Electronic spectroscopy of the A1A" <--> X1A' system of CDBr |
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Authors: | Tao Chong Deselnicu Mihaela Mukarakate Calvin Reid Scott A |
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Institution: | Department of Chemistry, Marquette University, Milwaukee, Wisconsin 53201-1881, USA. |
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Abstract: | We report fluorescence excitation and single vibronic level emission spectra of jet-cooled CDBr in the 450-750 nm region. A total of 32 cold bands involving the pure bending levels 2(0)n with n=3-10 and combination bands 2(0)n3(0)1 (n=2-10), 2(0)n3(0)2 (n=2-9), 1(0)(1)2(0)n (n=7-10), and 1(0)(1)2(0)n3(0)(1) (n=6,8-9) in the A1A" <-- X1A' system of this carbene were observed; most of these are reported and/or rotationally analyzed here for the first time. Rotational analysis yielded band origins and effective (B) rotational constants for both bromine isotopomers (CD79Br and CD81Br). The derived A1A" vibrational intervals are combined with results of Yu et al. J. Chem. Phys. 115, 5433 (2001)] to derive barriers to linearity for the 2n, 2n3(1), and 2n3(2) progressions. The A1A" state C-D stretching frequency (2350 cm(-1)) is determined for the first time, in excellent agreement with theory, as are the 79Br-81Br isotope splittings in the excited state. Our emission spectra probe the vibrational structure of the X1A' and a3A" states up to approximately 9000 cm(-1) above the vibrationless level of the X1A' state; the total number of levels observed is around twice that previously reported. Unlike CHBr, where even the lowest bending levels are perturbed by spin-orbit interaction with the triplet origin, the term energy of every level save one below 3000 cm(-1) in CDBr is reproduced by a Dunham expansion to within a standard deviation of 1 cm(-1), and a spin-orbit coupling matrix element of approximately 330 cm(-1) is derived from a deperturbation analysis of the triplet origin. The multireference configuration interaction (MRCI) calculations of Yu et al. J. Chem. Phys. 115, 5433 (2001)] well reproduce triplet perturbations in the pure bending manifold, and globally, the vibrational frequencies of X1A', a3A", and A1A" are in excellent agreement with theoretical predictions. |
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