Parametrization ========================================================= Fit to Experimental Data ------------------------ Parameters can be fit for one component at a time, and as many parameters as desired *can* be fit. Input file structure is very similar to before with the mandatory addition of an ``optimization_parameters`` section whose presence will signify to DESPASITO that this is a fitting job. Here we summarize the available experimental data types that are currently supported for fitting, followed by the description of the main fitting function containing more details. .. automodule:: despasito.parameter_fitting :members: .. _data-types: Available Data Types ------------------------ .. currentmodule:: despasito.parameter_fitting.data_classes .. autosummary:: :toctree: _autosummary flash.Data liquid_density.Data saturation_properties.Data solubility_parameter.Data TLVE.Data Supporting Thermodynamic Functions ------------------------------------------------ .. currentmodule:: despasito.parameter_fitting .. autosummary:: :toctree: _autosummary fit_functions global_methods constraint_types Estimate with Electronic Structure Methods ------------------------------------------ In SAFT, self-interaction parameters are often fit to experimental data, and in most cases so are the cross-interaction parameters (between segments of different types). In a work nearing publication, we derived combining rules extended to utilize multipole moments of molecular fragments from density functional theory (DFT) methods using R.E.D. server `[1]`_. Once the multipole moments of molecular fragments are obtained, the temperature dependent parameters can be directly predicted in DESAPSITO with the package, `MAPSCI `_, as a plug-in. Alternatively, the parameters could be estimated with MAPSCI separately and fine tuned to be independent of temperature in an iterative fashion. _`[1]` Vanquelef, E.; Simon, S.; Marquant, G.; Garcia, E.; Klimerak, G.; Delepine, J. C.; Cieplak, P.; Dupradeau, F.-Y. R.E.D. Server: A Web Service for Deriving RESP and ESP Charges and Building Force Field Libraries for New Molecules and Molecular Fragments. Nucleic Acids Res. 2011, 39 (suppl_2), W511–W517. https://doi.org/10.1093/nar/gkr288