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<HR>
<H3>10. Modifying & extending LAMMPS
</H3>
<P>LAMMPS is designed in a modular fashion so as to be easy to modify and
extend with new functionality. In fact, about 75% of its source code
is files added in this fashion.
</P>
<P>In this section, changes and additions users can make are listed along
with minimal instructions. If you add a new feature to LAMMPS and
think it will be of interest to general users, we encourage you to
submit it to the developers for inclusion in the released version of
LAMMPS. Information about how to do this is provided
<A HREF = "#package">below</A>.
</P>
<P>The best way to add a new feature is to find a similar feature in
LAMMPS and look at the corresponding source and header files to figure
out what it does. You will need some knowledge of C++ to be able to
understand the hi-level structure of LAMMPS and its class
organization, but functions (class methods) that do actual
computations are written in vanilla C-style code and operate on simple
C-style data structures (vectors and arrays).
</P>
<P>Most of the new features described in this section require you to
write a new C++ derived class (except for exceptions described below,
where you can make small edits to existing files). Creating a new
class requires 2 files, a source code file (*.cpp) and a header file
(*.h). The derived class must provide certain methods to work as a
new option. Depending on how different your new feature is compared
to existing features, you can either derive from the base class
itself, or from a derived class that already exists. Enabling LAMMPS
to invoke the new class is as simple as putting the two source
files in the src dir and re-building LAMMPS.
</P>
<P>The advantage of C++ and its object-orientation is that all the code
and variables needed to define the new feature are in the 2 files you
write, and thus shouldn't make the rest of LAMMPS more complex or
cause side-effect bugs.
</P>
<P>Here is a concrete example. Suppose you write 2 files pair_foo.cpp
and pair_foo.h that define a new class PairFoo that computes pairwise
potentials described in the classic 1997 <A HREF = "#Foo">paper</A> by Foo, et al.
If you wish to invoke those potentials in a LAMMPS input script with a
command like
</P>
<PRE>pair_style foo 0.1 3.5
</PRE>
<P>then your pair_foo.h file should be structured as follows:
</P>
<PRE>#ifdef PAIR_CLASS
PairStyle(foo,PairFoo)
#else
...
(class definition for PairFoo)
...
#endif
</PRE>
<P>where "foo" is the style keyword in the pair_style command, and
PairFoo is the class name defined in your pair_foo.cpp and pair_foo.h
files.
</P>
<P>When you re-build LAMMPS, your new pairwise potential becomes part of
the executable and can be invoked with a pair_style command like the
example above. Arguments like 0.1 and 3.5 can be defined and
processed by your new class.
</P>
<P>As illustrated by this pairwise example, many kinds of options are
referred to in the LAMMPS documentation as the "style" of a particular
command.
</P>
<P>The instructions below give the header file for the base class that
these styles are derived from. Public variables in that file are ones
used and set by the derived classes which are also used by the base
class. Sometimes they are also used by the rest of LAMMPS. Virtual
functions in the base class header file which are set = 0 are ones you
must define in your new derived class to give it the functionality
LAMMPS expects. Virtual functions that are not set to 0 are functions
you can optionally define.
</P>
<P>Additionally, new output options can be added directly to the
thermo.cpp, dump_custom.cpp, and variable.cpp files as explained
below.
</P>
<HR>
<P>Here are additional guidelines for modifying LAMMPS and adding new
functionality:
</P>
<UL><LI>Think about whether what you want to do would be better as a pre- or
post-processing step. Many computations are more easily and more
quickly done that way.
<LI>Don't do anything within the timestepping of a run that isn't
parallel. E.g. don't accumulate a bunch of data on a single processor
and analyze it. You run the risk of seriously degrading the parallel
efficiency.
<LI>If your new feature reads arguments or writes output, make sure you
follow the unit conventions discussed by the <A HREF = "units.html">units</A>
command.
<LI>If you add something you think is truly useful and doesn't impact
LAMMPS performance when it isn't used, send an email to the
<A HREF = "http://lammps.sandia.gov/authors.html">developers</A>. We might be
interested in adding it to the LAMMPS distribution. See further
details on this at the bottom of this page.
