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NAME

       gmx-wham - Perform weighted histogram analysis after umbrella sampling

SYNOPSIS

          gmx wham [-ix [<.dat>]] [-if [<.dat>]] [-it [<.dat>]] [-ip [<.dat>]]
                   [-is [<.dat>]] [-iiact [<.dat>]] [-tab [<.dat>]]
                   [-o [<.xvg>]] [-hist [<.xvg>]] [-oiact [<.xvg>]]
                   [-bsres [<.xvg>]] [-bsprof [<.xvg>]] [-xvg <enum>]
                   [-min <real>] [-max <real>] [-[no]auto] [-bins <int>]
                   [-temp <real>] [-tol <real>] [-[no]v] [-b <real>]
                   [-e <real>] [-dt <real>] [-[no]histonly] [-[no]boundsonly]
                   [-[no]log] [-unit <enum>] [-zprof0 <real>] [-[no]cycl]
                   [-[no]sym] [-[no]ac] [-acsig <real>] [-ac-trestart <real>]
                   [-nBootstrap <int>] [-bs-method <enum>] [-bs-tau <real>]
                   [-bs-seed <int>] [-histbs-block <int>] [-[no]vbs]

DESCRIPTION

       gmx  wham  is  an  analysis  program that implements the Weighted Histogram Analysis Method (WHAM). It is
       intended to analyze output files generated by umbrella sampling simulations to  compute  a  potential  of
       mean force (PMF).

       gmx  wham  is  currently  not  fully  up  to  date.  It  only  supports  pull setups where the first pull
       coordinate(s) is/are umbrella pull coordinates and, if multiple coordinates need to be analyzed, all used
       the same geometry and dimensions. In most cases this is not an issue.

       At present, three input modes are supported.

       • With  option  -it,  the  user  provides a file which contains the file names of the umbrella simulation
         run-input files (.tpr files), AND, with option -ix, a file which contains file names of the pullx mdrun
         output  files. The .tpr and pullx files must be in corresponding order, i.e. the first .tpr created the
         first pullx, etc.

       • Same as the previous input mode, except that the  user  provides  the  pull  force  output  file  names
         (pullf.xvg)  with  option -if.  From the pull force the position in the umbrella potential is computed.
         This does not work with tabulated umbrella potentials.

       • With option -ip, the user provides file names of (gzipped) .pdo files, i.e.  the GROMACS  3.3  umbrella
         output  files.  If  you have some unusual reaction coordinate you may also generate your own .pdo files
         and feed them with the -ip option into to gmx wham. The  .pdo  file  header  must  be  similar  to  the
         following:

            # UMBRELLA      3.0
            # Component selection: 0 0 1
            # nSkip 1
            # Ref. Group 'TestAtom'
            # Nr. of pull groups 2
            # Group 1 'GR1'  Umb. Pos. 5.0 Umb. Cons. 1000.0
            # Group 2 'GR2'  Umb. Pos. 2.0 Umb. Cons. 500.0
            #####

         The  number  of  pull  groups,  umbrella  positions, force constants, and names may (of course) differ.
         Following the header, a time  column  and  a  data  column  for  each  pull  group  follows  (i.e.  the
         displacement with respect to the umbrella center). Up to four pull groups are possible per .pdo file at
         present.

       By default, all pull coordinates found in all pullx/pullf files are used in WHAM. If  only  some  of  the
       pull  coordinates  should  be  used,  a  pull coordinate selection file (option -is) can be provided. The
       selection file must contain one line for each tpr file  in  tpr-files.dat.   Each  of  these  lines  must
       contain  one  digit  (0  or 1) for each pull coordinate in the tpr file.  Here, 1 indicates that the pull
       coordinate is used in WHAM, and 0 means it is omitted.  Example:  If  you  have  three  tpr  files,  each
       containing  4 pull coordinates, but only pull coordinates 1 and 2 should be used, coordsel.dat looks like
       this:

          1 1 0 0
          1 1 0 0
          1 1 0 0

       By default, the output files are:

          ``-o``      PMF output file
          ``-hist``   Histograms output file

       Always check whether the histograms sufficiently overlap.

