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Limits on inelastic dark matter from ZEPLIN-III

Akimov, D; Araújo, HM; Barnes, EJ; Belov, VA; Bewick, A; Burenkov, AA; Cashmore, R; ... Walker, RJ; + view all (2010) Limits on inelastic dark matter from ZEPLIN-III. Physics Letters B , 692 (3) pp. 180-183. 10.1016/j.physletb.2010.07.042. Green open access

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Abstract

We present limits on the WIMP-nucleon cross section for inelastic dark matter from a reanalysis of the 2008 run of ZEPLIN-III. Cuts, notably on scintillation pulse shape and scintillation-to-ionisation ratio, give a net exposure of 63kgday in the range 20-80 keV nuclear recoil energy, in which 6 events are observed. Upper limits on signal rate are derived from the maximum empty patch in the data. Under standard halo assumptions a small region of parameter space consistent, at 99% CL, with causing the 1.17tonyr DAMA modulation signal is allowed at 90% CL: it is in the mass range 45-60 GeVc-2 with a minimum CL of 87%, again derived from the maximum patch. This is the tightest constraint yet presented using xenon, a target nucleus whose similarity to iodine mitigiates systematic error from the assumed halo.

Type: Article
Title: Limits on inelastic dark matter from ZEPLIN-III
Open access status: An open access version is available from UCL Discovery
DOI: 10.1016/j.physletb.2010.07.042
Publisher version: http://doi.org/10.1016/j.physletb.2010.07.042
Language: English
Additional information: Copyright © 2010 Elsevier B.V. Open access under CC BY license.
Keywords: Inelastic dark matter, WIMPs, Xenon
UCL classification: UCL
UCL > Provost and Vice Provost Offices > UCL BEAMS
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences
UCL > Provost and Vice Provost Offices > UCL BEAMS > Faculty of Maths and Physical Sciences > Dept of Physics and Astronomy
URI: https://discovery.ucl.ac.uk/id/eprint/1352130
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