiation in pure liquid xenon to discriminate signal from background down to 4.5 keV nuclear-recoil energy. A blind analysis of 58.6 live days of data, acquired between October 6, 2006, and February 14, 2007, and using a fiducial mass of 5.4 kg, excludes previously unexplored parameter space, setting a new 90% C.L. upper limit for the WIMP-nucleon spin-independent cross section of 8.8×10-44cm2 for a WIMP mass of 100GeV/c2, and 4.5×10-44cm2 for a WIMP mass of 30GeV/c2. This result further constrains predictions of supersymmetric models.
Original language | English (US) |
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Article number | 021303 |
Journal | Physical review letters |
Volume | 100 |
Issue number | 2 |
DOIs | |
State | Published - Jan 17 2008 |
All Science Journal Classification (ASJC) codes
- General Physics and Astronomy