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NAME

       gmx-energy - Writes energies to xvg files and display averages

SYNOPSIS

          gmx energy [-f [<.edr>]] [-f2 [<.edr>]] [-s [<.tpr>]] [-o [<.xvg>]]
                     [-viol [<.xvg>]] [-pairs [<.xvg>]] [-ora [<.xvg>]]
                     [-ort [<.xvg>]] [-oda [<.xvg>]] [-odr [<.xvg>]]
                     [-odt [<.xvg>]] [-oten [<.xvg>]] [-corr [<.xvg>]]
                     [-vis [<.xvg>]] [-ravg [<.xvg>]] [-odh [<.xvg>]]
                     [-b <time>] [-e <time>] [-[no]w] [-xvg <enum>] [-[no]fee]
                     [-fetemp <real>] [-zero <real>] [-[no]sum] [-[no]dp]
                     [-nbmin <int>] [-nbmax <int>] [-[no]mutot] [-skip <int>]
                     [-[no]aver] [-nmol <int>] [-[no]fluct_props]
                     [-[no]driftcorr] [-[no]fluc] [-[no]orinst] [-[no]ovec]
                     [-acflen <int>] [-[no]normalize] [-P <enum>]
                     [-fitfn <enum>] [-beginfit <real>] [-endfit <real>]

DESCRIPTION

       gmx  energy  extracts  energy  components  or  distance  restraint  data from an energy file. The user is
       prompted to interactively select the desired energy terms.

       Average, RMSD, and drift are calculated with full precision from the  simulation  (see  printed  manual).
       Drift  is calculated by performing a least-squares fit of the data to a straight line. The reported total
       drift is the difference of the fit at the first and last point.  An error  estimate  of  the  average  is
       given  based  on a block averages over 5 blocks using the full-precision averages. The error estimate can
       be performed over multiple block lengths with the options -nbmin and -nbmax.  Note that in most cases the
       energy files contains averages over all MD steps, or over many more points than the number of  frames  in
       energy  file.  This makes the gmx energy statistics output more accurate than the .xvg output. When exact
       averages are not present in the energy file, the statistics mentioned above are simply over  the  single,
       per-frame energy values.

       The term fluctuation gives the RMSD around the least-squares fit.

       Some  fluctuation-dependent  properties can be calculated provided the correct energy terms are selected,
       and that the command line option -fluct_props is given. The following properties will be computed:
                              ┌─────────────────────────────────┬─────────────────────┐
                              │ Property                        │ Energy terms needed │
                              ├─────────────────────────────────┼─────────────────────┤
                              │ Heat capacity C_p (NPT sims):   │ Enthalpy, Temp      │
                              ├─────────────────────────────────┼─────────────────────┤
                              │ Heat capacity C_v (NVT sims):   │ Etot, Temp          │
                              ├─────────────────────────────────┼─────────────────────┤
                              │ Thermal expansion coeff. (NPT): │ Enthalpy, Vol, Temp │
                              ├─────────────────────────────────┼─────────────────────┤
                              │ Isothermal compressibility:     │ Vol, Temp           │
                              ├─────────────────────────────────┼─────────────────────┤
                              │ Adiabatic bulk modulus:         │ Vol, Temp           │
                              └─────────────────────────────────┴─────────────────────┘

       You always need to set the number of molecules -nmol.   The  C_p/C_v  computations  do  not  include  any
       corrections for quantum effects. Use the gmx dos program if you need that (and you do).

       When  the -viol option is set, the time averaged violations are plotted and the running time-averaged and
       instantaneous sum of violations are recalculated. Additionally running  time-averaged  and  instantaneous
       distances between selected pairs can be plotted with the -pairs option.

       Options -ora, -ort, -oda, -odr and -odt are used for analyzing orientation restraint data.  The first two
       options  plot  the  orientation,  the last three the deviations of the orientations from the experimental
       values.  The options that end on an 'a' plot the average over  time  as  a  function  of  restraint.  The
       options  that end on a 't' prompt the user for restraint label numbers and plot the data as a function of
       time. Option -odr plots the RMS deviation as a function of restraint.  When the run used time or ensemble
       averaged  orientation  restraints,  option  -orinst  can  be  used  to  analyse  the  instantaneous,  not
       ensemble-averaged orientations and deviations instead of the time and ensemble averages.

       Option  -oten  plots  the  eigenvalues  of  the  molecular  order  tensor  for each orientation restraint
       experiment. With option -ovec also the eigenvectors are plotted.

       Option -odh extracts and plots the free  energy  data  (Hamiltoian  differences  and/or  the  Hamiltonian
       derivative dhdl) from the ener.edr file.

