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交叉场中氢原子高能区域的经典动力学与共振局域化

Classical dynamics and localization of resonances in the high-energy region of the hydrogen atom in crossed fields.

作者信息

Schweiner Frank, Main Jörg, Cartarius Holger, Wunner Günter

机构信息

Institut für Theoretische Physik 1, Universität Stuttgart, 70550 Stuttgart, Germany.

出版信息

Phys Rev E Stat Nonlin Soft Matter Phys. 2015 Jan;91(1):012915. doi: 10.1103/PhysRevE.91.012915. Epub 2015 Jan 20.

DOI:10.1103/PhysRevE.91.012915
PMID:25679690
Abstract

When superimposing the potentials of external fields on the Coulomb potential of the hydrogen atom, a saddle point (called the Stark saddle point) appears. For energies slightly above the saddle point energy, one can find classical orbits that are located in the vicinity of this point. We follow those so-called quasi-Penning orbits to high energies and field strengths, observing structural changes and uncovering their bifurcation behavior. By plotting the stability behavior of those orbits against energy and field strength, the appearance of a stability apex is reported. A cusp bifurcation, located in the vicinity of the apex, will be investigated in detail. In this cusp bifurcation, another orbit of similar shape is found. This orbit becomes completely stable in the observed region of positive energy, i.e., in a region of parameter space, where the Kepler-like orbits located around the nucleus are already unstable. By quantum mechanically exact calculations, we prove the existence of signatures in quantum spectra belonging to those orbits. Husimi distributions are used to compare quantum-Poincaré sections with the extension of the classical torus structure around the orbits. Since periodic orbit theory predicts that each classical periodic orbit contributes an oscillating term to photoabsorption spectra, we finally give an estimation for future experiments, which could verify the existence of the stable orbits.

摘要

当将外场的势叠加到氢原子的库仑势上时,会出现一个鞍点(称为斯塔克鞍点)。对于略高于鞍点能量的能量,可以找到位于该点附近的经典轨道。我们追踪这些所谓的准彭宁轨道到高能量和场强,观察结构变化并揭示它们的分岔行为。通过绘制这些轨道的稳定性行为与能量和场强的关系图,报告了一个稳定性顶点的出现。将详细研究位于顶点附近的尖点分岔。在这个尖点分岔中,发现了另一个形状相似的轨道。这个轨道在观测到的正能量区域,即在参数空间的一个区域内变得完全稳定,在该区域中围绕原子核的类开普勒轨道已经不稳定。通过量子力学精确计算,我们证明了属于这些轨道的量子光谱中特征的存在。胡西米分布用于将量子庞加莱截面与围绕轨道的经典环面结构的扩展进行比较。由于周期轨道理论预测每个经典周期轨道对光吸收光谱贡献一个振荡项,我们最终对未来的实验给出了一个估计,这些实验可以验证稳定轨道的存在。

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