</UL>
<HR>
<P>Here are the subsequent topics discussed below, most of which are new
features that can be added in the manner just described:
</P>
10.1 <A HREF = "#mod_1">Atom styles</A><BR>
10.2 <A HREF = "#mod_2">Bond, angle, dihedral, improper potentials</A><BR>
10.3 <A HREF = "#mod_3">Compute styles</A><BR>
10.4 <A HREF = "#mod_4">Dump styles</A><BR>
10.5 <A HREF = "#mod_5">Dump custom output options</A><BR>
10.6 <A HREF = "#mod_6">Fix styles</A> which include integrators, temperature and pressure control, force constraints, boundary conditions, diagnostic output, etc<BR>
10.7 <A HREF = "mod_7">Input script commands</A><BR>
10.8 <A HREF = "#mod_8">Kspace computations</A><BR>
10.9 <A HREF = "#mod_9">Minimization styles</A><BR>
10.10 <A HREF = "#mod_10">Pairwise potentials</A><BR>
10.11 <A HREF = "#mod_11">Region styles</A><BR>
10.12 <A HREF = "#mod_12">Thermodynamic output options</A><BR>
10.13 <A HREF = "#mod_13">Variable options</A><BR>
10.14 <A HREF = "#mod_14">Submitting new features for inclusion in LAMMPS</A> <BR>
<HR>
<HR>
<A NAME = "mod_1"></A><H4>10.1 Atom styles
</H4>
<P>Classes that define an atom style are derived from the Atom class.
The atom style determines what quantities are associated with an atom.
A new atom style can be created if one of the existing atom styles
does not define all the arrays you need to store and communicate with
atoms.
</P>
<P>Atom_vec_atomic.cpp is a simple example of an atom style.
</P>
<P>Here is a brief description of methods you define in your new derived
class. See atom.h for details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >grow</TD><TD > re-allocate atom arrays to longer lengths</TD></TR>
<TR><TD >copy</TD><TD > copy info for one atom to another atom's array locations</TD></TR>
<TR><TD >pack_comm</TD><TD > store an atom's info in a buffer communicated every timestep</TD></TR>
<TR><TD >pack_comm_vel</TD><TD > add velocity info to buffer</TD></TR>
<TR><TD >pack_comm_one</TD><TD > store extra info unique to this atom style</TD></TR>
<TR><TD >unpack_comm</TD><TD > retrieve an atom's info from the buffer</TD></TR>
<TR><TD >unpack_comm_vel</TD><TD > also retrieve velocity info</TD></TR>
<TR><TD >unpack_comm_one</TD><TD > retreive extra info unique to this atom style</TD></TR>
<TR><TD >pack_reverse</TD><TD > store an atom's info in a buffer communicating partial forces</TD></TR>
<TR><TD >pack_reverse_one</TD><TD > store extra info unique to this atom style</TD></TR>
<TR><TD >unpack_reverse</TD><TD > retrieve an atom's info from the buffer</TD></TR>
<TR><TD >unpack_reverse_one</TD><TD > retreive extra info unique to this atom style</TD></TR>
<TR><TD >pack_border</TD><TD > store an atom's info in a buffer communicated on neighbor re-builds</TD></TR>
<TR><TD >pack_border_vel</TD><TD > add velocity info to buffer</TD></TR>
<TR><TD >pack_border_one</TD><TD > store extra info unique to this atom style</TD></TR>
<TR><TD >unpack_border</TD><TD > retrieve an atom's info from the buffer</TD></TR>
<TR><TD >unpack_border_vel</TD><TD > also retrieve velocity info</TD></TR>
<TR><TD >unpack_border_one</TD><TD > retreive extra info unique to this atom style</TD></TR>
<TR><TD >pack_exchange</TD><TD > store all an atom's info to migrate to another processor</TD></TR>
<TR><TD >unpack_exchange</TD><TD > retrieve an atom's info from the buffer</TD></TR>
<TR><TD >size_restart</TD><TD > number of restart quantities associated with proc's atoms</TD></TR>
<TR><TD >pack_restart</TD><TD > pack atom quantities into a buffer</TD></TR>
<TR><TD >unpack_restart</TD><TD > unpack atom quantities from a buffer</TD></TR>
<TR><TD >create_atom</TD><TD > create an individual atom of this style</TD></TR>
<TR><TD >data_atom</TD><TD > parse an atom line from the data file</TD></TR>
<TR><TD >memory_usage</TD><TD > tally memory allocated by atom arrays
</TD></TR></TABLE></DIV>
<P>The constructor of the derived class sets values for several variables
that you must set when defining a new atom style, which are documented
in atom_vec.h. New atom arrays are defined in atom.cpp. Search for
the word "customize" and you will find locations you will need to
modify.
