Phys. Rev. Lett.
100,
021303
(2008)
[5 pages]
First Results from the XENON10 Dark Matter Experiment at the Gran Sasso National Laboratory
J. Angle et al. XENON Collaboration
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J. Angle1,2, E. Aprile3,*, F. Arneodo4, L. Baudis2, A. Bernstein5, A. Bolozdynya6, P. Brusov6, L. C. C. Coelho7, C. E. Dahl6,8, L. DeViveiros9, A. D. Ferella2,4, L. M. P. Fernandes7, S. Fiorucci9, R. J. Gaitskell9, K. L. Giboni3, R. Gomez10, R. Hasty11, L. Kastens11, J. Kwong6,8, J. A. M. Lopes7, N. Madden5, A. Manalaysay1,2, A. Manzur11, D. N. McKinsey11, M. E. Monzani3, K. Ni11, U. Oberlack10, J. Orboeck2, G. Plante3, R. Santorelli3, J. M. F. dos Santos7, P. Shagin10, T. Shutt6, P. Sorensen9, S. Schulte2, C. Winant5, and M. Yamashita3 (XENON Collaboration)
1Department of Physics, University of Florida, Gainesville, Florida 32611, USA 2Department of Physics, RWTH Aachen University, Aachen, 52074, Germany 3Department of Physics, Columbia University, New York, New York 10027, USA 4INFN-Laboratori Nazionali del Gran Sasso, Assergi, 67010, Italy 5Lawrence Livermore National Laboratory, Livermore, California 94550, USA 6Department of Physics, Case Western Reserve University, Cleveland, Ohio 44106, USA 7Department of Physics, University of Coimbra, R. Larga, 3004-516, Coimbra, Portugal 8Department of Physics, Princeton University, Princeton, New Jersey 08540, USA 9Department of Physics, Brown University, Providence, Rhode Island 02912, USA 10Department of Physics and Astronomy, Rice University, Houston, Texas, 77251, USA 11Department of Physics, Yale University, New Haven, Connecticut 06511, USA
Received 31 May 2007; published 17 January 2008
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 8.8×10-44 cm2 for a WIMP mass of 100 GeV/c2, and 4.5×10-44 cm2 for a WIMP mass of 30 GeV/c2. This result further constrains predictions of supersymmetric models.
© 2008 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevLett.100.021303
DOI:
10.1103/PhysRevLett.100.021303
PACS:
95.35.+d, 14.80.Ly, 29.40.Mc, 95.55.Vj
*XENON Spokesperson. age@astro.columbia.edu.
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