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Critical revision of the ZEPLIN-I sensitivity to WIMP interactions

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arxiv astro-ph/0512120 v2 pith:22D47Z6G submitted 2005-12-05 astro-ph

classification astro-ph
keywords discriminationpicobarnsensitivityzeplin-iinteractionsrecoilwimpabove
verification ladder T0 review T1 audit T2 compute T3 formal
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abstract

The ZEPLIN collaboration has recently published its first result presenting a maximum sensitivity of $1.1 \times 10^{-6}$ picobarn for a WIMP mass of $\approx$ 60 GeV. The analysis is based on a discrimination method using the different time distribution of scintillation light generated in electron recoil and nuclear recoil interactions. We show that the methodology followed both for the calibration of the ZEPLIN-I detector response and for the estimation of the discrimination power is not reliable enough to claim any background discrimination at the present stage. The ZEPLIN-I sensitivity appears then to be in the order of 10$^{-3}$ picobarn, three orders of magnitude above the claimed 1.1 10$^{-6}$ picobarn.

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