This is part of the bias module |
Used to performed Parallel Bias metadynamics.
This action activate Parallel Bias Metadynamics (PBMetaD) [85], a version of metadynamics [64] in which multiple low-dimensional bias potentials are applied in parallel. In the current implementation, these have the form of mono-dimensional metadynamics bias potentials:
\[ {V(s_1,t), ..., V(s_N,t)} \]
where:
\[ V(s_i,t) = \sum_{ k \tau < t} W_i(k \tau) \exp\left( - \frac{(s_i-s_i^{(0)}(k \tau))^2}{2\sigma_i^2} \right). \]
To ensure the convergence of each mono-dimensional bias potential to the corresponding free energy, at each deposition step the Gaussian heights are multiplied by the so-called conditional term:
\[ W_i(k \tau)=W_0 \frac{\exp\left( - \frac{V(s_i,k \tau)}{k_B T} \right)}{\sum_{i=1}^N \exp\left( - \frac{V(s_i,k \tau)}{k_B T} \right)} \]
where \(W_0\) is the initial Gaussian height.
The PBMetaD bias potential is defined by:
\[ V_{PB}(\vec{s},t) = -k_B T \log{\sum_{i=1}^N \exp\left( - \frac{V(s_i,t)}{k_B T} \right)}. \]
Information on the Gaussian functions that build each bias potential are printed to multiple HILLS files, which are used both to restart the calculation and to reconstruct the mono-dimensional free energies as a function of the corresponding CVs. These can be reconstructed using the sum_hills utility because the final bias is given by:
\[ V(s_i) = -F(s_i) \]
Currently, only a subset of the METAD options are available in PBMetaD.
The bias potentials can be stored on a grid to increase performances of long PBMetaD simulations. You should provide either the number of bins for every collective variable (GRID_BIN) or the desired grid spacing (GRID_SPACING). In case you provide both PLUMED will use the most conservative choice (highest number of bins) for each dimension. In case you do not provide any information about bin size (neither GRID_BIN nor GRID_SPACING) and if Gaussian width is fixed PLUMED will use 1/5 of the Gaussian width as grid spacing. This default choice should be reasonable for most applications.
Another option that is available is well-tempered metadynamics [11]. In this variant of PBMetaD the heights of the Gaussian hills are scaled at each step by the additional well-tempered metadynamics term. This ensures that each bias converges more smoothly. It should be noted that, in the case of well-tempered metadynamics, in the output printed the Gaussian height is re-scaled using the bias factor. Also notice that with well-tempered metadynamics the HILLS files do not contain the bias, but the negative of the free-energy estimate. This choice has the advantage that one can restart a simulation using a different value for the \(\Delta T\). The applied bias will be scaled accordingly.
Note that you can use here also the flexible Gaussian approach [25] in which you can adapt the Gaussian to the extent of Cartesian space covered by a variable or to the space in collective variable covered in a given time. In this case the width of the deposited Gaussian potential is denoted by one value only that is a Cartesian space (ADAPTIVE=GEOM) or a time (ADAPTIVE=DIFF). Note that a specific integration technique for the deposited Gaussian kernels should be used in this case. Check the documentation for utility sum_hills.
With the keyword INTERVAL one changes the metadynamics algorithm setting the bias force equal to zero outside boundary [10]. If, for example, metadynamics is performed on a CV s and one is interested only to the free energy for s > boundary, the history dependent potential is still updated according to the above equations but the metadynamics force is set to zero for s < boundary. Notice that Gaussian kernels are added also if s < boundary, as the tails of these Gaussian kernels influence VG in the relevant region s > boundary. In this way, the force on the system in the region s > boundary comes from both metadynamics and the force field, in the region s < boundary only from the latter. This approach allows obtaining a history-dependent bias potential VG that fluctuates around a stable estimator, equal to the negative of the free energy far enough from the boundaries. Note that:
For systems with multiple CVs that share identical properties, PBMetaD with partitioned families can be used to group them under one bias potential that each contributes to [93]. This is done with a list of PF keywords, where each PF* argument contains the list of CVs from ARG to be placed in that family. Once invoked, each CV in ARG must be placed in exactly one PF, even if it results in families containing only one CV. Additionally, in cases where each of SIGMA or GRID entry would correspond to each ARG entry, they now correspond to each PF and must be adjusted accordingly.
Multiple walkers [95] can also be used. See below the examples.
