1988
DOI: 10.1021/j100330a025
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High-resolution interferometric Fourier transform infrared absorption spectroscopy in supersonic free jet expansions: carbon monoxide, nitric oxide, methane, ethyne, propyne, and trifluoromethane

Abstract: DMABN by two-color time-of-flight mass spectrometry (TOFMS). This has revealed absorption features due to two isomeric 1:1 DMABN-H20 complexes, one with AP = 14 cm"1 (also observed in LIF) and one with Ap = 199 cm"1 which was not observed in LIF but predominates in TOFMS. A DMABN-(H20)2 complex, invisible by LIF, was also found, with Ap = 401 cm"1. This work provides direct evidence of the existence of nonfluorescent DMABN-solvent complexes and supports the (40) Warren,

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Cited by 143 publications
(84 citation statements)
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“…As can be seen from figure 4, the final simulations of the spectra provide an excellent agreement between experiment and simulation. The rotational temperatures for the best simulations are about 2 K. As this corresponds to (kT/hc) > 1 cm -1 >> A _~ B > C, even this low temperature is somewhat too high to observe effects arising from nuclear spin symmetry conservation in the supersonic jet expansion [42,43]. In figure 4 we also show a simulation for a rotational temperature of 1.5 K which does not show a dramatically poorer agreement with the experimental spectrum.…”
Section: Resultsmentioning
confidence: 76%
“…As can be seen from figure 4, the final simulations of the spectra provide an excellent agreement between experiment and simulation. The rotational temperatures for the best simulations are about 2 K. As this corresponds to (kT/hc) > 1 cm -1 >> A _~ B > C, even this low temperature is somewhat too high to observe effects arising from nuclear spin symmetry conservation in the supersonic jet expansion [42,43]. In figure 4 we also show a simulation for a rotational temperature of 1.5 K which does not show a dramatically poorer agreement with the experimental spectrum.…”
Section: Resultsmentioning
confidence: 76%
“…Absorption spectra of methane cooled down to 77 K using cooled cells could already be investigated in several spectral regions [5][6][7][8][9][10][11][12], thanks to the important available vapor pressure (~10 Torr). Further cooling was also achieved by means of supersonic expansions [11,[13][14][15][16][17][18][19]. Though important, these achievements remain insufficient to allow an exhaustive and global modeling of the individual line parameters below 1.7 µm.…”
Section: Introductionmentioning
confidence: 99%
“…Of course, similar to the setup with our Bomem spectrometer, [16] one can also build an interface with a supersonic jet system. [14] The FTIR spectrum of the molecules presented here have been recorded in the region 600-3600 cm À1 . The instrumental resolution, defined by 1/MOPD (maximum optical path difference) ranged from 0.001-0.002 cm…”
mentioning
confidence: 99%