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<HTML>
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<CENTER><A HREF = "http://lammps.sandia.gov">LAMMPS WWW Site</A> - <A HREF = "Manual.html">LAMMPS Documentation</A> - <A HREF = "Section_commands.html#comm">LAMMPS Commands</A>
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<HR>
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<H3>thermo_style command
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</H3>
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<P><B>Syntax:</B>
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</P>
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<PRE>thermo_style style args
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</PRE>
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<UL><LI>style = <I>one</I> or <I>multi</I> or <I>granular</I> or <I>custom</I>
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<LI>args = list of arguments for a particular style
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<PRE> <I>one</I> args = none
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<I>multi</I> args = none
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<I>granular</I> args = none
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<I>custom</I> args = list of attributes
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2006-12-20 00:33:33 +08:00
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possible attributes = step, atoms, cpu, temp, press,
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pe, ke, etotal, enthalpy,
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evdwl, ecoul, epair, ebond, eangle, edihed, eimp,
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emol, elong, etail,
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vol, lx, ly, lz, xlo, xhi, ylo, yhi, zlo, zhi,
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pxx, pyy, pzz, pxy, pxz, pyz
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drot, grot,
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tave, pave, eave, peave,
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c_ID, c_ID[n], f_ID, f_ID[n], v_name
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step = timestep
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atoms = # of atoms
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cpu = elapsed CPU time
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temp = temperature
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press = pressure
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pe = total potential energy
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ke = kinetic energy
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etotal = total energy (pe + ke)
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enthalpy = enthalpy (pe + press*vol)
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evdwl = VanderWaal pairwise energy
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ecoul = Coulombic pairwise energy
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epair = pairwise energy (evdwl + ecoul + elong + etail)
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ebond = bond energy
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eangle = angle energy
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edihed = dihedral energy
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eimp = improper energy
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emol = molecular energy (ebond + eangle + edihed + eimp)
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elong = long-range kspace energy
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etail = VanderWaal energy long-range tail correction
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vol = volume
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lx,ly,lz = box lengths in x,y,z
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xlo,xhi,ylo,yhi,zlo,zhi = box boundaries
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pxx,pyy,pzz,pxy,pxz,pyz = 6 components of pressure tensor
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drot = rotational energy of dipolar atoms
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grot = rotational energy of granular atoms
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tave, pave, eave, peave = time-averaged temp, press, etotal, pe
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c_ID = scalar quantity calculated by a compute identified by its ID
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c_ID[N] = Nth vector quantity calculated by a compute identified by its ID
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f_ID = scalar quantity calculated by a fix identified by its ID
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f_ID[N] = Nth vector quantity calculated by a fix identified by its ID
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v_name = current value of a variable identified by the variable name
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</PRE>
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</UL>
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<P><B>Examples:</B>
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</P>
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<PRE>thermo_style multi
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thermo_style custom step temp pe etotal press vol
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thermo_style custom step temp etotal c_myTemp v_abc
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</PRE>
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<P><B>Description:</B>
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</P>
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<P>Set the style and content for printing thermodynamic data to the
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screen and log file.
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</P>
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<P>Style <I>one</I> prints a one-line summary of thermodynamic info that is
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the equivalent of "thermo_style custom step temp epair emol etotal
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press". The line contains only numeric values.
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</P>
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<P>Style <I>multi</I> prints a multiple-line listing of thermodynamic info
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that is the equivalent of "thermo_style custom etotal ke temp pe ebond
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eangle edihed eimp evdwl ecoul elong press". The listing contains
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numeric values and a string ID for each quantity.
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</P>
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<P>Style <I>granular</I> is used with <A HREF = "atom_style.html">atom style</A> granular
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and prints a one-line numeric summary that is the equivalent of
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"thermo_style custom step atoms ke grot".
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</P>
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<P>Style <I>custom</I> is the most general setting and allows you to specify
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which of the keywords listed above you want printed on each
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thermodynamic timestep. Note that the keywords c_ID, f_ID, v_name are
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references to <A HREF = "compute.html">computes</A>, <A HREF = "fix.html">fixes</A>, and
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<A HREF = "variable.html"">variables</A> that have been defined elsewhere in the
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input script or can even be new styles which users have added to
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LAMMPS (see the <A HREF = "Section_modify.html">Section_modify</A> section of the
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documentation). Thus the <I>custom</I> style provides a flexible means of
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outputting essentially any desired quantity as a simulation proceeds.
