Direct measurement of the energy thresholds to conformational isomerization in Tryptamine: Experiment and theory

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The methods of stimulated emission pumping-hole filling spectroscopy (SEP-HFS) and stimulated emission pumping population transfer spectroscopy (SEP-PTS) were applied to the conformation-specific study of conformational isomerization in tryptamine [TRA, 3-(2-aminoethyl)indole]. These experimental methods employ stimulated emission pumping to selectively excite a fraction of the population of a single conformation of TRA to well-defined ground-state vibrational levels. This produces single conformations with well-defined internal energy, tunable over a range of energies from near the zero-point level to well above the lowest barriers to conformational isomerization. When the SEP step overcomes a barrier to isomerization, a fraction of the excited population isomerizes to form that product. By carrying out SEP excitation early in a supersonic expansion, these product molecules are subsequently cooled to their zero-point vibrational levels, where they can be detected downstream with a third tunable laser that probes the ground-state population of a particular product conformer via a unique ultraviolet transition using laser-induced fluorescence. The population transfer spectra (recorded by tuning the SEP dump laser while holding the pump and probe lasers fixed) exhibit sharp onsets that directly determine the energy thresholds for conformational isomerization in a given reactant-product conformer pair. In the absence of tunneling effects, the first observed transition in a given X–Y PTS constitutes an upper bound to the energy barrier to conformational isomerization, while the last transition not observed constitutes a lower bound. The bounds for isomerizing conformer A of tryptamine to B(688–748  cm^–1), C(1)(860–1000  cm^–1), C(2)(1219–1316  cm^–1), D(1219–1282  cm^–1), E(1219–1316  cm^–1), and F(688–748  cm^–1) are determined. In addition, thresholds for isomerizing from B to A(<1562  cm^–1), B to F(562–688  cm^–1), and out of C(2) to B(<747  cm^–1) are also determined. The AB and BA transitions are used to place bounds on the relative energies of minima B relative to A, with B lying at least 126  cm^–1 above A. The corresponding barriers have been computed using both density functional and second-order many-body perturbation theory methods in order to establish the level of theory needed to reproduce experimental results. While most of the computed barriers match experiment well, the barriers for the A–F and B–F transitions are too high by almost a factor of 2. Possible reasons for this discrepancy are discussed. ©2005 American Institute of Physics