       The umbrella potential is assumed to be harmonic and the force constants are read from the .tpr  or  .pdo
       files. If a non-harmonic umbrella force was applied a tabulated potential can be provided with -tab.

   WHAM options-bins   Number of bins used in analysis

       • -temp   Temperature in the simulations

       • -tol    Stop iteration if profile (probability) changed less than tolerance

       • -auto   Automatic determination of boundaries

       • -min,-max   Boundaries of the profile

       The  data  points  that  are  used to compute the profile can be restricted with options -b, -e, and -dt.
       Adjust -b to ensure sufficient equilibration in each umbrella window.

       With -log (default) the profile is written in energy units, otherwise (with -nolog) as  probability.  The
       unit can be specified with -unit.  With energy output, the energy in the first bin is defined to be zero.
       If you want the free energy at a different position to be zero, set -zprof0 (useful  with  bootstrapping,
       see below).

       For  cyclic  or periodic reaction coordinates (dihedral angle, channel PMF without osmotic gradient), the
       option -cycl is useful.  gmx wham will make use of the periodicity of the system and generate a  periodic
       PMF. The first and the last bin of the reaction coordinate will assumed be be neighbors.

       Option -sym symmetrizes the profile around z=0 before output, which may be useful for, e.g. membranes.

   Parallelization
       If  available,  the  number  of  OpenMP  threads  used  by  gmx  wham  can  be  controlled by setting the
       OMP_NUM_THREADS environment variable.

   Autocorrelations
       With -ac, gmx wham estimates the integrated autocorrelation time (IACT) tau for each umbrella window  and
       weights the respective window with 1/[1+2*tau/dt]. The IACTs are written to the file defined with -oiact.
       In verbose mode, all autocorrelation functions (ACFs) are  written  to  hist_autocorr.xvg.   Because  the
       IACTs  can be severely underestimated in case of limited sampling, option -acsig allows one to smooth the
       IACTs along the reaction coordinate with a Gaussian (sigma provided with -acsig, see output in iact.xvg).
       Note  that  the IACTs are estimated by simple integration of the ACFs while the ACFs are larger 0.05.  If
       you prefer to compute the IACTs by a more sophisticated (but possibly less robust) method such as fitting
       to a double exponential, you can compute the IACTs with gmx analyze and provide them to gmx wham with the
       file iact-in.dat (option -iiact), which should contain one line per input file (.pdo or pullx/f file) and
       one column per pull coordinate in the respective file.

   Error analysis
       Statistical  errors may be estimated with bootstrap analysis. Use it with care, otherwise the statistical
       error may be substantially underestimated.  More background and examples for the bootstrap technique  can
       be found in Hub, de Groot and Van der Spoel, JCTC (2010) 6: 3713-3720.  -nBootstrap defines the number of
       bootstraps (use, e.g., 100).  Four bootstrapping methods are supported and selected with -bs-method.

       • b-hist   Default: complete histograms are considered as independent data points, and the  bootstrap  is
         carried  out by assigning random weights to the histograms ("Bayesian bootstrap"). Note that each point
         along the reaction coordinate must be covered by multiple independent histograms (e.g. 10  histograms),
         otherwise the statistical error is underestimated.

       • hist     Complete  histograms  are  considered  as  independent  data  points.   For  each bootstrap, N
         histograms are randomly chosen from the N given histograms (allowing duplication,  i.e.  sampling  with
         replacement).   To  avoid  gaps  without  data  along  the  reaction  coordinate  blocks  of histograms
         (-histbs-block) may be defined. In that case, the given histograms are divided  into  blocks  and  only
         histograms  within  each  block  are  mixed.  Note  that  the  histograms  within  each  block  must be
         representative for all possible histograms, otherwise the statistical error is underestimated.

       • traj  The given histograms are used to generate new random trajectories, such that the  generated  data
         points  are distributed according the given histograms and properly autocorrelated. The autocorrelation
         time (ACT) for each window must be known, so use -ac or provide the ACT with -iiact. If the ACT of  all
         windows  are  identical (and known), you can also provide them with -bs-tau.  Note that this method may
         severely underestimate the error in case of limited sampling, that is if individual histograms  do  not
         represent the complete phase space at the respective positions.

