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In the case of L-Phe, the calculated stability of conformers was highly dependent on the calculation level. In addition, there was discrepancy between the band intensity in the electronic spectra and the relative stability calculated. As shown in ref 6, conformer A of L-Phe was calculated to be the ninth and fifth most stable structure at the B3LYP/6-31+G* and MP2/6-311G** levels, respectively. However, in the electronic spectra, the band of conformer A appears quite strongly; the intensity is much stronger than that estimated from Boltzmann distribution at 418 K ref 6, This enhanced band intensity for conformer A of L-Phe may be due to some factors other than population of conformers, such as enhanced probability of electronic transitions for conformer A. For L-Tyr, on the contrary, the LIF spectra show strong bands of conformers B-n and X-n, which are predicted to be the most stable in DFT calculations. Therefore, it is reasonable to assign vibronic bands o
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In the case of L-Phe, the calculated stability of conformers was highly dependent on the calculation level. In addition, there was discrepancy between the band intensity in the electronic spectra and the relative stability calculated. As shown in ref 6, conformer A of L-Phe was calculated to be the ninth and fifth most stable structure at the B3LYP/6-31+G* and MP2/6-311G** levels, respectively. However, in the electronic spectra, the band of conformer A appears quite strongly; the intensity is much stronger than that estimated from Boltzmann distribution at 418 K (ref 6). This enhanced band intensity for conformer A of L-Phe may be due to some factors other than population of conformers, such as enhanced probability of electronic transitions for conformer A. For L-Tyr, on the contrary, the LIF spectra show strong bands of conformers B-n and X-n, which are predicted to be the most stable in DFT calculations. Therefore, it is reasonable to assign vibronic bands of L-Tyr on the basis of the total energy of stable conformers calculated at the B3LYP/6-31+G* level.
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