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@ -2515,7 +2515,9 @@ the electrostatic environment inducing polarizability.
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<P>Technically, shells are attached to the cores by a spring force f =
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<P>Technically, shells are attached to the cores by a spring force f =
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k*r where k is a parametrized spring constant and r is the distance
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k*r where k is a parametrized spring constant and r is the distance
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between the core and the shell. The charges of the core and the shell
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between the core and the shell. The charges of the core and the shell
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add up to the ion charge, thus q(ion) = q(core) + q(shell). In a
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add up to the ion charge, thus q(ion) = q(core) + q(shell). This
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setup introduces the ion polarizability (alpha) given by
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alpha = q(shell)^2 / k. In a
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similar fashion the mass of the ion is distributed on the core and the
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similar fashion the mass of the ion is distributed on the core and the
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shell with the core having the larger mass.
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shell with the core having the larger mass.
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</P>
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</P>
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@ -2560,7 +2562,7 @@ for NaCl, as found in examples/coreshell, has this format:
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<P>Non-Coulombic (e.g. Lennard-Jones) pairwise interactions are only
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<P>Non-Coulombic (e.g. Lennard-Jones) pairwise interactions are only
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defined between the shells. Coulombic interactions are defined
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defined between the shells. Coulombic interactions are defined
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between all cores and shells. If desired, additional bonds can be
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between all cores and shells. If desired, additional bonds can be
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specified between cores.
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specified between cores.
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</P>
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</P>
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<P>The <A HREF = "special_bonds.html">special_bonds</A> command should be used to
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<P>The <A HREF = "special_bonds.html">special_bonds</A> command should be used to
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turn-off the Coulombic interaction within core/shell pairs, since that
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turn-off the Coulombic interaction within core/shell pairs, since that
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@ -2577,7 +2579,7 @@ satellite particle if desired.
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</P>
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</P>
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<P>Since the core/shell model permits distances of r = 0.0 between the
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<P>Since the core/shell model permits distances of r = 0.0 between the
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core and shell, a pair style with a "cs" suffix needs to be used to
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core and shell, a pair style with a "cs" suffix needs to be used to
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implement a valid long-rangeCoulombic correction. Several such pair
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implement a valid long-range Coulombic correction. Several such pair
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styles are provided in the CORESHELL package. See <A HREF = "pair_cs.html">this doc
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styles are provided in the CORESHELL package. See <A HREF = "pair_cs.html">this doc
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page</A> for details. All of the core/shell enabled pair
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page</A> for details. All of the core/shell enabled pair
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styles require the use of a long-range Coulombic solver, as specified
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styles require the use of a long-range Coulombic solver, as specified
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@ -2600,8 +2602,9 @@ bond_coeff 2 25.724 0.0
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<P>When running dynamics with the adiabatic core/shell model, the
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<P>When running dynamics with the adiabatic core/shell model, the
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following issues should be considered. Since the relative motion of
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following issues should be considered. Since the relative motion of
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the core and shell particles corresponds to the polarization, typical
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the core and shell particles corresponds to the polarization, typical
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thermostats can alter the polarization behaviour, meaining the shell
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thermostats can alter the polarization behaviour, meaning the shell
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will not react freely to its electrostatic environment. Therefore
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will not react freely to its electrostatic environment. This is
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critical during the equilibration of the system. Therefore
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it's typically desirable to decouple the relative motion of the
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it's typically desirable to decouple the relative motion of the
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core/shell pair, which is an imaginary degree of freedom, from the
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core/shell pair, which is an imaginary degree of freedom, from the
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real physical system. To do that, the <A HREF = "compute_temp_cs.html">compute
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real physical system. To do that, the <A HREF = "compute_temp_cs.html">compute
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@ -2620,9 +2623,9 @@ into account by the <I>group-ID</I> (2nd argument) of the compute. The
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groups can be defined using the <A HREF = "group.html">group <I>type</I></A> command.
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groups can be defined using the <A HREF = "group.html">group <I>type</I></A> command.
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Note that to perform thermostatting using this definition of
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Note that to perform thermostatting using this definition of
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temperature, the <A HREF = "fix_modify.html">fix modify temp</A> command should be
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temperature, the <A HREF = "fix_modify.html">fix modify temp</A> command should be
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used to assign the comptue to the thermostat fix. Likewise the
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used to assign the compute to the thermostat fix. Likewise the
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<A HREF = "thermo_modify.html">thermo_modify temp</A> command can be used to make
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<A HREF = "thermo_modify.html">thermo_modify temp</A> command can be used to make
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this temperature be output for the overall system.