</P>
<HR>
<A NAME = "mod_2"></A><H4>10.2 Bond, angle, dihedral, improper potentials
</H4>
<P>Classes that compute molecular interactions are derived from the Bond,
Angle, Dihedral, and Improper classes. New styles can be created to
add new potentials to LAMMPS.
</P>
<P>Bond_harmonic.cpp is the simplest example of a bond style. Ditto for
the harmonic forms of the angle, dihedral, and improper style
commands.
</P>
<P>Here is a brief description of methods you define in your new derived
bond class. See bond.h, angle.h, dihedral.h, and improper.h for
details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >compute</TD><TD > compute the molecular interactions</TD></TR>
<TR><TD >coeff</TD><TD > set coefficients for one bond type</TD></TR>
<TR><TD >equilibrium_distance</TD><TD > length of bond, used by SHAKE</TD></TR>
<TR><TD >write & read_restart</TD><TD > writes/reads coeffs to restart files</TD></TR>
<TR><TD >single</TD><TD > force and energy of a single bond
</TD></TR></TABLE></DIV>
<HR>
<A NAME = "mod_3"></A><H4>10.3 Compute styles
</H4>
<P>Classes that compute scalar and vector quantities like temperature
and the pressure tensor, as well as classes that compute per-atom
quantities like kinetic energy and the centro-symmetry parameter
are derived from the Compute class. New styles can be created
to add new calculations to LAMMPS.
</P>
<P>Compute_temp.cpp is a simple example of computing a scalar
temperature. Compute_ke_atom.cpp is a simple example of computing
per-atom kinetic energy.
</P>
<P>Here is a brief description of methods you define in your new derived
class. See compute.h for details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >compute_scalar</TD><TD > compute a scalar quantity</TD></TR>
<TR><TD >compute_vector</TD><TD > compute a vector of quantities</TD></TR>
<TR><TD >compute_peratom</TD><TD > compute one or more quantities per atom</TD></TR>
<TR><TD >pack_comm</TD><TD > pack a buffer with items to communicate</TD></TR>
<TR><TD >unpack_comm</TD><TD > unpack the buffer</TD></TR>
<TR><TD >pack_reverse</TD><TD > pack a buffer with items to reverse communicate</TD></TR>
<TR><TD >unpack_reverse</TD><TD > unpack the buffer</TD></TR>
<TR><TD >memory_usage</TD><TD > tally memory usage
</TD></TR></TABLE></DIV>
<HR>
<A NAME = "mod_4"></A><H4>10.4 Dump styles
</H4>
<A NAME = "mod_5"></A><H4>10.5 Dump custom output options
</H4>
<P>Classes that dump per-atom info to files are derived from the Dump
class. To dump new quantities or in a new format, a new derived dump
class can be added, but it is typically simpler to modify the
DumpCustom class contained in the dump_custom.cpp file.
</P>
<P>Dump_atom.cpp is a simple example of a derived dump class.
</P>
<P>Here is a brief description of methods you define in your new derived
class. See dump.h for details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >write_header</TD><TD > write the header section of a snapshot of atoms</TD></TR>
<TR><TD >count</TD><TD > count the number of lines a processor will output</TD></TR>
<TR><TD >pack</TD><TD > pack a proc's output data into a buffer</TD></TR>
<TR><TD >write_data</TD><TD > write a proc's data to a file
</TD></TR></TABLE></DIV>
<P>See the <A HREF = "dump.html">dump</A> command and its <I>custom</I> style for a list of
keywords for atom information that can already be dumped by
DumpCustom. It includes options to dump per-atom info from Compute
classes, so adding a new derived Compute class is one way to calculate
new quantities to dump.
</P>
<P>Alternatively, you can add new keywords to the dump custom command.