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</P>
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<P>All styles except <I>custom</I> have <I>vol</I> appended to their list of
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outputs if the simulation box volume changes during the simulation.
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</P>
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<P>Options invoked by the <A HREF = "thermo_modify.html">thermo_modify</A> command can
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be used to set the one- or multi-line format of the print-out, the
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normalization of energy quantities (total or per-atom), and the
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numeric precision of each printed value.
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</P>
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<P>IMPORTANT NOTE: When you specify a "thermo_style<A HREF = "thermo_modify.html"> command, all
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thermodynamic settings are restored to their default values, including
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those previously set by a :thermo_modify</A> command.
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Thus if your input script specifies a thermo_style command, you should
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use the thermo_modify command after it.
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2007-06-20 20:56:17 +08:00
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</P>
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<HR>
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<P>Several of the thermodynamic quantities require a temperature to be
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computed: "temp", "press", "ke", "etotal", "enthalpy", "pxx etc",
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"tave", "pave". By default this is done by using the "thermo_temp"
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compute which is created by LAMMPS as if this command had been issued:
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</P>
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<PRE>compute thermo_temp all temp
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</PRE>
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<P>See the <A HREF = "compute_temp.html">compute temp</A> command for details. Note
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that the ID of this compute is <I>thermo_temp</I> and the group is <I>all</I>.
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You can change the attributes of this temperature (e.g. its
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degrees-of-freedom) via the <A HREF = "compute_modify.html">compute_modify</A>
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command. Alternatively, you can directly assign a new compute (that
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calculates temperature) which you have defined, to be used for
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calculating any thermodynamic quantity that requires a temperature.
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This is done via the <A HREF = "thermo_modify.html">thermo_modify</A> command.
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</P>
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<P>Several of the thermodynamic quantities require a pressure to be
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computed: "press", "enthalpy", "pxx etc", "pave". By default this is
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done by using the "thermo_pressure" compute which is created by LAMMPS
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as if this command had been issued:
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</P>
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<PRE>compute thermo_pressure all pressure thermo_temp
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</PRE>
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<P>See the <A HREF = "compute_pressure.html">compute pressure</A> command for details.
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Note that the ID of this compute is <I>thermo_pressure</I> and the group is
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<I>all</I>. You can change the attributes of this pressure via the
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<A HREF = "compute_modify.html">compute_modify</A> command. Alternatively, you can
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directly assign a new compute (that calculates pressure) which you
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have defined, to be used for calculating any thermodynamic quantity
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that requires a pressure. This is done via the
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<A HREF = "thermo_modify.html">thermo_modify</A> command.
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</P>
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<P>The <I>drot</I> keyword requires a rotational energy to be computed for
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point dipole particles. To do this, a compute of style
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"rotate/dipole" is created, as if this command had been issued:
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</P>
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<PRE>compute thermo_rotate_dipole all rotate/dipole
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</PRE>
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<P>See the <A HREF = "compute_rotate_dipole.html">compute rotate/dipole</A> command for
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details. Note that the ID of the new compute is
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<I>thermo_rotate_dipole</I> and the group is <I>all</I>. You can change the
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attributes of this computation via the
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<A HREF = "compute_modify.html">compute_modify</A> command. Alternatively, you can
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directly assign a new compute which you have defined, to be used for
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<I>drot</I>. This is done via the <A HREF = "thermo_modify.html">thermo_modify</A>
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command. For example, this could be useful if you wish to exclude
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certain particles from the compuation.
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</P>
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<P>The <I>grot</I> keyword requires a rotational energy to be computed for
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granular particles. To do this, a compute of style "rotate/gran" is
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created, as if this command had been issued:
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</P>
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<PRE>compute thermo_rotate_gran all rotate/gran
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</PRE>
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<P>See the <A HREF = "compute_rotate_gran.html">compute rotate/gran</A> command for
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details. Note that the ID of the new compute is <I>thermo_rotate_gran</I>
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and the group is <I>all</I>. You can change the attributes of this
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computation via the <A HREF = "compute_modify.html">compute_modify</A> command.
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Alternatively, you can directly assign a new compute which you have
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defined, to be used for <I>grot</I>. This is done via the
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<A HREF = "thermo_modify.html">thermo_modify</A> command. For example, this could
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be useful if you wish to exclude frozen particles from the compuation.