The following input is for PBMetaD calculation using as collective variables the distance between atoms 3 and 5 and the distance between atoms 2 and 4. The value of the CVs and the PBMetaD bias potential are written to the COLVAR file every 100 steps.
d1: DISTANCEATOMS=3,5 d2: DISTANCEthe pair of atom that we are calculating the distance between.ATOMS=2,4 pb: PBMETADthe pair of atom that we are calculating the distance between.ARG=d1,d2compulsory keyword the labels of the scalars on which the bias will actSIGMA=0.2,0.2compulsory keyword the widths of the Gaussian hillsHEIGHT=0.3the height of the Gaussian hills, one for all biases.PACE=500compulsory keyword the frequency for hill addition, one for all biasesFILE=HILLS_d1,HILLS_d2 PRINTfiles in which the lists of added hills are stored, default names are assigned using arguments if FILE is not foundARG=d1,d2,pb.biascompulsory keyword the labels of the values that you would like to print to the fileSTRIDE=100compulsory keyword ( default=1 ) the frequency with which the quantities of interest should be outputFILE=COLVARthe name of the file on which to output these quantities
(See also DISTANCE and PRINT).
d1: DISTANCEATOMS=3,5 d2: DISTANCEthe pair of atom that we are calculating the distance between.ATOMS=2,4 pb: PBMETAD ...the pair of atom that we are calculating the distance between.ARG=d1,d2compulsory keyword the labels of the scalars on which the bias will actSIGMA=0.2,0.2compulsory keyword the widths of the Gaussian hillsHEIGHT=0.3the height of the Gaussian hills, one for all biases.PACE=500compulsory keyword the frequency for hill addition, one for all biasesBIASFACTOR=8use well tempered metadynamics with this bias factor, one for all biases.FILE=HILLS_d1,HILLS_d2 ... PRINTfiles in which the lists of added hills are stored, default names are assigned using arguments if FILE is not foundARG=d1,d2,pb.biascompulsory keyword the labels of the values that you would like to print to the fileSTRIDE=100compulsory keyword ( default=1 ) the frequency with which the quantities of interest should be outputFILE=COLVARthe name of the file on which to output these quantities
d1: DISTANCEATOMS=3,5 d2: DISTANCEthe pair of atom that we are calculating the distance between.ATOMS=2,4 d3: DISTANCEthe pair of atom that we are calculating the distance between.ATOMS=1,2 pb: PBMETAD ...the pair of atom that we are calculating the distance between.ARG=d1,d2,d3compulsory keyword the labels of the scalars on which the bias will actSIGMA=0.2,0.2compulsory keyword the widths of the Gaussian hillsHEIGHT=0.3the height of the Gaussian hills, one for all biases.PF0=d1specify which CVs belong in a partitioned family.PF1=d2,d3specify which CVs belong in a partitioned family.PACE=500compulsory keyword the frequency for hill addition, one for all biasesBIASFACTOR=8use well tempered metadynamics with this bias factor, one for all biases.FILE=HILLS_d1,HILLS_d2 ... PRINTfiles in which the lists of added hills are stored, default names are assigned using arguments if FILE is not foundARG=d1,d2,d3,pb.biascompulsory keyword the labels of the values that you would like to print to the fileSTRIDE=100compulsory keyword ( default=1 ) the frequency with which the quantities of interest should be outputFILE=COLVARthe name of the file on which to output these quantities
d1: DISTANCEATOMS=3,5 d2: DISTANCEthe pair of atom that we are calculating the distance between.ATOMS=2,4 pb: PBMETAD ...the pair of atom that we are calculating the distance between.ARG=d1,d2compulsory keyword the labels of the scalars on which the bias will actSIGMA=0.2,0.2compulsory keyword the widths of the Gaussian hillsHEIGHT=0.3the height of the Gaussian hills, one for all biases.PACE=500compulsory keyword the frequency for hill addition, one for all biasesBIASFACTOR=8use well tempered metadynamics with this bias factor, one for all biases.FILE=HILLS_d1,HILLS_d2files in which the lists of added hills are stored, default names are assigned using arguments if FILE is not foundWALKERS_MPI... PRINT( default=off ) Switch on MPI version of multiple walkers - not compatible with WALKERS_* options other than WALKERS_DIRARG=d1,d2,pb.biascompulsory keyword the labels of the values that you would like to print to the fileSTRIDE=100compulsory keyword ( default=1 ) the frequency with which the quantities of interest should be outputFILE=COLVARthe name of the file on which to output these quantities