       • traj-gauss   The  same  as  method  traj,  but  the trajectories are not bootstrapped from the umbrella
         histograms but from Gaussians with the average and width of the umbrella histograms. That method yields
         similar error estimates like method traj.

       Bootstrapping output:

       • -bsres   Average profile and standard deviations

       • -bsprof  All bootstrapping profiles

       With  -vbs  (verbose  bootstrapping),  the  histograms of each bootstrap are written, and, with bootstrap
       method traj, the cumulative distribution functions of the histograms.

OPTIONS

       Options to specify input files:

       -ix [<.dat>] (pullx-files.dat) (Optional)
              Generic data file

       -if [<.dat>] (pullf-files.dat) (Optional)
              Generic data file

       -it [<.dat>] (tpr-files.dat) (Optional)
              Generic data file

       -ip [<.dat>] (pdo-files.dat) (Optional)
              Generic data file

       -is [<.dat>] (coordsel.dat) (Optional)
              Generic data file

       -iiact [<.dat>] (iact-in.dat) (Optional)
              Generic data file

       -tab [<.dat>] (umb-pot.dat) (Optional)
              Generic data file

       Options to specify output files:

       -o [<.xvg>] (profile.xvg)
              xvgr/xmgr file

       -hist [<.xvg>] (histo.xvg)
              xvgr/xmgr file

       -oiact [<.xvg>] (iact.xvg) (Optional)
              xvgr/xmgr file

       -bsres [<.xvg>] (bsResult.xvg) (Optional)
              xvgr/xmgr file

       -bsprof [<.xvg>] (bsProfs.xvg) (Optional)
              xvgr/xmgr file

       Other options:

       -xvg <enum> (xmgrace)
              xvg plot formatting: xmgrace, xmgr, none

       -min <real> (0)
              Minimum coordinate in profile

       -max <real> (0)
              Maximum coordinate in profile

       -[no]auto (yes)
              Determine min and max automatically

       -bins <int> (200)
              Number of bins in profile

       -temp <real> (298)
              Temperature

       -tol <real> (1e-06)
              Tolerance

       -[no]v (no)
              Verbose mode

       -b <real> (50)
              First time to analyse (ps)

       -e <real> (1e+20)
              Last time to analyse (ps)

       -dt <real> (0)
              Analyse only every dt ps

       -[no]histonly (no)
              Write histograms and exit

       -[no]boundsonly (no)
              Determine min and max and exit (with -auto)

       -[no]log (yes)
              Calculate the log of the profile before printing

       -unit <enum> (kJ)
              Energy unit in case of log output: kJ, kCal, kT

       -zprof0 <real> (0)
              Define profile to 0.0 at this position (with -log)

       -[no]cycl (no)
              Create cyclic/periodic profile. Assumes min and max are the same point.

       -[no]sym (no)
              Symmetrize profile around z=0

       -[no]ac (no)
              Calculate integrated autocorrelation times and use in wham

       -acsig <real> (0)
              Smooth autocorrelation times along reaction coordinate with Gaussian of this sigma

       -ac-trestart <real> (1)
              When computing autocorrelation functions, restart computing every .. (ps)

       -nBootstrap <int> (0)
              nr of bootstraps to estimate statistical uncertainty (e.g., 200)

       -bs-method <enum> (b-hist)
              Bootstrap method: b-hist, hist, traj, traj-gauss

       -bs-tau <real> (0)
              Autocorrelation time (ACT) assumed for all histograms. Use option -ac if ACT is unknown.

       -bs-seed <int> (-1)
              Seed for bootstrapping. (-1 = use time)

       -histbs-block <int> (8)
              When mixing histograms only mix within blocks of -histbs-block.

       -[no]vbs (no)
              Verbose bootstrapping. Print the CDFs and a histogram file for each bootstrap.

SEE ALSO

       gmx(1)

       More information about GROMACS is available at <http://www.gromacs.org/>.

COPYRIGHT

       2020, GROMACS development team