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The Dark Matter Enigma

机译:黑暗物质之谜

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The standard model of particle physics has been extraordinary successful. This model describes all known particles and nuclei in terms of a few fundamental quarks and leptons, and accounts for their interactions via strong, weak, and electromagnetic interactions. The model has undergone rigorous testing and measured values are seen to agree with theory to phenomenal precision. For example, the anomalous magnetic moment of the electron, a precision test of the electromagnetic part of the theory agrees with the theoretical prediction to a phenomenal 12 decimal place accuracy~([1]). Despite this success the model appears to be incomplete. During the past few decades it has become abundantly clear that we can only account for 20% of the total matter content of the Universe in terms of standard model particles. The nature of the other 80%, dubbed "dark matter" as it doesn't produce observable light like other astronomical objects, is completely unknown today. The detection and characterization of dark matter is one of the highest priority research topics in physics today.
机译:粒子物理学的标准模型非常成功。该模型用一些基本的夸克和轻子描述了所有已知的粒子和核,并通过强,弱和电磁相互作用解释了它们的相互作用。该模型经过了严格的测试,测量值与理论上的惊人精度相吻合。例如,电子的反常磁矩,理论电磁部分的精确度测试与理论预测相符,达到了惊人的12位小数位精度〜([1])。尽管取得了成功,但该模型似乎并不完整。在过去的几十年中,非常清楚的是,就标准模型粒子而言,我们只能占宇宙总物质含量的20%。其余80%的性质被称为“暗物质”,因为它不像其他天文物体那样产生可观察到的光,今天完全未知。暗物质的检测和表征是当今物理学中最优先的研究课题之一。

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