Phys. Rev. D
80,
115005
(2009)
[8 pages]
Constraints on inelastic dark matter from XENON10
J. Angle et al.
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J. Angle1,2, E. Aprile3, F. Arneodo4, L. Baudis2, A. Bernstein5, A. Bolozdynya6, L. C. C. Coelho7, C. E. Dahl8, 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. Kwong8, J. A. M. Lopes7, N. Madden5, A. Manalaysay1,2, A. Manzur11, D. N. McKinsey11, M. E. Monzani3, K. Ni11, U. Oberlack10, J. Orboeck12, G. Plante3, R. Santorelli3, J. M. F. dos Santos7, P. Shagin10, T. Shutt6, P. Sorensen5,*, S. Schulte12, C. Winant5, and M. Yamashita3 (XENON10 Collaboration)
1Department of Physics, University of Florida, Gainesville, Florida 32611, USA 2Physics Institute, University of Zürich, Winterthurerstrasse 190, CH-8057, Zürich, Switzerland 3Department of Physics, Columbia University, New York, New York 10027, USA 4Gran Sasso National Laboratory, Assergi, L’Aquila, 67010, Italy 5Lawrence Livermore National Laboratory, 7000 East Avenue, 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 12Department of Physics, RWTH Aachen University, Aachen, 52074, Germany
Received 19 October 2009; published 9 December 2009
It has been suggested that dark matter particles which scatter inelastically from detector target nuclei could explain the apparent incompatibility of the DAMA modulation signal (interpreted as evidence for particle dark matter) with the null results from CDMS-II and XENON10. Among the predictions of inelastically interacting dark matter are a suppression of low-energy events, and a population of nuclear recoil events at higher nuclear recoil equivalent energies. This is in stark contrast to the well-known expectation of a falling exponential spectrum for the case of elastic interactions. We present a new analysis of XENON10 dark matter search data extending to Enr=75 keV nuclear recoil equivalent energy. Our results exclude a significant region of previously allowed parameter space in the model of inelastically interacting dark matter. In particular, it is found that dark matter particle masses mχ≳150 GeV are disfavored.
© 2009 The American Physical Society
URL:
http://link.aps.org/doi/10.1103/PhysRevD.80.115005
DOI:
10.1103/PhysRevD.80.115005
PACS:
95.35.+d, 14.80.Ly, 29.40.Gx, 95.55.Vj
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