Lorentzian Linewidth in Chili
Posted: Thu Jan 21, 2016 4:34 pm
Hey all,
If I understand correctly, chili should be compatible with the MOMD approach (http://www.sciencedirect.com/science/ar ... 5896901138) described by Budil et. al. However, they describe a Lorentzian linewidth tensor -- Wxx, Wyy, and Wzz in their notation -- which is distinct from the lw or lwpp option in chili:
Does anyone know whether fitting for these parameters is possible, or whether there is a way to account for them using chili?
If I understand correctly, chili should be compatible with the MOMD approach (http://www.sciencedirect.com/science/ar ... 5896901138) described by Budil et. al. However, they describe a Lorentzian linewidth tensor -- Wxx, Wyy, and Wzz in their notation -- which is distinct from the lw or lwpp option in chili:
I haven't been able to find this anywhere in EasySpin, but it seems clear from experimental data (for instance, from the spectra fitted in this paper http://www.nature.com/nmat/journal/v13/ ... at3979.pdf) that this variable can change substantially, and can have a significant influence on the simulation results.In addition to the explicit magnetic interactions of the electronic and nuclear spins, it is possible to specify two types of orientation-dependent inhomogeneous broadening: (a) a linewidth tensor W associated with the magnetic frame from rigid-limit spectra and (b) the varying only the dynamic and ordering parameters in the quantities Delta (0) and Delta (2) that specify an added homogeneous linewidth Delta
Does anyone know whether fitting for these parameters is possible, or whether there is a way to account for them using chili?