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This range is limited to the fitting of the ensemble line shape only, and a larger range of -1100 to 1100 cm-1 is used for the integration of the FRET and MC-FRET rate expressions
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g. Once the emission lineshape is stored, the line shapes for other values of the energy can be obtained by shifting the reference value only.
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There is a typo in the unit definition related to scaling factor in the Figure 2 caption of this paper, ℏ = 1 should read as h = 1.
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Kimura and Kakitani in ref 48 also used different spectral densities with longer tails and bumps in the high frequency phonon modes, which seems necessary for the understanding of the experimental rates for mutuants with large energy bias (data points e and f in their Figure 1). This shows that the use of more accurate spectral densities including high frequency phonon modes may be necessary for satisfactory theoretical description of all the experimental data in ref 23 even if we include the effect of back transfer reactions.
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Kimura and Kakitani in ref 48 also used different spectral densities with longer tails and bumps in the high frequency phonon modes, which seems necessary for the understanding of the experimental rates for mutuants with large energy bias (data points e and f in their Figure 1). This shows that the use of more accurate spectral densities including high frequency phonon modes may be necessary for satisfactory theoretical description of all the experimental data in ref 23 even if we include the effect of back transfer reactions.
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