论文标题

直接的暗物质搜索使用XMASS-I的完整数据集进行

Direct dark matter searches with the full data set of XMASS-I

论文作者

XMASS Collaboration, Abe, K., Hiraide, K., Kato, N., Moriyama, S., Nakahata, M., Sato, K., Sekiya, H., Suzuki, T., Suzuki, Y., Takeda, A., Yang, B. S., Kim, N. Y., Kim, Y. D., Kim, Y. H., Itow, Y., Martens, K., Mason, A., Yamashita, M., Miuchi, K., Takeuchi, Y., Lee, K. B., Lee, M. K., Fukuda, Y., Ogawa, H., Ichimura, K., Kishimoto, Y., Nishijima, K., Fushimi, K., Xu, B. D., Kobayashi, K., Nakamura, S.

论文摘要

本文报道了使用Xmass-I(单相液体氙气检测器)的完整数据集进行各种WIMP暗物质搜索。稳定的XMASS-I数据在2013年11月20日至2019年2月1日之间累积了1590.9天的总直播时间,分析门槛为$ {\ rm 1.0 \,kev_ {ee}} $。在后半部分中,数据采用$ {\ rm 0.5 \的较低分析阈值,kev_ {ee}}} $也可以通过新的低阈值触发器获得。在检测器的97〜 kg基准量中搜索wimb信号,对$ {\ rm 1.4 \ rm 1.4 \ times 10^{ - 44} \,cm^{2}} $的Wimp-nucleon散射横截面的限制限制了$ {\ rm 60 \,gev,gev,gev,gev,gev/c^priforts $ coptripter/cm^{2}} $。我们还搜索了探测器的整个目标体积中的WIMP诱导的年度调制特征,其中包含832〜kg液体氙气。对于$ {\ rm 8 \,gev/c^{2}} $ wimp的核后坐力,此分析产生了90 \%Cl横截面限制$ {\ rm 2.3 \ times 10^{ - 42}} { - 42} \,cm^{2}}} $。评估了$ {\ rm 0.5 \,gev/c^{2}} $ migdal效果和bremsstrahlung签名,并导致90 \%cl横截面限制$ {\ rm 1.4 \ rm 1.4 \ rm 1.4 \ rm 1.4 \ rm times 10^{ - 35} { - 35} { - 35} \,cm^{2}} 10^{ - 33} \,cm^{2}} $。

Various WIMP dark matter searches using the full data set of XMASS-I, a single-phase liquid xenon detector, are reported in this paper. Stable XMASS-I data taking accumulated a total live time of 1590.9 days between November 20, 2013 and February 1, 2019 with an analysis threshold of ${\rm 1.0\,keV_{ee}}$. In the latter half of data taking a lower analysis threshold of ${\rm 0.5\,keV_{ee}}$ was also available through a new low threshold trigger. Searching for a WIMP signal in the detector's 97~kg fiducial volume yielded a limit on the WIMP-nucleon scattering cross section of ${\rm 1.4\times 10^{-44}\, cm^{2}}$ for a ${\rm 60\,GeV/c^{2}}$ WIMP at the 90$\%$ confidence level. We also searched for WIMP induced annual modulation signatures in the detector's whole target volume, containing 832~kg of liquid xenon. For nuclear recoils of a ${\rm 8\,GeV/c^{2}}$ WIMP this analysis yielded a 90\% CL cross section limit of ${\rm 2.3\times 10^{-42}\, cm^{2}}$. At a WIMP mass of ${\rm 0.5\, GeV/c^{2}}$ the Migdal effect and Bremsstrahlung signatures were evaluated and lead to 90\% CL cross section limits of ${\rm 1.4\times 10^{-35}\, cm^{2}}$ and ${\rm 1.1\times 10^{-33}\, cm^{2}}$ respectively.

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