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this temperature be output for the overall system.
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</P>
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</P>
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<P>For the NaCl example, this can be done as follows:
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<P>For the NaCl example, this can be done as follows:
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</P>
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</P>
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@ -2634,6 +2637,15 @@ fix thermostatequ all nve # integrator as needed f
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fix_modify thermoberendsen temp CSequ
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fix_modify thermoberendsen temp CSequ
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thermo_modify temp CSequ # output of center-of-mass derived temperature
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thermo_modify temp CSequ # output of center-of-mass derived temperature
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</PRE>
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</PRE>
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<P>If <A HREF = "compute_temp_cs.html">compute temp/cs</A> is used, the decoupled
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relative motion of the core and the shell should in theory be
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stable. However numerical fluctuation can introduce a small
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momentum to the system, which is noticable over long trajectories.
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Therefore it is recomendable to use the <A HREF = "fix_momentum.html">fix
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momentum</A> command in combination with <A HREF = "compute_temp_cs.html">compute
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temp/cs</A> when equilibrating the system to
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prevent any drift.
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</P>
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<P>When intializing the velocities of a system with core/shell pairs, it
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<P>When intializing the velocities of a system with core/shell pairs, it
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is also desirable to not introduce energy into the relative motion of
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is also desirable to not introduce energy into the relative motion of
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the core/shell particles, but only assign a center-of-mass velocity to
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the core/shell particles, but only assign a center-of-mass velocity to
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@ -2653,12 +2665,19 @@ velocity. This allow the shells to effectively react instantaneously
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to the electrostatic environment. This fast movement also limits the
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to the electrostatic environment. This fast movement also limits the
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timestep size that can be used.
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timestep size that can be used.
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</P>
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</P>
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<P>Additionally, the mass mismatch of the core and shell particles means
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<P>The primary literature of the adiabatic core/shell model suggests that
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that only a small amount of energy is transfered to the decoupled
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the fast relative motion of the core/shell pairs only allows negligible
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imaginary degrees of freedom. However, this transfer will typically
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energy transfer to the environment. Therefore it is not intended to
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lead to a a small drift in total energy over time. This internal
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decouple the core/shell degree of freedom from the physical system
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energy can be monitored using the <A HREF = "compute_chunk_atom.html">compute
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during production runs. In other words, the <A HREF = "compute_temp_cs.html">compute
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chunk/atom</A> and <A HREF = "compute_temp_chunk.html">compute
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temp/cs</A> command should not be used during
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production runs and is only required during equilibration. This way one
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is consistent with literature (based on the code packages DL_POLY or
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GULP for instance).
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</P>
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<P>The mentioned energy transfer will typically lead to a a small drift
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in total energy over time. This internal energy can be monitored
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using the <A HREF = "compute_chunk_atom.html">compute chunk/atom</A> and <A HREF = "compute_temp_chunk.html">compute
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temp/chunk</A> commands. The internal kinetic
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temp/chunk</A> commands. The internal kinetic
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energies of each core/shell pair can then be summed using the sum()
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energies of each core/shell pair can then be summed using the sum()
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special function of the <A HREF = "variable.html">variable</A> command. Or they can
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special function of the <A HREF = "variable.html">variable</A> command. Or they can
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@ -67,8 +67,8 @@ calculated by this compute for use in the computation of a pressure
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tensor. The formula for the components of the tensor is the same as
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tensor. The formula for the components of the tensor is the same as
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the above formula, except that v^2 is replaced by vx*vy for the xy
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the above formula, except that v^2 is replaced by vx*vy for the xy
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component, etc. The 6 components of the vector are ordered xx, yy,
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component, etc. The 6 components of the vector are ordered xx, yy,
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zz, xy, xz, yz. Again, the velocity of each core or shell atom is its
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zz, xy, xz, yz. In contrast to the temperature, the velocity of
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COM velocity.
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each core or shell atom is taken individually.
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</P>
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</P>
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<P>The change this fix makes to core/shell atom velocities is essentially
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<P>The change this fix makes to core/shell atom velocities is essentially
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computing the temperature after a "bias" has been removed from the
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computing the temperature after a "bias" has been removed from the
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@ -926,6 +926,10 @@
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</dt>
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</dt>
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<dt><a href="fix_ave_correlate_long.html#index-0">fix ave/correlate/long</a>
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</dt>
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<dt><a href="fix_ave_histo.html#index-0">fix ave/histo</a>
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<dt><a href="fix_ave_histo.html#index-0">fix ave/histo</a>
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</dt>
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</dt>
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