Spin-dependent dark matter interactions at loop-level in Ar and Xe

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Nassim Bozorgnia, Muping Chen, Graciela B. Gelmini, Alvine C. Kamaha and Yongheng Xu
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引用次数: 0

Abstract

Xenon and argon are the two noble gases used in tonne scale dark matter direct detection experiments. We compare the detection capability of both target elements for interactions due to a pseudoscalar mediator including loop-level contributions to the cross section. At tree-level this type of interaction depends on the nuclear spin and would thus not be detectable in argon-based detectors, since Ar has spin zero. However, at the loop-level the same interaction yields spin-independent contributions that would be detectable in an argon target and are not negligible with respect to the tree-level interactions in xenon, because these are momentum suppressed. In fact, the loop-level contributions are also important for xenon-based experiments at low recoil energies, which could change their discovery reach for this interaction.
Ar和Xe中自旋依赖的暗物质环水平相互作用
氙和氩是吨级暗物质直接探测实验中使用的两种惰性气体。我们比较了两个目标元件的相互作用的检测能力,这是由于一个伪标量中介,包括环路水平对截面的贡献。在树的层次上,这种类型的相互作用依赖于核自旋,因此在氩基探测器中是检测不到的,因为Ar的自旋为零。然而,在环水平上,同样的相互作用产生了与自旋无关的贡献,在氩气目标中可以检测到,并且相对于氙中的树水平相互作用来说是不可忽略的,因为这些相互作用是动量抑制的。事实上,环路水平的贡献对于低反冲能量的氙基实验也很重要,这可能会改变他们对这种相互作用的发现范围。
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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