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Effective field theory analysis of the first LUX dark matter search
Physical Review D ( IF 4.6 ) Pub Date : 2021-06-22 , DOI: 10.1103/physrevd.103.122005
D. S. Akerib , S. Alsum , H. M. Araújo , X. Bai , J. Balajthy , A. Baxter , E. P. Bernard , A. Bernstein , T. P. Biesiadzinski , E. M. Boulton , B. Boxer , P. Brás , S. Burdin , D. Byram , M. C. Carmona-Benitez , C. Chan , J. E. Cutter , L. de Viveiros , E. Druszkiewicz , A. Fan , S. Fiorucci , R. J. Gaitskell , C. Ghag , M. G. D. Gilchriese , C. Gwilliam , C. R. Hall , S. J. Haselschwardt , S. A. Hertel , D. P. Hogan , M. Horn , D. Q. Huang , C. M. Ignarra , R. G. Jacobsen , O. Jahangir , W. Ji , K. Kamdin , K. Kazkaz , D. Khaitan , E. V. Korolkova , S. Kravitz , V. A. Kudryavtsev , N. A. Larsen , E. Leason , B. G. Lenardo , K. T. Lesko , J. Liao , J. Lin , A. Lindote , M. I. Lopes , A. Manalaysay , R. L. Mannino , N. Marangou , D. N. McKinsey , D.-M. Mei , M. Moongweluwan , J. A. Morad , A. St. J. Murphy , A. Naylor , C. Nehrkorn , H. N. Nelson , F. Neves , A. Nilima , K. C. Oliver-Mallory , K. J. Palladino , E. K. Pease , Q. Riffard , G. R. C. Rischbieter , C. Rhyne , P. Rossiter , S. Shaw , T. A. Shutt , C. Silva , M. Solmaz , V. N. Solovov , P. Sorensen , T. J. Sumner , M. Szydagis , D. J. Taylor , R. Taylor , W. C. Taylor , B. P. Tennyson , P. A. Terman , D. R. Tiedt , W. H. To , L. Tvrznikova , U. Utku , S. Uvarov , A. Vacheret , V. Velan , R. C. Webb , J. T. White , T. J. Whitis , M. S. Witherell , F. L. H. Wolfs , D. Woodward , J. Xu , C. Zhang ,

The Large Underground Xenon (LUX) dark matter search was a 250-kg active mass dual-phase time projection chamber that operated by detecting light and ionization signals from particles incident on a xenon target. In December 2015, LUX reported a minimum 90% upper C.L. of 6×1046cm2 on the spin-independent WIMP-nucleon elastic scattering cross section based on a 1.4×104kg·day exposure in its first science run. Tension between experiments and the absence of a definitive positive detection suggest it would be prudent to search for WIMPs outside the standard spin-independent/spin-dependent paradigm. Recent theoretical work has identified a complete basis of 14 independent effective field theory (EFT) operators to describe WIMP-nucleon interactions. In addition to spin-independent and spin-dependent nuclear responses, these operators can produce novel responses such as angular-momentum-dependent and spin-orbit couplings. Here we report on a search for all 14 of these EFT couplings with data from LUX’s first science run. Limits are placed on each coupling as a function of WIMP mass.

中文翻译:

第一次LUX暗物质搜索的有效场论分析

大型地下氙气 (LUX) 暗物质搜索是一个 250 千克活性质量双相时间投影室,它通过检测入射在氙气靶上的粒子的光和电离信号进行操作。2015 年 12 月,LUX 报告了至少 90% 的上限值6×10-46厘米2 在基于自旋的 WIMP-核子弹性散射截面上 1.4×104公斤·在第一次科学运行中曝光。实验之间的紧张和没有明确的阳性检测表明在标准的自旋独立/自旋依赖范式之外搜索 WIMP 是谨慎的。最近的理论工作已经确定了 14 个独立的有效场理论 (EFT) 算子的完整基础来描述 WIMP-核子相互作用。除了与自旋无关和与自旋相关的核响应之外,这些算子还可以产生新的响应,例如角动量相关和自旋轨道耦合。在这里,我们报告了对所有 14 个这些 EFT 耦合的搜索,以及来自 LUX 首次科学运行的数据。作为 WIMP 质量的函数,对每个耦合施加了限制。
更新日期:2021-06-22
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