Search for the word "customize" in dump_custom.cpp to see the
half-dozen or so locations where code will need to be added.
</P>
<HR>
<A NAME = "mod_6"></A><H4>10.6 Fix styles
</H4>
<P>In LAMMPS, a "fix" is any operation that is computed during
timestepping that alters some property of the system. Essentially
everything that happens during a simulation besides force computation,
neighbor list construction, and output, is a "fix". This includes
time integration (update of coordinates and velocities), force
constraints or boundary conditions (SHAKE or walls), and diagnostics
(compute a diffusion coefficient). New styles can be created to add
new options to LAMMPS.
</P>
<P>Fix_setforce.cpp is a simple example of setting forces on atoms to
prescribed values. There are dozens of fix options already in LAMMPS;
choose one as a template that is similar to what you want to
implement.
</P>
<P>Here is a brief description of methods you can define in your new
derived class. See fix.h for details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >setmask</TD><TD > determines when the fix is called during the timestep</TD></TR>
<TR><TD >init</TD><TD > initialization before a run</TD></TR>
<TR><TD >setup</TD><TD > called immediately before the 1st timestep</TD></TR>
<TR><TD >initial_integrate</TD><TD > called at very beginning of each timestep</TD></TR>
<TR><TD >pre_exchange</TD><TD > called before atom exchange on re-neighboring steps</TD></TR>
<TR><TD >pre_neighbor</TD><TD > called before neighbor list build</TD></TR>
<TR><TD >post_force</TD><TD > called after pair & molecular forces are computed</TD></TR>
<TR><TD >final_integrate</TD><TD > called at end of each timestep</TD></TR>
<TR><TD >end_of_step</TD><TD > called at very end of timestep</TD></TR>
<TR><TD >write_restart</TD><TD > dumps fix info to restart file</TD></TR>
<TR><TD >restart</TD><TD > uses info from restart file to re-initialize the fix</TD></TR>
<TR><TD >grow_arrays</TD><TD > allocate memory for atom-based arrays used by fix</TD></TR>
<TR><TD >copy_arrays</TD><TD > copy atom info when an atom migrates to a new processor</TD></TR>
<TR><TD >memory_usage</TD><TD > report memory used by fix</TD></TR>
<TR><TD >pack_exchange</TD><TD > store atom's data in a buffer</TD></TR>
<TR><TD >unpack_exchange</TD><TD > retrieve atom's data from a buffer</TD></TR>
<TR><TD >pack_restart</TD><TD > store atom's data for writing to restart file</TD></TR>
<TR><TD >unpack_restart</TD><TD > retrieve atom's data from a restart file buffer</TD></TR>
<TR><TD >size_restart</TD><TD > size of atom's data</TD></TR>
<TR><TD >maxsize_restart</TD><TD > max size of atom's data</TD></TR>
<TR><TD >initial_integrate_respa</TD><TD > same as initial_integrate, but for rRESPA</TD></TR>
<TR><TD >post_force_respa</TD><TD > same as post_force, but for rRESPA</TD></TR>
<TR><TD >final_integrate_respa</TD><TD > same as final_integrate, but for rRESPA</TD></TR>
<TR><TD >pack_comm</TD><TD > pack a buffer to communicate a per-atom quantity</TD></TR>
<TR><TD >unpack_comm</TD><TD > unpack a buffer to communicate a per-atom quantity</TD></TR>
<TR><TD >pack_reverse_comm</TD><TD > pack a buffer to reverse communicate a per-atom quantity</TD></TR>
<TR><TD >unpack_reverse_comm</TD><TD > unpack a buffer to reverse communicate a per-atom quantity</TD></TR>
<TR><TD >thermo</TD><TD > compute quantities for thermodynamic output
</TD></TR></TABLE></DIV>
<P>Typically, only a small fraction of these methods are defined for a
particular fix. Setmask is mandatory, as it determines when the fix
will be invoked during the timestep. Fixes that perform time
integration (<I>nve</I>, <I>nvt</I>, <I>npt</I>) implement initial_integrate() and
final_integrate() to perform velocity Verlet updates. Fixes that
constrain forces implement post_force().
