直接探测暗物质的有效理论方法

J. Hisano
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引用次数: 11

摘要

现在可以肯定宇宙中存在暗物质。然而,我们不知道它的性质,在粒子物理学或天文学的标准模型中也没有暗物质候选者。然而,在标准模型之外的模型中,弱相互作用的大质量粒子(wimp)是可以提供解释的主要候选者之一。暗物质直接探测实验是阐明暗物质本质的一种方法,该实验是寻找被wimp反冲的原子核。本章介绍了一种有效的场理论(EFT)方法来计算核子- wimp弹性散射截面。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Effective Theory Approach to Direct Detection of Dark Matter
It is now certain that dark matter exists in the Universe. However, we do not know its nature, nor are there dark matter candidates in the standard model of particle physics or astronomy However, weakly interacting massive particles (WIMPs) in models beyond the standard model are one of the leading candidates available to provide explanation. The dark matter direct detection experiments, in which the nuclei recoiled by WIMPs are sought, are one of the methods to elucidate the nature of dark matter. This chapter introduces an effective field theory (EFT) approach in order to evaluate the nucleon–WIMP elastic scattering cross section.
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