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arXiv 1902.04031astro-ph.COhep-exphysics.ins-det
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PICO-60 C $_3$ F $_8$泡室完全曝光的暗物质搜索结果

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

C. Amole, M. Ardid, I. J. Arnquist, D. M. Asner, D. Baxter, E. Behnke, M. Bressler, B. Broerman, G. Cao, C. J. Chen, U. Chowdhury, K. Clark, J. I. Collar, P. S.… 展开作者

C. Amole, M. Ardid, I. J. Arnquist, D. M. Asner, D. Baxter, E. Behnke, M. Bressler, B. Broerman, G. Cao, C. J. Chen, U. Chowdhury, K. Clark, J. I. Collar, P. S. Cooper, C. B. Coutu, C. Cowles, M. Crisler, G. Crowder, N. A. Cruz-Venegas, C. E. Dahl, M. Das, S. Fallows, J. Farine, I. Felis, R. Filgas, F. Girard, G. Giroux, J. Hall, C. Hardy, O. Harris, T. Hillier, E. W. Hoppe, C. M. Jackson, M. Jin, L. Klopfenstein, C. B. Krauss, M. Laurin, I. Lawson, A. Leblanc, I. Levine, C. Licciardi, W. H. Lippincott, B. Loer, F. Mamedov, P. Mitra, C. Moore, T. Nania, R. Neilson, A. J. Noble, P. Oedekerk, A. Ortega, M. -C. Piro, A. Plante, R. Podviyanuk, S. Priya, A. E. Robinson, S. Sahoo, O. Scallon, S. Seth, A. Sonnenschein, N. Starinski, I. Štekl, T. Sullivan, F. Tardif, E. Vázquez-Jáuregui, N. Walkowski, E. Weima, U. Wichoski, K. Wierman, Y. Yan, V. Zacek, J. Zhang

摘要:

最后的结果报告的PICO-60 C $_3$ F $_8$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。该室在低至1.2 keV的热力学阈值下操作,而不损失稳定性。在2.45 keV阈值下获得了新的盲态1404 kg-天暴露量,预期总背景速率与之前在3.3 keV下的1167 kg-天暴露量大致相同。这种增加的曝光部分是通过新的光学跟踪分析来实现的,以更好地识别探测器壁附近的事件,从而允许更大的基准体积。这些结果设置了最严格的直接检测约束的日期在2.5 $\times$ 10 $^{-41}$ cm $^2$的25 GeV的WIMP质子自旋相关的横截面,并改善了以前的PICO结果为3-5 GeV的WIMP的数量级。

英文摘要:

Final results are reported from operation of the PICO-60 C$_3$F$_8$ dark matter detector, a bubble chamber filled with 52 kg of C$_3$F$_8$ located in the SNOLAB underground laboratory. The chamber was operated at thermodynamic thresholds as low as 1.2 keV without loss of stability. A new blind 1404-kg-day exposure at 2.45 keV threshold was acquired with approximately the same expected total background rate as the previous 1167-kg-day exposure at 3.3 keV. This increased exposure is enabled in part by a new optical tracking analysis to better identify events near detector walls, permitting a larger fiducial volume. These results set the most stringent direct-detection constraint to date on the WIMP-proton spin-dependent cross section at 2.5 $\times$ 10$^{-41}$ cm$^2$ for a 25 GeV WIMP, and improve on previous PICO results for 3-5 GeV WIMPs by an order of magnitude.

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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