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Create input files with polarisable force field for OpenMM

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paduagroup/pol_openmm

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CL&Pol force field in xml format for use with OpenMM

These tools follow the same procedure as in paduagroup/clandpol to create input files for polarizable simulations, so for more detailed information check the instructions there.

Attention: please use with a recent version of fftool (no older than 02/2024) since there were some changes in the format of the xml files.

Creating Input Files

  1. Use fftool and packmol as usual, only in the second round give the -x --type options:

     fftool 200 ch.xyz 200 Cl.zmat 400 EG.zmat -b 55
     packmol < pack.inp
     fftool 200 ch.xyz 200 Cl.zmat 400 EG.zmat -b 55 -x --type
    

    This creates field.xml and config.pdb.

  2. Add Drude particles using the polxml script (analogous to the polarizer script from paduagroup/clandpol). Supposing an alpha.ff force field file describing the Drude parameters is present, run

     polxml
    

    This creates files field-p.xml and config-p.pdb with Drude particles added after each core and the necessary force field terms. These files should run with OpenMM.

  3. If necessary scale the LJ potentials, for which the fragment database fragment.ff and fragment molecular files are required (in this example the additional meoh.zmat for the fragments of ethyleneglycol). A frag.inp file specifying which atoms belong to which fragments needs to be prepared. The identification is by atom name:

     # frag.inp for ChCl:EG
     ch N4 C1 C1A COL H1 HC OH
     cl Cl 
     meoh CTO OHG H1O
    

    Then run

     scaleLJxml
    

    will generate field-p-sc.xml

  4. Tun OpenMM using the field-p-sc.xml and config-p.pdb as force field and topology. Since Drude particles are already present in config-p.pdb, it is not necessary to add Drude particles in the OpenMM script, although it should also be possible to use the initial config.pdb and have OpenMM add Drude particles with modeller.addExtraParticles(forcefield).

  5. If necessary add Coulomb damping between charges and induced dipoles. This is often required to avoid the polarization catastrophe in systems with strong hydrogen bonds or densely-charged ions. The following script creates OpenMM code implementing the Tang-Toennies damping function:

     coulttxml field-p.xml config-p.pdb
    

The code generated is to be included in the OpenMM script (the atoms involved have to be identified).

Some points worth mentioning

The fragment input file is different from the one for use with LAMMPS

This is unfortunate when using the scaleLJxml script. It happens because LAMMPS uses numerical atom type IDs, so the fragment.inp input file for scaling LJ parameters in LAMMPS input files has to use atom type numbers. In xml input files the atom types are character strings, therefore the two tools are not perfectly compatible in terms of input specification.

Unique atom names and types

The --type option of fftool creates unique atom types (within the entire system), as required by OpenMM to set Drude particle-core pairs. The unique atom type is composed from 3 characters from the molecule (residue) name, plus the atom name (non-bonded type), plus a serial number. Drude particles will get a preceding D-. As a consequence of using the unique atom types, the non-bonded types of the force field are used as the atom class (instead of the bonded types), which causes some redundancies in the bonded terms.

Within each residue the atom name is composed of the chemical element plus a serial number if more than 1 atom of the same element are present. These have to be unique within a residue because they are used to specify bonds. This is the CHARMM convention, quite different from the OPLS one that we use mostly. We suppose it is also used by TRAVIS. In order to circumvent the limits of the PDB format (4 characters for the atom name), 32-decimal notation is used for the serial number in very large molecules or materials (which are considered as a single molecule).

Choice of Drude thermostat (and OpenMM version)

Although the TGNH thermostat is certainly superior, we couldn't make it work with our xml force field files, which run fine in the latest OpenMM versions. There may be bugs or incomplete implementations in OpenMM 7.4.2.

The authors of the TGNH should update it to a more recent version of OpenMM. We think that reverse engineering the force field formats for our systems to run with TGNH in OpenMM 7.4.2 is not worth the effort.

As a result, we would favour using the standard Drude dual thermostats that come with vanilla OpenMM. Maybe these are not the very best but they should be ok for equilibrium quantities (but maybe not ideal for transport properties). Anyway, this is what almost everyone else is using.

Another point is that the Langevin integrators can be considerably faster than Nosé-Hoover, also in their Drude versions. The Langevin are stochastic and not reliable for transport properties, but should be ok for equilibrium quantities.

Temperatures

The Drude integrators in OpenMM don't compute the temperatures of atoms and Drude particles (relative to cores) and show a global temperature that is lower than the set point. The temperatures corresponding to atoms and Drude particles have to be computed separately by the user (as shown in the omm.py script).

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Create input files with polarisable force field for OpenMM

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