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      First results from the LUX dark matter experiment at the Sanford Underground Research Facility

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          Abstract

          The Large Underground Xenon (LUX) experiment, a dual-phase xenon time-projection chamber operating at the Sanford Underground Research Facility (Lead, South Dakota), was cooled and filled in February 2013. We report results of the first WIMP search dataset, taken during the period April to August 2013, presenting the analysis of 85.3 live-days of data with a fiducial volume of 118 kg. A profile-likelihood analysis technique shows our data to be consistent with the background-only hypothesis, allowing 90% confidence limits to be set on spin-independent WIMP-nucleon elastic scattering with a minimum upper limit on the cross section of \(7.6 \times 10^{-46}\) cm\(^{2}\) at a WIMP mass of 33 GeV/c\(^2\). We find that the LUX data are in strong disagreement with low-mass WIMP signal interpretations of the results from several recent direct detection experiments.

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          Detectability of certain dark-matter candidates

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            Asymptotic formulae for likelihood-based tests of new physics

            We describe likelihood-based statistical tests for use in high energy physics for the discovery of new phenomena and for construction of confidence intervals on model parameters. We focus on the properties of the test procedures that allow one to account for systematic uncertainties. Explicit formulae for the asymptotic distributions of test statistics are derived using results of Wilks and Wald. We motivate and justify the use of a representative data set, called the "Asimov data set", which provides a simple method to obtain the median experimental sensitivity of a search or measurement as well as fluctuations about this expectation.
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              Inelastic and Elastic Scattering of 187-Mev Electrons from Selected Even-Even Nuclei

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                Author and article information

                Journal
                30 October 2013
                2014-02-05
                Article
                10.1103/PhysRevLett.112.091303
                1310.8214
                9fe5e7ef-1cee-4852-b7e8-c503c8a034f3

                http://arxiv.org/licenses/nonexclusive-distrib/1.0/

                History
                Custom metadata
                Phys. Rev. Lett. 112, 091303 (2014)
                Accepted by Phys. Rev. Lett. Appendix A included as supplementary material with PRL article
                astro-ph.CO astro-ph.IM hep-ex physics.ins-det

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