Precision Measurement of Parity Non-Conserving, Weak-force Induced Transitions in Atomic Cesium

原子铯中宇称非守恒、弱力诱导跃迁的精确测量

• 批准号: 1912519
• 负责人: Daniel Elliott
• 金额: $ 108.21万
• 依托单位: Purdue University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2019
• 资助国家: 美国
• 起止时间: 2019-07-15 至 2024-06-30
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1912519&HistoricalAwards=false
• 关键词: Precision; Measurement; Parity; Non; Conserving

We understand the universe in which we live through four fundamental forces: gravitational, electromagnetic, weak (responsible for radioactivity and beta decay), and strong (which provides the force that binds atomic nuclei together). A theoretical framework that unifies three of these forces (electromagnetic, weak and strong) is known as the standard model, and has been very successful at explaining a broad range of observables and predicting others. There are, however, several notable effects that the standard model has not been able to explain, including the preponderance of regular matter in the universe (but very little anti-matter), and the existence and nature of dark matter and dark energy. The evidence of the existence of dark matter is provided by observations of the rotation of galaxies. From this, we know that the universe contains much more matter than we have been able to observe. But we know very little about what this "dark" matter is, or how, other than through gravity, it interacts with the matter that we can observe. In this project, the principal investigator and his team will use precision measurements of extremely weak optical interactions of a laser field with cesium atoms to test the standard model, and to search for signatures of physical effects that lie outside the realm of the standard model. The Principal Investigator and his research team are developing two measurement techniques to probe the weak force interactions in atomic cesium. Each measurement technique is a variant of two-color coherent control, in which the amplitudes for two transitions in the optical or radio-frequency range interfere with one another. One measurement, based on the 6s 2S1/2 → 7s 2S1/2 transition, is designed to provide an improved value of the weak charge of the cesium nucleus. The second, based on the 9.19 GHz transition between the hyperfine components of the ground state, is due solely to nuclear-spin dependent contributions such as the anapole moment of the nucleus. Atomic cesium was, of course, the choice of Wieman for his 1997 work, and that group's measurement is still the most precise measurement of the weak charge in any atomic species. Cesium is also the only species in which the nuclear anapole moment has been observed. The degree to which the measurement of the weak charge agrees with the standard model prediction will place constraints upon various models of physics beyond the standard model. The coherent control technique is expected to result in a reduction of the susceptibility of the measurement to systematic errors, critical for the success of these measurements.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

我们通过四种基本力来理解我们所生活的宇宙：引力，电磁力，弱（负责放射性和β衰变）和强（提供将原子核结合在一起的力）。一个统一了三种力（电磁力、弱力和强力）的理论框架被称为标准模型，它在解释广泛的可观测量和预测其他可观测量方面非常成功。 然而，有几个值得注意的效应是标准模型无法解释的，包括宇宙中规则物质的优势（但反物质很少），以及暗物质和暗能量的存在和性质。 暗物质存在的证据是由星系旋转的观测提供的。 由此，我们知道宇宙包含的物质比我们能够观察到的要多得多。 但是我们对这种“暗”物质是什么知之甚少，或者除了通过引力之外，它如何与我们可以观察到的物质相互作用。 在这个项目中，首席研究员和他的团队将使用激光场与铯原子的极弱光学相互作用的精确测量来测试标准模型，并寻找标准模型范围之外的物理效应的特征。首席研究员和他的研究小组正在开发两种测量技术，以探测原子铯中的弱力相互作用。 每种测量技术都是双色相干控制的一种变体，其中光学或射频范围内的两个跃迁的振幅相互干扰。 其中一种测量是基于6s 2S 1/2#8594; 7s 2S 1/2跃迁，旨在提供铯核弱电荷的改进值。第二个，基于9.19 GHz的过渡之间的超精细组件的基态，是完全由于核自旋相关的贡献，如原子核的anapole时刻。 当然，原子铯是Wieman在1997年的工作中选择的，并且该小组的测量仍然是任何原子物种中弱电荷的最精确测量。 铯也是唯一一个被观察到原子核顶点矩的物质。 弱电荷的测量与标准模型预测一致的程度将对标准模型之外的各种物理模型施加约束。 相干控制技术预计将导致测量的系统误差的敏感性降低，这些测量的成功至关重要。该奖项反映了NSF的法定使命，并已被认为是值得通过使用基金会的智力价值和更广泛的影响审查标准进行评估的支持。