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arXiv 1702.07666astro-ph.COhep-exphysics.ins-det
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PICO-60 C $_3$ F $_8$泡室的暗物质搜索结果

Dark Matter Search Results from the PICO-60 C$_3$F$_8$ Bubble Chamber

C. Amole, M. Ardid, I. J. Arnquist, D. M. Asner, D. Baxter, E. Behnke, P. Bhattacharjee, H. Borsodi, M. Bou-Cabo, P. Campion, G. Cao, C. J. Chen, U. Chowdhury, … 展开作者

C. Amole, M. Ardid, I. J. Arnquist, D. M. Asner, D. Baxter, E. Behnke, P. Bhattacharjee, H. Borsodi, M. Bou-Cabo, P. Campion, G. Cao, C. J. Chen, U. Chowdhury, K. Clark, J. I. Collar, P. S. Cooper, M. Crisler, G. Crowder, C. E. Dahl, M. Das, S. Fallows, J. Farine, I. Felis, R. Filgas, F. Girard, G. Giroux, J. Hall, O. Harris, E. W. Hoppe, M. Jin, C. B. Krauss, M. Laurin, I. Lawson, A. Leblanc, I. Levine, W. H. Lippincott, F. Mamedov, D. Maurya, P. Mitra, T. Nania, R. Neilson, A. J. Noble, S. Olson, A. Ortega, A. Plante, R. Podviyanuk, S. Priya, A. E. Robinson, A. Roeder, R. Rucinski, O. Scallon, S. Seth, A. Sonnenschein, N. Starinski, I. Štekl, F. Tardif, E. Vázquez-Jáuregui, J. Wells, U. Wichoski, Y. Yan, V. Zacek, J. Zhang

摘要:

PICO-60暗物质探测器,一个泡室充满了52公斤的C $_3$ F $_8$位于SNOLAB地下实验室的操作报告的新结果。与以前的PICO气泡室一样,PICO-60 C $_3$ F $_8$具有出色的电子反冲和α衰变抑制能力,观察到的多次散射中子率表明每月的单次散射中子背景小于1次。在3.3千电子伏的热力学阈值下,对效率校正后的1167千克-天曝光量进行盲分析,发现没有单散射核反冲候选物,与预测的背景一致。这些结果设置了最严格的直接检测约束,迄今为止在3.4 $\times$ 10 $^{-41}$厘米$^2$的30 GeV的$\thinspace$ c $^{-2}$ WIMP,一个以上的数量级的改进,从以前的PICO结果的WIMP质子自旋相关的横截面。

英文摘要:

New results are reported from the operation of the PICO-60 dark matter detector, a bubble chamber filled with 52 kg of C$_3$F$_8$ located in the SNOLAB underground laboratory. As in previous PICO bubble chambers, PICO-60 C$_3$F$_8$ exhibits excellent electron recoil and alpha decay rejection, and the observed multiple-scattering neutron rate indicates a single-scatter neutron background of less than 1 event per month. A blind analysis of an efficiency-corrected 1167-kg-day exposure at a 3.3-keV thermodynamic threshold reveals no single-scattering nuclear recoil candidates, consistent with the predicted background. These results set the most stringent direct-detection constraint to date on the WIMP-proton spin-dependent cross section at 3.4 $\times$ 10$^{-41}$ cm$^2$ for a 30-GeV$\thinspace$c$^{-2}$ WIMP, more than one order of magnitude improvement from previous PICO results.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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