</P>
<P>Fixes that perform diagnostics typically implement end_of_step(). For
an end_of_step fix, one of your fix arguments must be the variable
"nevery" which is used to determine when to call the fix and you must
set this variable in the constructor of your fix. By convention, this
is the first argument the fix defines (after the ID, group-ID, style).
</P>
<P>If the fix needs to store information for each atom that persists from
timestep to timestep, it can manage that memory and migrate the info
with the atoms as they move from processors to processor by
implementing the grow_arrays, copy_arrays, pack_exchange, and
unpack_exchange methods. Similarly, the pack_restart and
unpack_restart methods can be implemented to store information about
the fix in restart files. If you wish an integrator or force
constraint fix to work with rRESPA (see the <A HREF = "run_style.html">run_style</A>
command), the initial_integrate, post_force_integrate, and
final_integrate_respa methods can be implemented. The thermo method
enables a fix to contribute values to thermodynamic output, as printed
quantities and/or to be summed to the potential energy of the system.
</P>
<HR>
<A NAME = "mod_7"></A><H4>10.7 Input script commands
</H4>
<P>New commands can be added to LAMMPS input scripts by adding new
classes that have a "command" method. For example, the create_atoms,
read_data, velocity, and run commands are all implemented in this
fashion. When such a command is encountered in the LAMMPS input
script, LAMMPS simply creates a class with the corresponding name,
invokes the "command" method of the class, and passes it the arguments
from the input script. The command method can perform whatever
operations it wishes on LAMMPS data structures.
</P>
<P>The single method your new class must define is as follows:
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >command</TD><TD > operations performed by the new command
</TD></TR></TABLE></DIV>
<P>Of course, the new class can define other methods and variables as
needed.
</P>
<HR>
<A NAME = "mod_8"></A><H4>10.8 Kspace computations
</H4>
<P>Classes that compute long-range Coulombic interactions via K-space
representations (Ewald, PPPM) are derived from the KSpace class. New
styles can be created to add new K-space options to LAMMPS.
</P>
<P>Ewald.cpp is an example of computing K-space interactions.
</P>
<P>Here is a brief description of methods you define in your new derived
class. See kspace.h for details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >init</TD><TD > initialize the calculation before a run</TD></TR>
<TR><TD >setup</TD><TD > computation before the 1st timestep of a run</TD></TR>
<TR><TD >compute</TD><TD > every-timestep computation</TD></TR>
<TR><TD >memory_usage</TD><TD > tally of memory usage
</TD></TR></TABLE></DIV>
<HR>
<A NAME = "mod_9"></A><H4>10.9 Minimization styles
</H4>
<P>Classes that perform energy minimization derived from the Min class.
New styles can be created to add new minimization algorithms to
LAMMPS.
</P>
<P>Min_cg.cpp is an example of conjugate gradient minimization.
</P>
<P>Here is a brief description of methods you define in your new derived
class. See min.h for details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >init</TD><TD > initialize the minimization before a run</TD></TR>
<TR><TD >run</TD><TD > perform the minimization</TD></TR>
<TR><TD >memory_usage</TD><TD > tally of memory usage
</TD></TR></TABLE></DIV>
<HR>
<A NAME = "mod_10"></A><H4>10.10 Pairwise potentials
</H4>
<P>Classes that compute pairwise interactions are derived from the Pair
class. In LAMMPS, pairwise calculation include manybody potentials
such as EAM or Tersoff where particles interact without a static bond
topology. New styles can be created to add new pair potentials to
LAMMPS.
</P>
<P>Pair_lj_cut.cpp is a simple example of a Pair class, though it
includes some optional methods to enable its use with rRESPA.
</P>
<P>Here is a brief description of the class methods in pair.h:
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >compute</TD><TD > workhorse routine that computes pairwise interactions</TD></TR>
<TR><TD >settings</TD><TD > reads the input script line with arguments you define</TD></TR>
<TR><TD >coeff</TD><TD > set coefficients for one i,j type pair</TD></TR>
<TR><TD >init_one</TD><TD > perform initialization for one i,j type pair</TD></TR>
<TR><TD >init_style</TD><TD > initialization specific to this pair style</TD></TR>
<TR><TD >write & read_restart</TD><TD > write/read i,j pair coeffs to restart files</TD></TR>
<TR><TD >write & read_restart_settings</TD><TD > write/read global settings to restart files</TD></TR>
<TR><TD >single</TD><TD > force and energy of a single pairwise interaction between 2 atoms</TD></TR>
<TR><TD >compute_inner/middle/outer</TD><TD > versions of compute used by rRESPA
</TD></TR></TABLE></DIV>
<P>The inner/middle/outer routines are optional.