d1: DISTANCEwhere WALKERS_N is the total number of walkers, WALKERS_ID is the id of the present walker (starting from 0 ) and the WALKERS_DIR is the directory where all the walkers are located. WALKERS_RSTRIDE is the number of step between one update and the other.ATOMS=3,5 d2: DISTANCEthe pair of atom that we are calculating the distance between.ATOMS=2,4 pb: PBMETAD ...the pair of atom that we are calculating the distance between.ARG=d1,d2compulsory keyword the labels of the scalars on which the bias will actSIGMA=0.2,0.2compulsory keyword the widths of the Gaussian hillsHEIGHT=0.3the height of the Gaussian hills, one for all biases.PACE=500compulsory keyword the frequency for hill addition, one for all biasesBIASFACTOR=8use well tempered metadynamics with this bias factor, one for all biases.FILE=HILLS_d1,HILLS_d2files in which the lists of added hills are stored, default names are assigned using arguments if FILE is not foundWALKERS_N=10number of walkersWALKERS_ID=3walker idWALKERS_DIR=../shared directory with the hills files from all the walkersWALKERS_RSTRIDE=100 ... PRINTstride for reading hills filesARG=d1,d2,pb.biascompulsory keyword the labels of the values that you would like to print to the fileSTRIDE=100compulsory keyword ( default=1 ) the frequency with which the quantities of interest should be outputFILE=COLVARthe name of the file on which to output these quantities
By default this Action calculates the following quantities. These quantities can be referenced elsewhere in the input by using this Action's label followed by a dot and the name of the quantity required from the list below.
Quantity | Description |
bias | the instantaneous value of the bias potential |
ARG | the labels of the scalars on which the bias will act |
SIGMA | the widths of the Gaussian hills |
PACE | the frequency for hill addition, one for all biases |
NUMERICAL_DERIVATIVES | ( default=off ) calculate the derivatives for these quantities numerically |
GRID_SPARSE | ( default=off ) use a sparse grid to store hills |
GRID_NOSPLINE | ( default=off ) don't use spline interpolation with grids |
WALKERS_MPI | ( default=off ) Switch on MPI version of multiple walkers - not compatible with WALKERS_* options other than WALKERS_DIR |
FILE | files in which the lists of added hills are stored, default names are assigned using arguments if FILE is not found |
HEIGHT | the height of the Gaussian hills, one for all biases. Compulsory unless TAU, TEMP and BIASFACTOR are given |
FMT | specify format for HILLS files (useful for decrease the number of digits in regtests) |
BIASFACTOR | use well tempered metadynamics with this bias factor, one for all biases. Please note you must also specify temp |
TEMP | the system temperature - this is only needed if you are doing well-tempered metadynamics |
TAU | in well tempered metadynamics, sets height to (k_B Delta T*pace*timestep)/tau |
GRID_MIN | the lower bounds for the grid |
GRID_MAX | the upper bounds for the grid |
GRID_BIN | the number of bins for the grid |
GRID_SPACING | the approximate grid spacing (to be used as an alternative or together with GRID_BIN) |
GRID_WSTRIDE | frequency for dumping the grid |
GRID_WFILES | dump grid for the bias, default names are used if GRID_WSTRIDE is used without GRID_WFILES. |
GRID_RFILES | read grid for the bias |
ADAPTIVE | use a geometric (=GEOM) or diffusion (=DIFF) based hills width scheme. Sigma is one number that has distance units or timestep dimensions |
SIGMA_MAX | the upper bounds for the sigmas (in CV units) when using adaptive hills. Negative number means no bounds |
SIGMA_MIN | the lower bounds for the sigmas (in CV units) when using adaptive hills. Negative number means no bounds |
PF | specify which CVs belong in a partitioned family. Once a PF is specified, all CVs in ARG must be placed in a PF even if there is one CV per PF”. You can use multiple instances of this keyword i.e. PF1, PF2, PF3... |
SELECTOR | add forces and do update based on the value of SELECTOR |
SELECTOR_ID | value of SELECTOR |
WALKERS_ID | walker id |
WALKERS_N | number of walkers |
WALKERS_DIR | shared directory with the hills files from all the walkers |
WALKERS_RSTRIDE | stride for reading hills files |
INTERVAL_MIN | one dimensional lower limits, outside the limits the system will not feel the biasing force. |
INTERVAL_MAX | one dimensional upper limits, outside the limits the system will not feel the biasing force. |
RESTART | allows per-action setting of restart (YES/NO/AUTO) |
UPDATE_FROM | Only update this action from this time |
UPDATE_UNTIL | Only update this action until this time |