SETI Institute, 189 Bernardo Avenue, Suite 100, Mountain View, California 94043, USA.
J Chem Phys. 2013 Aug 28;139(8):084313. doi: 10.1063/1.4819069.
The interstellar presence of protonated nitrous oxide has been suspected for some time. Using established high-accuracy quantum chemical techniques, spectroscopic constants and fundamental vibrational frequencies are provided for the lower energy O-protonated isomer of this cation and its deuterated isotopologue. The vibrationally-averaged B0 and C0 rotational constants are within 6 MHz of their experimental values and the D(J) quartic distortion constants agree with experiment to within 3%. The known gas phase O-H stretch of NNOH(+) is 3330.91 cm(-1), and the vibrational configuration interaction computed result is 3330.9 cm(-1). Other spectroscopic constants are also provided, as are the rest of the fundamental vibrational frequencies for NNOH(+) and its deuterated isotopologue. This high-accuracy data should serve to better inform future observational or experimental studies of the rovibrational bands of protonated nitrous oxide in the interstellar medium and the laboratory.
一段时间以来,人们一直怀疑星际空间中存在质子化一氧化二氮。使用成熟的高精度量子化学技术,为这种阳离子的低能 O-质子化异构体及其氘代同位素提供了光谱常数和基本振动频率。振动平均的 B0 和 C0 转动常数与实验值相差在 6MHz 以内,D(J)四次离解常数与实验值相差在 3%以内。已知 NNOH(+)的气相 O-H 伸缩振动为 3330.91cm(-1),计算出的振动构型相互作用结果为 3330.9cm(-1)。还提供了其他光谱常数,以及 NNOH(+)及其氘代同位素的其他基本振动频率。这些高精度数据应该有助于更好地了解星际介质中质子化一氧化二氮的转动带的未来观测或实验研究以及实验室研究。