Department of Physics, University of Liverpool, Liverpool L697ZE, UK.
Department of Physics, University of California at Berkeley, Berkeley, California 94720-7300, USA.
Nature. 2016 Jan 21;529(7586):373-6. doi: 10.1038/nature16491.
Antimatter continues to intrigue physicists because of its apparent absence in the observable Universe. Current theory requires that matter and antimatter appeared in equal quantities after the Big Bang, but the Standard Model of particle physics offers no quantitative explanation for the apparent disappearance of half the Universe. It has recently become possible to study trapped atoms of antihydrogen to search for possible, as yet unobserved, differences in the physical behaviour of matter and antimatter. Here we consider the charge neutrality of the antihydrogen atom. By applying stochastic acceleration to trapped antihydrogen atoms, we determine an experimental bound on the antihydrogen charge, Qe, of |Q| < 0.71 parts per billion (one standard deviation), in which e is the elementary charge. This bound is a factor of 20 less than that determined from the best previous measurement of the antihydrogen charge. The electrical charge of atoms and molecules of normal matter is known to be no greater than about 10(-21)e for a diverse range of species including H2, He and SF6. Charge-parity-time symmetry and quantum anomaly cancellation demand that the charge of antihydrogen be similarly small. Thus, our measurement constitutes an improved limit and a test of fundamental aspects of the Standard Model. If we assume charge superposition and use the best measured value of the antiproton charge, then we can place a new limit on the positron charge anomaly (the relative difference between the positron and elementary charge) of about one part per billion (one standard deviation), a 25-fold reduction compared to the current best measurement.
反物质因其在可观测宇宙中明显缺失而继续引起物理学家的兴趣。目前的理论要求,在大爆炸之后,物质和反物质以相等的数量出现,但粒子物理的标准模型并没有对宇宙的一半似乎消失提供定量解释。最近已经有可能研究被捕获的反氢原子,以寻找可能尚未观察到的物质和反物质物理行为之间的差异。在这里,我们考虑反氢原子的电中性。通过对被捕获的反氢原子施加随机加速,我们确定了反氢电荷 Qe 的实验界限,|Q| < 0.71 个十亿分之一(一个标准差),其中 e 是基本电荷。这个界限比以前对反氢电荷的最佳测量结果低 20 倍。已知正常物质的原子和分子的电荷不大于约 10(-21)e,包括 H2、He 和 SF6 等多种物质。电荷宇称时间对称和量子反常取消要求反氢的电荷也同样小。因此,我们的测量构成了对标准模型基本方面的改进限制和测试。如果我们假设电荷叠加,并使用最佳测量的反质子电荷值,那么我们可以对正电子电荷异常(正电子和基本电荷之间的相对差异)施加新的限制,约为十亿分之一(一个标准差),与当前最佳测量相比降低了 25 倍。