Procedures | <Prev Next> |
A basic level of a non-Boltzmann population distribution is available through setting the vibrational temperature, Tvib, which affects the relative populations of different vibronic states, or the spin temperature Tspin.
For more control there are two possible methods; to use a different functional form than the simple Boltzmann equation; see Custom Populations for how to do this. Alternatively, the populations of each level can be specified individually, for uses such as simulating double resonance spectra or nascent population distributions following reactions. It is also possible to fit these populations to measured intensities or band contours, as the populations are simply parameters that can be floated as any other; see the sections on Line Intensity Fitting and Contour Fitting. This process can also be used to simulate and fit time of flight or kinetic energy release spectra; use IntensityUnits = PopDist to ignore transition moments and just plot energy levels with populations derived as described in this section. Plots against velocity (in units of cm-1/2), rather than energy can be obtained by Setting PlotUnits to sqrtcm1.