</P>
<HR>
<A NAME = "mod_11"></A><H4>10.11 Region styles
</H4>
<P>Classes that define geometric regions are derived from the Region
class. Regions are used elsewhere in LAMMPS to group atoms, delete
atoms to create a void, insert atoms in a specified region, etc. New
styles can be created to add new region shapes to LAMMPS.
</P>
<P>Region_sphere.cpp is an example of a spherical region.
</P>
<P>Here is a brief description of methods you define in your new derived
class. See region.h for details.
</P>
<DIV ALIGN=center><TABLE BORDER=1 >
<TR><TD >match</TD><TD > determine whether a point is in the region
</TD></TR></TABLE></DIV>
<HR>
<A NAME = "mod_12"></A><H4>10.12 Thermodynamic output options
</H4>
<P>There is one class that computes and prints thermodynamic information
to the screen and log file; see the file thermo.cpp.
</P>
<P>There are two styles defined in thermo.cpp: "one" and "multi". There
is also a flexible "custom" style which allows the user to explicitly
list keywords for quantities to print when thermodynamic info is
output. See the <A HREF = "thermo_style.html">thermo_style</A> command for a list
of defined quantities.
</P>
<P>The thermo styles (one, multi, etc) are simply lists of keywords.
Adding a new style thus only requires defining a new list of keywords.
Search for the word "customize" with references to "thermo style" in
thermo.cpp to see the two locations where code will need to be added.
</P>
<P>New keywords can also be added to thermo.cpp to compute new quantities
for output. Search for the word "customize" with references to
"keyword" in thermo.cpp to see the several locations where code will
need to be added.
</P>
<P>Note that the <A HREF = "thermo.html">thermo_style custom</A> command already allows
for thermo output of quantities calculated by <A HREF = "fix.html">fixes</A>,
<A HREF = "compute.html">computes</A>, and <A HREF = "variable.html">variables</A>. Thus, it may
be simpler to compute what you wish via one of those constructs, than
by adding a new keyword to the thermo command.
</P>
<HR>
<A NAME = "mod_13"></A><H4>10.13 Variable options
</H4>
<P>There is one class that computes and stores <A HREF = "variable.html">variable</A>
information in LAMMPS; see the file variable.cpp. The value
associated with a variable can be periodically printed to the screen
via the <A HREF = "print.html">print</A>, <A HREF = "fix_print.html">fix print</A>, or
<A HREF = "thermo_style.html">thermo_style custom</A> commands. Variables of style
"equal" can compute complex equations that involve the following types
of arguments:
</P>
<P>thermo keywords = ke, vol, atoms, ...
other variables = v_a, v_myvar, ...
math functions = div(x,y), mult(x,y), add(x,y), ...
group functions = mass(group), xcm(group,x), ...
atom values = x<B>123</B>, y<B>3</B>, vx<B>34</B>, ...
compute values = c_mytemp<B>0</B>, c_thermo_press<B>3</B>, ...
</P>
<P>Adding keywords for the <A HREF = "thermo_style.html">thermo_style custom</A> command
(which can then be accessed by variables) was discussed
<A HREF = "Section_modify.html#thermo">here</A> on this page.
</P>
<P>Adding a new math function of one or two arguments can be done by
editing one section of the Variable::evaulate() method. Search for
the word "customize" to find the appropriate location.
</P>
<P>Adding a new group function can be done by editing one section of the
Variable::evaulate() method. Search for the word "customize" to find
the appropriate location. You may need to add a new method to the
Group class as well (see the group.cpp file).
</P>
<P>Accessing a new atom-based vector can be done by editing one section
of the Variable::evaulate() method. Search for the word "customize"
to find the appropriate location.
</P>
<P>Adding new <A HREF = "compute.html">compute styles</A> (whose calculated values can
then be accessed by variables) was discussed
<A HREF = "Section_modify.html#compute">here</A> on this page.
