Institut für Ionenphysik und Angewandte Physik, Universität Innsbruck, Technikerstraße 25, 6020 Innsbruck, Austria.
Department of Physics, University of Central Florida, 4111 Libra Drive, Physical Sciences Building 430, Orlando, Florida 32816-2385, USA.
Phys Rev Lett. 2018 Jun 22;120(25):253003. doi: 10.1103/PhysRevLett.120.253003.
Rotational transitions of the nonlinear triatomic molecular anion NH_{2}^{-} have been observed by terahertz spectroscopy in a cryogenic radio frequency ion trap. Absorption of terahertz photons has been probed by rotational state-dependent photodetachment of the trapped negative ions near the detachment threshold. Using this two-photon scheme, the two lowest rotational transitions for the asymmetric top rotor NH_{2}^{-} have been found. For the para nuclear spin configuration, the 1_{0}←0_{0} transition frequency was determined to be 933 954(2) MHz, and for the ortho configuration the 1_{+1}←1_{-1} transition frequency was determined to be 447 375(3) MHz. This result appears to preclude the recent tentative assignment of an interstellar absorption feature to NH_{2}^{-}.
通过在低温射频离子阱中进行太赫兹光谱学研究,观察到了非线性三原子分子阴离子 NH_{2}^{-}的转动跃迁。通过在离解阈值附近的囚禁负离子的转动态相关光电离探测太赫兹光子的吸收。使用这种双光子方案,发现了非对称转子 NH_{2}^{-}的两个最低转动跃迁。对于顺磁核自旋构型,确定 1_{0}←0_{0}跃迁频率为 933 954(2) MHz,对于反磁核自旋构型,确定 1_{+1}←1_{-1}跃迁频率为 447 375(3) MHz。这一结果似乎排除了最近对星际吸收特征归因于 NH_{2}^{-}的推测。