3D-RISM Molecular Reconstruction ================================ This directory includes input files to produce water and thermodynamic distributions around Factor Xa with 3D-RISM and the resulting output files. Both site and molecular distributions are produced. Running the script ------------------ Output files may be reproduced using the `run.sh` script. The script requires AmberTool 19.4 or higher and for `$AMBERHOME` to be set. By default, the script will run on a single core. To run in parallel, ensure that AmberTools has been build with the `-mpi` and `-rism` options and that the `$DO_PARALLEL` environment variable has been set. E.g., export DO_PARALLEL='mpiexec -np 4' Input files ----------- The input files are `fxa-strip.parm7` : The Amber parameter/topology file for factor Xa. `fxa-strip.nc` : An Amber NetCDF trajectory file for factor Xa. Contains only one frame. `fxa-strip.pdb` : A PDB coordinate file for factor Xa. `cTIP3P_pse3.xvv` : 1D-RISM XVV file for cTIP3 water using the PSE-3 closure. Output files ------------ The primary output file is `rism.out` : Primary output file for `rism3d.snglpnt`. It contains all of the settings, timings, memory use, and global solvation thermodynamic values. The remaining outputfiles are volumetric distribution files, named according to the following format: ... ### `` One of `g` : Pair distribution function. `g_dT` : Temperature derivative fo the pair distribution function. `exchem` : The excess chemical potential. `solvEne` : The total solvation energy. `potUV` : The solute-solvent potential energy. `entropy` : Solvation -T∆S. ### `` Maybe the the solvent site name (e.g., `O` or `H1`), sum of all solvent sites (omitted), or `mol` for the molecular reconstruction. ### `` Always '1' in this examples. ### `` The [DX format](https://www.ks.uiuc.edu/Research/vmd/plugins/molfile/dxplugin.html) is used in all cases and specified by 'dx'.