A Rydberg impurity in a dense background gas (Conference Presentation)

T. Liebisch, Michael Schlagmüller, F. Engel, Karl M. Westphal, K. Kleinbach, F. Böttcher, R. Loew, S. Hofferberth, T. Pfau, J. Pérez-Ríos, C. Greene
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Abstract

A single Rydberg atom impurity excited in a BEC is a system that can be utilized to measure the quantum mechanical properties of electron - neutral scattering andthe electron probability density of a Rydberg atom. The Rydberg electron – neutral atom scattering process, is a fundamental scattering process, which can be described via Fermi’s pseudopotential as V{vec{r},vec{R} )=2pi textit{a}[k(R)]delta^{(3)}(vec{r}-vec{R}). The scattering length is dependent on the momentum of the Rydberg electron, and therefore is dependent on the separation of the Rydberg electron from the ion core. At the classical outermost turning point of the electron, it has the slowest momentum leading to s-wave dominated scattering potentials 10’s of MHz in depth for n<40 (Greene et al. PRL 85 2458 (2000), Bendkowsky et al. PRL 105 163201 (2010)). In alkali atoms there is a shape resonance for p-wave scattering, which becomes relevant at ion-neutral separations of ~75nm (I.I. Fabrikant J.Phys B 19, 1527 (1985)). This shape resonance potential is several GHz deep, spanning the energy level spacing between n and n-1 principal quantum numbers. At high BEC densities of 5x10^14cm-3 the nearest neighbor spacing is less than 70nm. A Rydberg atom excited within a BEC, is an excitation of the Rydberg atom and all N neutral atoms located within the Rydberg orbit, described as nS+N x 5S. The nS+N x 5S state is density shifted from the Rydberg resonance. Not only does the distribution of atoms within the Rydberg orbit lead to a density shift, but, at these high densities, atoms excited in the nS+N x 5S state near the shape resonance potential cause large perturbations to the density shift, leading to a line broadening. Therefore the spectroscopic line shape of a Rydberg atom in a BEC allows us to probe the theoretically calculated p-wave shape resonance potential. Furthermore, we can observe and measure the dynamics of neutrals excited in the nS+N x 5S state. In the ultracold regime of a BEC, the background neutral atoms within the Rydberg orbit have kinetic energies of a few kHz, and experience large forces due to the GHz-deep shape resonance potentials. An atom dragged into this deep potential leads to an exothermic state-changing collision. We measure the timescale of this state-changing collision and compare to semi-classical calculations of the neutral atoms evolving in the potential of the two-particle nS+ 5S system. We also measure the change in energy from the original nS state to the product state, (n-4)L (L<3). On time scales shorter than the state-changing collisions, which for n<100 is on the order of 10 microseconds, the neutral atoms will evolve and collect in the shallower electron-neutral potentials, which mimic the electron probability density of the Rydberg atom.With n<100, the Rydberg atom has a diameter greater than 2 micrometers. With an imaging system with <1 micrometer resolution, we expect to observe a macroscopic change in the density profile of the BEC indicating an nS versus nD Rydberg state. The BEC would serve as a contrast agent for observing textbook atomic wavefunctions (Karpiuk et al. New Journal of Physics 17, 053046 (2015)).
致密背景气体中的里德伯杂质(会议报告)
在BEC中激发的单个里德伯原子杂质是一个可以用来测量电子中性散射的量子力学性质和里德伯原子的电子概率密度的系统。Rydberg电子-中性原子散射过程是一种基本散射过程,可以用费米赝势描述为V{vec{r},vec{r})=2pi textit{a}[k(r)]delta^{(3)}(vec{r}-vec{r})。散射长度取决于里德堡电子的动量,因此取决于里德堡电子与离子核的分离。在电子的经典最外层转折点,它具有最慢的动量,导致n<40时s波主导的散射势深度为10兆赫兹(Greene等)。中华科学杂志,2004(2),中国科学院院刊。PRL 105 163201(2010))。在碱原子中存在p波散射的形状共振,这在~75nm的离子中性分离处变得相关(I.I. Fabrikant J.Phys B 19, 1527(1985))。这种形状的共振电位是几GHz深,跨越n和n-1主量子数之间的能级间隔。在5 × 10^14cm-3的高BEC密度下,最近邻间距小于70nm。在BEC中被激发的里德伯原子,是里德伯原子和位于里德伯轨道内的所有N个中性原子的激发,描述为nS+N x 5S。nS+N x 5S态是由里德伯共振引起的密度偏移。不仅里德伯轨道内原子的分布导致了密度位移,而且,在这些高密度下,在形状共振势附近的nS+N x 5S态激发的原子对密度位移造成了大的扰动,导致了谱线的展宽。因此,在BEC中,里德伯原子的谱线形状允许我们探测理论计算的p波形状共振势。此外,我们还可以观察和测量在nS+N x 5S状态下激发的中性粒子的动力学。在BEC的超冷状态下,Rydberg轨道内的背景中性原子具有几kHz的动能,并且由于ghz深形状共振电位而受到较大的力。一个原子被拖入如此深的势能中,就会引发一场改变状态的放热碰撞。我们测量了这种状态改变碰撞的时间尺度,并与双粒子nS+ 5S系统中中性原子演化的半经典计算进行了比较。我们还测量了从原始nS态到产物态的能量变化,(n-4)L (L<3)。在比状态改变碰撞更短的时间尺度上,对于n<100大约是10微秒,中性原子将进化并聚集在较浅的电子中性电位中,这模仿了里德伯原子的电子概率密度。当n<100时,里德伯原子的直径大于2微米。在分辨率小于1微米的成像系统中,我们期望观察到BEC密度分布的宏观变化,表明nS与nD的里德伯态。BEC将作为对比剂用于观察教科书中的原子波函数(Karpiuk et al.)。物理学报17,05 - 03(2015)。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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