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First limits on WIMP nuclear recoil signals in ZEPLIN-II: A two-phase xenon detector for dark matter detection

机译:ZEPLIN-II中WIMP核反冲信号的第一个限制:用于暗物质检测的两相氙检测器

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摘要

Results are presented from the first underground data run of ZEPLIN-II, a 31 kg two-phase xenon detector developed to observe nuclear recoils from hypothetical weakly interacting massive dark matter particles. Discrimination between nuclear recoils and background electron recoils is afforded by recording both the scintillation and ionisation signals generated within the liquid xenon, with the ratio of these signals being different for the two classes of event. This ratio is calibrated for different incident species using an AmBe neutron source and 60Co γ-ray sources. From our first 31 live days of running ZEPLIN-II, the total exposure following the application of fiducial and stability cuts was 225 kg × days. A background population of radon progeny events was observed in this run, arising from radon emission in the gas purification getters, due to radon daughter ion decays on the surfaces of the walls of the chamber. An acceptance window, defined by the neutron calibration data, of 50% nuclear recoil acceptance between 5 keVee and 20 keVee, had an observed count of 29 events, with a summed expectation of 28.6 ± 4.3 γ-ray and radon progeny induced background events. These figures provide a 90% c.l. upper limit to the number of nuclear recoils of 10.4 events in this acceptance window, which converts to a WIMP nucleon spin-independent cross-section with a minimum of 6.6 × 10-7 pb following the inclusion of an energy-dependent, calibrated, efficiency. A second run is currently underway in which the radon progeny will be eliminated, thereby removing the background population, with a projected sensitivity of 2 × 10-7 pb for similar exposures as the first run.
机译:结果来自ZEPLIN-II的第一个地下数据运行,ZEPLIN-II是一种31千克的两相氙探测器,其开发目的是观察假设的弱相互作用的大型暗物质粒子的核后坐力。通过记录在液体氙气中产生的闪烁和电离信号,可以区分核后座力和背景电子后座力,这两种事件的比率不同。使用AmBe中子源和60Coγ射线源对不同入射物种的该比率进行了校准。从运行ZEPLIN-II的前31个工作日开始,应用基准和稳定性削减后的总暴露量为225 kg×天。在此运行中,由于the气子离子在腔室壁表面的衰变而在气体净化吸气剂中产生emission气,因此在本次运行中观察到of气后代事件的背景种群。由中子校准数据定义的5keVee和20keVee之间的50%核反冲接受度的接受窗口具有29个事件的观察计数,总期望值为28.6±4.3γ射线和ra子代诱发的背景事件。这些数字提供了90%的c.l.此接受窗口中发生10.4次事件的核后坐次数的上限,在包含能量相关的校准效率后,其转换为WIMP核子自旋无关截面,最小为6.6×10-7 pb 。目前正在进行第二轮试验,其中eliminated后代将被消除,从而消除背景种群,对于与第一轮试验相似的暴露,预计灵敏度为2×10-7 pb。

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