The Muon g – 2 Experiment

Q4 Physics and Astronomy Nuclear Physics News Pub Date : 2022-04-03 DOI:10.1080/10619127.2022.2029235
M. Incagli, L. Gibbons
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Abstract

Introduction As its overarching quest, particle physics seeks to discover the complete set of fundamental components of matter and understand the forces through which they interact. Progress in our understanding, eventually culminating the Standard Model (SM) of fundamental particles, has been driven by increasing the energy available in the Center of Mass of collisions, the Energy Frontier, or through highprecision experiments that typically require large statistics, the Intensity Frontier. While the SM explains an astonishing range of phenomena, fundamental questions remain unanswered by the model: why three generations of quarks and of leptons; does the Higgs sector really provide the mass generation mechanism for quarks and leptons; what keeps the Higgs boson mass small when radiative corrections should drive it large; and many others. Explorations in both particle and nuclear physics at both frontiers strive to address these questions. The Intensity Frontier itself encompasses two complementary strategies: the search for rare or forbidden processes, like Lepton Flavor Violating (LFV) decays, that have highly suppressed rates within the SM but can receive significant rate enhancements in extensions of the SM, or the high-precision measurement of a fundamental quantity in which to search for a discrepancy with the value predicted by the SM. A discrepancy between measurement and prediction can hint at new physics, while agreement can often provide limits on the mass scales of new physics in various models well beyond those directly accessible at the energy frontier. This article addresses an example of the second method, the high-precision measurement of the muon magnetic anomaly, often known as g – 2, which has a long and rich history of theoretical and experimental successes that contributed to the establishment of the SM.
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μ子g - 2实验
作为其首要任务,粒子物理学试图发现物质的基本组成部分的完整集合,并了解通过它们相互作用的力。我们的理解的进步,最终达到基本粒子的标准模型(SM),是由不断增加的碰撞质量中心可用能量(能量边界),或通过通常需要大量统计数据的高精度实验(强度边界)推动的。虽然SM解释了一系列惊人的现象,但该模型仍未回答一些基本问题:为什么会有三代夸克和轻子;希格斯扇区真的提供了夸克和轻子的质量生成机制吗?当辐射修正应该使希格斯玻色子的质量变大时,是什么使它保持较小的质量;还有其他许多人。粒子物理和核物理在这两个前沿领域的探索都在努力解决这些问题。强度前沿本身包含两种互补的策略:寻找罕见或禁止的过程,如轻子风味破坏(LFV)衰变,在SM中具有高度抑制的速率,但在SM的扩展中可以获得显着的速率增强,或者对基本量进行高精度测量,以寻找与SM预测值的差异。测量和预测之间的差异可以暗示新的物理,而一致性通常可以在各种模型中为新物理的质量尺度提供限制,远远超出了在能量前沿直接获得的限制。本文讨论了第二种方法的一个例子,即高精度测量μ子磁异常,通常称为g - 2,它具有悠久而丰富的理论和实验成功的历史,有助于建立SM。
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来源期刊
Nuclear Physics News
Nuclear Physics News Physics and Astronomy-Nuclear and High Energy Physics
CiteScore
0.80
自引率
0.00%
发文量
39
期刊最新文献
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