JILA, National Institute of Standards and Technology, University of Colorado and Department of Chemistry and Biochemistry, University of Colorado at Boulder, Boulder, Colorado 80309, USA.
Service de Chimie Quantique et Photophysique, Université Libre de Bruxelles, 50 av. F.D. Roosevelt, CP 160/09, 1050 Brussels, Belgium.
J Chem Phys. 2017 Mar 14;146(10):104204. doi: 10.1063/1.4977061.
Vibrationally state selective overtone spectroscopy and dynamics of weakly bound Ne-HO complexes (D = 31.67 cm, D = 34.66 cm) are reported for the first time, based on near infrared excitation of van der Waals cluster bands correlating with v = 2 ← 0 overtone transitions (|02⟩←|00⟩ and |02⟩←|00⟩) out of the ortho (1) and para (0) internal rotor states of the HO moiety. Quantum theoretical calculations for nuclear motion on a high level ab initio potential energy surface (CCSD(T)/VnZ-f12 (n = 3,4), corrected for basis set superposition error and extrapolated to the complete basis set limit) are employed for assignment of Σ←Σ,Π←Σ, and Σ←Π infrared bands in the overtone spectra, where Σ(K = 0) and Π (K = 1) represent approximate projections (K) of the body angular momentum along the Ne-HO internuclear axis. End-over-end tumbling of the ortho Ne-HO cluster is evident via rotational band contours observed, with band origins and rotational progressions in excellent agreement with ab initio frequency and intensity predictions. A clear Q branch in the corresponding |02⟩Π(1)←Σ(0) para Ne-HO spectrum provides evidence for a novel e/f parity-dependent metastability in these weakly bound clusters, in agreement with ab initio bound state calculations and attributable to the symmetry blocking of an energetically allowed channel for internal rotor predissociation. Finally, Boltzmann analysis of the rotational spectra reveals anomalously low jet temperatures (T ≈ 4(1) K), which are attributed to "evaporative cooling" of weakly bound Ne-HO clusters and provide support for similar cooling dynamics in rare gas-tagging studies.
首次报道了弱束缚 Ne-HO 复合物(D = 31.67 cm,D = 34.66 cm)的振动态选择泛频光谱和动力学,基于范德华团簇带的近红外激发,与 v = 2 → 0 泛频跃迁(|02⟩←|00⟩ 和 |02⟩←|00⟩)相关联,这些跃迁来自 HO 部分的正(1)和仲(0)内转子态的正交(1)和仲(0)内转子态。对于核运动,采用高水平从头算势能表面上的量子理论计算(CCSD(T)/VnZ-f12(n = 3,4),校正了基组超支误差并外推到完全基组极限),用于分配Σ←Σ、Π←Σ和Σ←Π 红外带在泛频光谱中,其中Σ(K = 0)和Π(K = 1)代表体角动量沿着 Ne-HO 核间轴的近似投影(K)。通过观察到的旋转带轮廓,可以明显看出仲 Ne-HO 团簇的首尾翻转,带起源和旋转进展与从头算频率和强度预测非常吻合。在相应的|02⟩Π(1)←Σ(0)仲 Ne-HO 光谱中存在明显的 Q 支,这为这些弱束缚团簇中存在新型 e/f 奇偶依赖的亚稳性提供了证据,这与从头算束缚态计算一致,归因于内部转子预解离的能量允许通道的对称阻塞。最后,旋转光谱的玻尔兹曼分析揭示了异常低的射流温度(T ≈ 4(1)K),这归因于弱束缚 Ne-HO 团簇的“蒸发冷却”,并为稀有气体标记研究中的类似冷却动力学提供了支持。