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利用冷原子对牛顿引力常数进行精密测量。

Precision measurement of the Newtonian gravitational constant using cold atoms.

机构信息

Dipartimento di Fisica e Astronomia and LENS, Università di Firenze - INFN Sezione di Firenze, Via Sansone 1, 50019 Sesto Fiorentino, Italy.

European Space Agency, Keplerlaan 1, PO Box 299, 2200 AG Noordwijk ZH, The Netherlands.

出版信息

Nature. 2014 Jun 26;510(7506):518-21. doi: 10.1038/nature13433. Epub 2014 Jun 18.

DOI:10.1038/nature13433
PMID:24965653
Abstract

About 300 experiments have tried to determine the value of the Newtonian gravitational constant, G, so far, but large discrepancies in the results have made it impossible to know its value precisely. The weakness of the gravitational interaction and the impossibility of shielding the effects of gravity make it very difficult to measure G while keeping systematic effects under control. Most previous experiments performed were based on the torsion pendulum or torsion balance scheme as in the experiment by Cavendish in 1798, and in all cases macroscopic masses were used. Here we report the precise determination of G using laser-cooled atoms and quantum interferometry. We obtain the value G = 6.67191(99) × 10(-11) m(3) kg(-1) s(-2) with a relative uncertainty of 150 parts per million (the combined standard uncertainty is given in parentheses). Our value differs by 1.5 combined standard deviations from the current recommended value of the Committee on Data for Science and Technology. A conceptually different experiment such as ours helps to identify the systematic errors that have proved elusive in previous experiments, thus improving the confidence in the value of G. There is no definitive relationship between G and the other fundamental constants, and there is no theoretical prediction for its value, against which to test experimental results. Improving the precision with which we know G has not only a pure metrological interest, but is also important because of the key role that G has in theories of gravitation, cosmology, particle physics and astrophysics and in geophysical models.

摘要

到目前为止,已有约 300 个实验试图确定牛顿引力常数 G 的值,但由于结果存在较大差异,因此无法精确获知其值。引力相互作用较弱,而且无法屏蔽重力的影响,这使得在控制系统效应的同时,很难对 G 进行测量。之前进行的大多数实验都是基于扭摆或扭秤方案,如 1798 年卡文迪什的实验,而且在所有情况下都使用了宏观质量。在这里,我们报告了使用激光冷却原子和量子干涉测量来精确确定 G 的结果。我们得到的值为 G = 6.67191(99) × 10(-11) m(3) kg(-1) s(-2),相对不确定度为 150 百万分之一(括号内给出的是综合标准不确定度)。与当前科学技术数据委员会推荐的值相比,我们的结果相差 1.5 个综合标准偏差。像我们这样的概念上不同的实验有助于识别先前实验中难以捉摸的系统误差,从而提高对 G 值的置信度。G 与其他基本常数之间没有确定的关系,也没有理论预测其值,因此无法用实验结果进行检验。提高我们对 G 了解的精度不仅具有纯粹的计量学意义,而且由于 G 在引力理论、宇宙学、粒子物理学和天体物理学以及地球物理模型中的关键作用,所以也很重要。

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