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</P>
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<HR>
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<P>The potential energy of the system <I>pe</I> will include contributions
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from fixes if the <A HREF = "fix_modify.html">fix_modify thermo</A> option was set
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for each fix. For example, the <A HREF = "fix_wall_lj93">fix wall/lj93</A> fix will
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contribute the energy of atoms interacting with the wall.
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</P>
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<P>A long-range tail correction <I>etail</I> for the VanderWaal pairwise
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energy will be non-zero only if the <A HREF = "pair_modify.html">pair_modify
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tail</A> option is turned on. The <I>etail</I> contribution
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is included in <I>evdwl</I>, <I>pe</I>, and <I>etotal</I>, and the corresponding tail
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correction to the pressure is included in <I>press</I> and <I>pxx</I>, <I>pyy</I>,
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etc.
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</P>
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<P>The time-averaged keywords <I>tave, pave, eave, peave</I> are averaged over
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the last N thermodynamic outputs to the screen (not the last N
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timesteps), where N is the value set by the <I>window</I> option of the
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<A HREF = "thermo_modify.html">thermo_modify</A> command (N = 10 by default).
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</P>
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<HR>
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<P>The <I>c_ID</I> and <I>c_ID[N]</I> keywords allow scalar or vector quantities
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calculated by a compute to be output. The ID in the keyword should be
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replaced by the actual ID of the compute that has been defined
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elsewhere in the input script. See the <A HREF = "compute.html">compute</A> command
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for details. Note that only global scalar or vector quantites
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calculated by a compute can be output as thermodynamic data; per-atom
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quantities calcalated by a compute are output by the <A HREF = "dump.html">dump
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custom</A> command.
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</P>
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<P>If <I>c_ID</I> is used as a keyword, then the scalar quantity calculated by
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the compute is printed. If <I>c_ID[N]</I> is used, then N in the range
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from 1-M will print the Nth component of the M-length vector
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calculated by the compute. See the doc pages for individual compute
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styles for info on what these quantities are.
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</P>
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<P>The <I>f_ID</I> and <I>f_ID[N]</I> keywords allow scalar or vector quantities
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calculated by a fix to be output. The ID in the keyword should be
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replaced by the actual ID of the fix that has been defined elsewhere
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in the input script.
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</P>
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<P>If <I>f_ID</I> is used as a keyword, then the scalar quantity calculated by
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the fix is printed. If <I>f_ID[N]</I> is used, then N in the range from
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1-M will print the Nth component of the M-length vector calculated by
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the fix. See the doc pages for individual fix styles for info on what
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these quantities are. For fixes that compute a contribution to the
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potential energy of the system, the scalar quantity f_ID is typically
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that quantity.
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</P>
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<P>The <I>v_name</I> keyword allow the current value of a variable to be
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output. The name in the keyword should be replaced by the actual namd
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of the variable that has been defined elsewhere in the input script.
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See the <A HREF = "variable.html">variable</A> command for details. Equal-style
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variables can calculate complex formulas involving atom and group
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properties, mathematical operations, other variables, etc. This
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keyword enables them to be evaluated and their value printed
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periodically during a simulation.
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</P>
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<P>See <A HREF = "Section_modify.html">this section</A> for information on how to add
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new compute and fix styles as well as variable options to LAMMPS that
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2007-06-25 22:36:36 +08:00
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calculate quantities that could then be output with these keywords as
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part of thermodyanmic information.
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2006-09-22 00:22:34 +08:00
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</P>
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2007-02-10 05:37:30 +08:00
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<HR>
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2006-09-22 00:22:34 +08:00
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<P><B>Restrictions:</B>
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</P>
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<P>This command must come after the simulation box is defined by a
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<A HREF = "read_data.html">read_data</A>, <A HREF = "read_restart.html">read_restart</A>, or
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<A HREF = "create_box.html">create_box</A> command.
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</P>
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<P><B>Related commands:</B>
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</P>
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<P><A HREF = "thermo.html">thermo</A>, <A HREF = "thermo_modify.html">thermo_modify</A>,
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<A HREF = "fix_modify.html">fix_modify</A>, <A HREF = "temperature.html">temperature</A>
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</P>
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<P><B>Default:</B>
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</P>
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<PRE>thermo_style one
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</PRE>
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</HTML>
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