       With -fee an estimate is calculated for the free-energy difference with an ideal gas state:

          Delta A = A(N,V,T) - A_idealgas(N,V,T) = kT ln(<exp(U_pot/kT)>)
          Delta G = G(N,p,T) - G_idealgas(N,p,T) = kT ln(<exp(U_pot/kT)>)

       where  k  is Boltzmann's constant, T is set by -fetemp and the average is over the ensemble (or time in a
       trajectory).  Note that this is in principle only correct  when  averaging  over  the  whole  (Boltzmann)
       ensemble and using the potential energy. This also allows for an entropy estimate using:

          Delta S(N,V,T) = S(N,V,T) - S_idealgas(N,V,T) = (<U_pot> - Delta A)/T
          Delta S(N,p,T) = S(N,p,T) - S_idealgas(N,p,T) = (<U_pot> + pV - Delta G)/T

       When a second energy file is specified (-f2), a free energy difference is calculated:

          dF = -kT ln(<exp(-(E_B-E_A)/kT)>_A) ,

       where  E_A  and  E_B are the energies from the first and second energy files, and the average is over the
       ensemble A. The running average of the free energy difference is printed to a file  specified  by  -ravg.
       Note that the energies must both be calculated from the same trajectory.

OPTIONS

       Options to specify input files:

       -f [<.edr>] (ener.edr)
              Energy file

       -f2 [<.edr>] (ener.edr) (Optional)
              Energy file

       -s [<.tpr>] (topol.tpr) (Optional)
              Portable xdr run input file

       Options to specify output files:

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

       -viol [<.xvg>] (violaver.xvg) (Optional)
              xvgr/xmgr file

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

       -ora [<.xvg>] (orienta.xvg) (Optional)
              xvgr/xmgr file

       -ort [<.xvg>] (orientt.xvg) (Optional)
              xvgr/xmgr file

       -oda [<.xvg>] (orideva.xvg) (Optional)
              xvgr/xmgr file

       -odr [<.xvg>] (oridevr.xvg) (Optional)
              xvgr/xmgr file

       -odt [<.xvg>] (oridevt.xvg) (Optional)
              xvgr/xmgr file

       -oten [<.xvg>] (oriten.xvg) (Optional)
              xvgr/xmgr file

       -corr [<.xvg>] (enecorr.xvg) (Optional)
              xvgr/xmgr file

       -vis [<.xvg>] (visco.xvg) (Optional)
              xvgr/xmgr file

       -ravg [<.xvg>] (runavgdf.xvg) (Optional)
              xvgr/xmgr file

       -odh [<.xvg>] (dhdl.xvg) (Optional)
              xvgr/xmgr file

       Other options:

       -b <time> (0)
              First frame (ps) to read from trajectory

       -e <time> (0)
              Last frame (ps) to read from trajectory

       -[no]w (no)
              View output .xvg, .xpm, .eps and .pdb files

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

       -[no]fee (no)
              Do a free energy estimate

       -fetemp <real> (300)
              Reference temperature for free energy calculation

       -zero <real> (0)
              Subtract a zero-point energy

       -[no]sum (no)
              Sum the energy terms selected rather than display them all

       -[no]dp (no)
              Print energies in high precision

       -nbmin <int> (5)
              Minimum number of blocks for error estimate

       -nbmax <int> (5)
              Maximum number of blocks for error estimate

       -[no]mutot (no)
              Compute the total dipole moment from the components

       -skip <int> (0)
              Skip number of frames between data points

       -[no]aver (no)
              Also print the exact average and rmsd stored in the energy frames (only when 1 term is requested)

       -nmol <int> (1)
              Number of molecules in your sample: the energies are divided by this number

       -[no]fluct_props (no)
              Compute properties based on energy fluctuations, like heat capacity

       -[no]driftcorr (no)
              Useful  only  for  calculations  of  fluctuation  properties. The drift in the observables will be
              subtracted before computing the fluctuation properties.

       -[no]fluc (no)
              Calculate autocorrelation of energy fluctuations rather than energy itself

       -[no]orinst (no)
              Analyse instantaneous orientation data

       -[no]ovec (no)
              Also plot the eigenvectors with -oten

       -acflen <int> (-1)
              Length of the ACF, default is half the number of frames

       -[no]normalize (yes)
              Normalize ACF

       -P <enum> (0)
              Order of Legendre polynomial for ACF (0 indicates none): 0, 1, 2, 3

       -fitfn <enum> (none)
              Fit function: none, exp, aexp, exp_exp, exp5, exp7, exp9

       -beginfit <real> (0)
              Time where to begin the exponential fit of the correlation function

       -endfit <real> (-1)
              Time where to end the exponential fit of the correlation function, -1 is until the end

SEE ALSO

       gmx(1)

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

COPYRIGHT

       2015, GROMACS development team

5.1.2                                           February 03, 2016                                  GMX-ENERGY(1)