</P>
<HR>
<HR>
<A NAME = "mod_14"></A><H4>10.14 Submitting new features for inclusion in LAMMPS
</H4>
<P>We encourage users to submit new features that they add to LAMMPS to
<A HREF = "http://lammps.sandia.gov/authors.html">the developers</A>, especially if
you think the features will be of interest to other users. If they
are broadly useful we may add them as core files to LAMMPS or as part
of a <A HREF = "Section_start.html#start_3">standard package</A>. Else we will add
them as a user-contributed package or file. Examples of user packages
are in src sub-directories that start with USER. The USER-MISC
package is simply a collection of (mostly) unrelated single files,
which is the simplest way to have your contribution quickly added to
the LAMMPS distribution. You can see a list of the both standard and
user packages by typing "make package" in the LAMMPS src directory.
</P>
<P>With user packages and files, all we are really providing (aside from
the fame and fortune that accompanies having your name in the source
code and on the <A HREF = "http://lammps.sandia.gov/authors.html">Authors page</A>
of the <A HREF = "http://lammps.sandia.gov">LAMMPS WWW site</A>), is a means for you to distribute your
work to the LAMMPS user community and a mechanism for others to easily
try out your new feature. This may help you find bugs or make contact
with new collaborators. Note that you're also implicitly agreeing to
support your code which means answer questions, fix bugs, and maintain
it if LAMMPS changes.
</P>
<P>The previous sections of this doc page describe how to add new
features of various kinds to LAMMPS. Packages are simply collections
of one or more new class files which are invoked as a new "style"
within a LAMMPS input script. If designed correctly, these additions
do not require changes to the main core of LAMMPS; they are simply
add-on files. If you think your new feature requires non-trivial
changes in core LAMMPS files, you'll need to <A HREF = "http://lammps.sandia.gov/authors.html">communicate with the
developers</A>, since we may or may
not want to make those changes. An example of a trivial change is
making a parent-class method "virtual" when you derive a new child
class from it.
</P>
<P>Here is what you need to do to submit a user package or single file
for our consideration. Following these steps will save time for both
you and us. See existing package files for examples.
</P>
<UL><LI>All source files you provide must compile with the most current
version of LAMMPS.
<LI>If your contribution is a single file (actually a *.cpp and *.h file)
it can most rapidly be added to the USER-MISC directory. Send us the
one-line entry to add to the USER-MISC/README file in that dir, along
with the 2 source files. You can do this multiple times if you wish
to contribute several individual features.
<LI>If your contribution is several related featues, it is probably best
to make it a user package directory with a name like USER-FOO. In
addition to your new files, the directory should contain a README, and
Install.csh file. The README text file should contain your name and
contact information and a brief description of what your new package
does. The Install.csh file enables LAMMPS to include and exclude your
package. See other README and Install.sh files in other USER
directories as examples. Send us a tarball of this USER-FOO
directory.
<LI>Your new source files need to have the LAMMPS copyright, GPL notice,
and your name at the top, like other LAMMPS source files. They need
to create a class that is inside the LAMMPS namespace. Other than
that, your files can do whatever is necessary to implement the new
features. They don't have to be written in the same stylistic format
and syntax as other LAMMPS files, though that would be nice.
<LI>Finally, you must also send a documentation file for each new command
or style you are adding to LAMMPS. This will be one file for a
single-file feature. For a package, it might be several files. These
are simple text files which we will convert to HTML. They must be in
the same format as other *.txt files in the lammps/doc directory for
similar commands and styles. The "Restrictions" section of the doc
page should indicate that your command is only available if LAMMPS is
built with the appropriate USER-MISC or USER-FOO package. See other
user package doc files for an example of how to do this. The txt2html
tool we use to do the conversion can be downloaded from <A HREF = "http://www.sandia.gov/~sjplimp/download.html">this
site</A>, so you can perform
the HTML conversion yourself to proofread your doc page.
</UL>
<P>Note that the more clear and self-explanatory you make your doc and
README files, the more likely it is that users will try out your new
feature.
</P>
<HR>
<HR>
<A NAME = "Foo"></A>
<P><B>(Foo)</B> Foo, Morefoo, and Maxfoo, J of Classic Potentials, 75, 345 (1997).
</P>
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