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Implications on Inelastic Dark Matter from 100 Live Days of XENON100 Data

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arxiv 1104.3121 v2 pith:FL52AK2X submitted 2011-04-15 astro-ph.CO

Implications on Inelastic Dark Matter from 100 Live Days of XENON100 Data

XENON100 Collaboration: E. Aprile , K. Arisaka , F. Arneodo , A. Askin , L. Baudis , A. Behrens , K. Bokeloh , E. Brown
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T. Bruch G. Bruno J. M. R. Cardoso W.-T. Chen B. Choi D. Cline E. Duchovni S. Fattori A. D. Ferella F. Gao K.-L. Giboni E. Gross A. Kish C. W. Lam J. Lamblin R. F. Lang C. Levy K. E. Lim Q. Lin S. Lindemann M. Lindner J. A. M. Lopes K. Lung T. Marrod\'an Undagoitia Y. Mei A. J. Melgarejo Fernandez K. Ni U. Oberlack S. E. A. Orrigo E. Pantic R. Persiani G. Plante A. C. C. Ribeiro R. Santorelli J. M. F. dos Santos G. Sartorelli M. Schumann M. Selvi P. Shagin H. Simgen A. Teymourian D. Thers O. Vitells H. Wang M. Weber C. Weinheimer
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The XENON100 experiment has recently completed a dark matter run with 100.9 live-days of data, taken from January to June 2010. Events in a 48kg fiducial volume in the energy range between 8.4 and 44.6 keVnr have been analyzed. A total of three events have been found in the predefined signal region, compatible with the background prediction of (1.8 \pm 0.6) events. Based on this analysis we present limits on the WIMP-nucleon cross section for inelastic dark matter. With the present data we are able to rule out the explanation for the observed DAMA/LIBRA modulation as being due to inelastic dark matter scattering off iodine at a 90% confidence level.

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