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ZEPLIN-III 实验首个科学运行限制了自旋相关 WIMP-核子散射截面。

Limits on the spin-dependent WIMP-nucleon cross sections from the first science run of the ZEPLIN-III experiment.

机构信息

Blackett Laboratory, Imperial College London, London, United Kingdom.

出版信息

Phys Rev Lett. 2009 Oct 9;103(15):151302. doi: 10.1103/PhysRevLett.103.151302. Epub 2009 Oct 8.

Abstract

We present new experimental constraints on the WIMP-nucleon spin-dependent elastic cross sections using data from the first science run of ZEPLIN-III, a two-phase xenon experiment searching for galactic dark matter weakly interacting massive particles based at the Boulby mine. Analysis of approximately 450 kg x days fiducial exposure allow us to place a 90%-confidence upper limit on the pure WIMP-neutron cross section of sigma(n)=1.9x10(-2) pb at 55 GeV/c(2) WIMP mass. Recent calculations of the nuclear spin structure based on the Bonn charge-dependent nucleon-nucleon potential were used for the odd-neutron isotopes 129Xe and 131Xe. These indicate that the sensitivity of xenon targets to the spin-dependent WIMP-proton interaction could be much lower than implied by previous calculations, whereas the WIMP-neutron sensitivity is impaired only by a factor of approximately 2.

摘要

我们提出了新的实验约束条件,用于 WIMP-核子自旋相关弹性散射截面,这些条件是基于在 Boulby 矿的 ZEPLIN-III 进行的第一次科学运行的数据,该实验是基于两相氙气实验,用于寻找银河系暗物质中的弱相互作用大质量粒子。对大约 450kg×天的本征曝光进行分析,我们可以在 55GeV/c(2)WIMP 质量处对纯 WIMP-中子截面 sigma(n)=1.9x10(-2)pb 施加 90%置信度的上限。最近基于 Bonn 电荷相关核子-核子势的核自旋结构计算被用于 129Xe 和 131Xe 这两种奇数中子同位素。这些结果表明,氙气靶对自旋相关 WIMP-质子相互作用的灵敏度可能比之前的计算所暗示的要低得多,而 WIMP-中子的灵敏度仅降低了大约 2 倍。

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