Write files suitable for other programs. Available filetypes are marvin, thbrel, xtl, xr, cssr, arc
xyz, trajectory, history, fdf, drv, frc and phonon:
marvin - generates a file suitable for input to Marvin for
surface calculations. Index of surface plane needs to be
added first, though this may be passed through GULP to the
marvin input but using the "marvin" option. If the file
extension ".mvn" is not given by the user it will be added
by the program.
e.g. output marvin alumina produces alumina.mvn
thbrel - converts the final bulk structure into a file format
suitable for the THBREL suite of programs. Not all features
are readily transferable between the programs so no guarantee
is made that the input file is perfect and for similar reasons
both programs may not always yield the same results unless the
user is careful to make sure the files are equivalent. If a
phonon run has been requested then the output is modified for
THBPHON instead of THBREL.
xtl - this is only applicable to crystal structures with a
single structure per file. Produces a .xtl file for input
into the BIOSYM software, though use of the archive file is
better unless symmetry is present. If the filename input is
not already terminated with ".xtl" then this will be added
by the program.
e.g. output xtl alumina produces alumina.xtl
xr - this will output a modified CSSR file suitable for
input into the Oxford Materials graphical interface
program Crysalis. The file will have the extension ".xr"
added. At the moment this is only applicable to 3D
systems.
e.g. output xr alumina produces alumina.xr
cssr - this will output a CSSR file suitable for input
into the MSI graphical interface Cerius2. The file will
have the extension ".cssr" added. At the moment this
is only applicable to 3D systems.
e.g. output cssr alumina produces alumina.cssr
arc - alternatively known as a ".car" file. This option produces
archive files suitable for input into the BIOSYM Insight software
and will handle bulk, cluster and defect calculations, all with
multiple structures. The username should input a root name,
e.g. output arc alumina
The program will then produce archive file names with either
"_bulk", "_defe", or "_clus" appended to distinguish the files
resulting from a particular section of the run. If multiple
structures are present then an underscore followed by the
structure number will be added, all followed by ".arc".
e.g. if the above input for alumina contained two bulk structures
then the files produced would be "alumina_bulk_1.arc" and
"alumina_bulk_2.arc".
If the word "movie" is specified then all structures during an
optimisation will be included in the arcfile, rather than just
the final one, so that the optimisation may be viewed.
e.g. output movie arc alumina
Note : for MD runs the name of the archive file is set by
"mdarchive" to avoid overwriting the optimisation archive
file if present.
xyz - this will output an xyz file suitable for
input into programs such as Molden and with slight
modification Unichem. The file will have the extension ".xyz"
At the moment this is only applicable to non-periodic
systems. When called with a periodic case just the Cartesian
coordinates will be output, without the unit cell.
e.g. output xyz cluster produces cluster.xyz
If the word "movie" is specified then all structures during an
optimisation will be included in the xyz file, rather than just
the final one, so that the optimisation may be viewed.
e.g. output movie xyz cluster
trajectory - this is a binary file which stores the coordinates
and velocities from a molecular dynamics run, as well as some
of the system properties. This file is used by the Cerius interface
to generate a .trj file for analysis in Cerius
e.g. output trajectory alumina
history - this is a text file in the DLPOLY HISTORY file format
containing the structure and velocities sampled from a MD run.
This file can be used for post-MD analysis using the same
programs as for DLPOLY such as "After".
fdf - this is a text file in the Flexible Data Format of Alberto
Garcia and Jose M. Soler. This file can then form the basis of
an input deck for the program SIESTA.
drv - this is a text file containing the energy and appropriate
derivatives calculated by GULP at the last function evaluation.
This can be used for QM/MM schemes.
frc - this is a text file containing the energy and appropriate
force constants for cores only calculated by GULP during a phonon
calculation. This can be used for QM/MM schemes, such as in the
program QMPOT. A phonon calculation must be specified otherwise
no file will be output.
phonon - this option leads to the density of states from a
phonon calculation and any dispersion curve points being
output to the files <filename>.dens and <filename>.disp,
respectively, in a format suitable for input into a curve
plotting program.
frequency - this option produces a list of frequencies over all
k points for use in an analysis program. A typical application
might be in the calculation of the Gruneisen parameter by
differencing of the frequencies with respect to the cell volume.
The file can either be output in binary format (to maintain
precision - the default):
e.g. output freq binary <filename>
or as ordinary text:
e.g. output freq text <filename>
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