Department of Physics, University of California, Berkeley, California, USA.
Phys Chem Chem Phys. 2011 Nov 14;13(42):19125-41. doi: 10.1039/c1cp21317b. Epub 2011 Aug 1.
We show that weakly bound He-containing van der Waals molecules can be produced and magnetically trapped in buffer-gas cooling experiments, and provide a general model for the formation and dynamics of these molecules. Our analysis shows that, at typical experimental parameters, thermodynamics favors the formation of van der Waals complexes composed of a helium atom bound to most open-shell atoms and molecules, and that complex formation occurs quickly enough to ensure chemical equilibrium. For molecular pairs composed of a He atom and an S-state atom, the molecular spin is stable during formation, dissociation, and collisions, and thus these molecules can be magnetically trapped. Collisional spin relaxation is too slow to affect trap lifetimes. However, (3)He-containing complexes can change spin due to adiabatic crossings between trapped and untrapped Zeeman states, mediated by the anisotropic hyperfine interaction, causing trap loss. We provide a detailed model for Ag(3)He molecules, using ab initio calculation of Ag-He interaction potentials and spin interactions, quantum scattering theory, and direct Monte Carlo simulations to describe formation and spin relaxation in this system. The calculated rate of spin-change agrees quantitatively with experimental observations, providing indirect evidence for molecular formation in buffer-gas-cooled magnetic traps. Finally, we discuss the possibilities for spectroscopic detection of these complexes, including a calculation of expected spectra for Ag(3)He, and report on our spectroscopic search for Ag(3)He, which produced a null result.
我们证明,弱束缚含氦范德华分子可以在缓冲气体冷却实验中产生并被磁捕获,并提供了这些分子形成和动力学的一般模型。我们的分析表明,在典型的实验参数下,热力学有利于形成由氦原子与大多数开壳原子和分子形成的范德华复合物,并且复合物的形成速度足够快以确保化学平衡。对于由氦原子和 S 态原子组成的分子对,分子自旋在形成、解离和碰撞过程中是稳定的,因此这些分子可以被磁捕获。碰撞自旋弛豫太慢,不会影响陷阱寿命。然而,(3)He 含复合物可以由于各向异性超精细相互作用介导的捕获和未捕获的塞曼态之间的绝热交叉而改变自旋,导致陷阱损失。我们提供了 Ag(3)He 分子的详细模型,使用从头算计算 Ag-He 相互作用势能和自旋相互作用、量子散射理论和直接蒙特卡罗模拟来描述该体系中的形成和自旋弛豫。计算的自旋变化速率与实验观察结果定量一致,为缓冲气体冷却磁阱中分子形成提供了间接证据。最后,我们讨论了这些复合物的光谱检测可能性,包括 Ag(3)He 的预期光谱计算,并报告了我们对 Ag(3)He 的光谱搜索,结果为零。