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\title{{\sc OpenMD}: Molecular Dynamics in the Open} |
| 48 |
|
|
| 49 |
< |
\author{Kelsey M. Stocker, Shenyu Kuang, Charles F. Vardeman II, \\ |
| 49 |
> |
\author{Shenyu Kuang, Charles F. Vardeman II, \\ |
| 50 |
|
Teng Lin, Christopher J. Fennell, Xiuquan Sun, \\ |
| 51 |
|
Chunlei Li, Kyle Daily, Yang Zheng, Matthew A. Meineke, and \\ |
| 52 |
|
J. Daniel Gezelter \\ |
| 2626 |
|
|
| 2627 |
|
\section{Constant Pressure without periodic boundary conditions (The LangevinHull)} |
| 2628 |
|
|
| 2629 |
< |
The Langevin Hull uses an external bath at a fixed constant pressure |
| 2629 |
> |
The Langevin Hull\cite{Vardeman2011} uses an external bath at a fixed constant pressure |
| 2630 |
|
($P$) and temperature ($T$) with an effective solvent viscosity |
| 2631 |
|
($\eta$). This bath interacts only with the objects on the exterior |
| 2632 |
|
hull of the system. Defining the hull of the atoms in a simulation is |
| 2938 |
|
\label{table:zconParams} |
| 2939 |
|
\end{longtable} |
| 2940 |
|
|
| 2941 |
< |
\chapter{\label{section:restraints}Restraints} |
| 2942 |
< |
Restraints are external potentials that are added to a system to keep |
| 2943 |
< |
particular molecules or collections of particles close to some |
| 2944 |
< |
reference structure. A restraint can be a collective |
| 2941 |
> |
% \chapter{\label{section:restraints}Restraints} |
| 2942 |
> |
% Restraints are external potentials that are added to a system to keep |
| 2943 |
> |
% particular molecules or collections of particles close to some |
| 2944 |
> |
% reference structure. A restraint can be a collective |
| 2945 |
|
|
| 2946 |
|
\chapter{\label{section:thermInt}Thermodynamic Integration} |
| 2947 |
|
|
| 3080 |
|
Einstein crystal |
| 3081 |
|
\label{table:thermIntParams} |
| 3082 |
|
\end{longtable} |
| 3083 |
+ |
|
| 3084 |
+ |
\chapter{\label{section:rnemd}RNEMD} |
| 3085 |
+ |
|
| 3086 |
+ |
There are many ways to compute transport properties from molecular |
| 3087 |
+ |
dynamic simulations. Equilibrium Molecular Dynamics (EMD) simulations |
| 3088 |
+ |
can be used by computing relevant time correlation functions and |
| 3089 |
+ |
assuming linear response theory holds. These approaches are generally |
| 3090 |
+ |
subject to noise and poor convergence of the relevant correlation |
| 3091 |
+ |
functions. Traditional Non-equilibrium Molecular Dynamics (NEMD) |
| 3092 |
+ |
methods impose a gradient (e.g. thermal or momentum) on a simulation. |
| 3093 |
+ |
However, the resulting flux is often difficult to |
| 3094 |
+ |
measure. Furthermore, problems arise for NEMD simulations of |
| 3095 |
+ |
heterogeneous systems, such as phase-phase boundaries or interfaces, |
| 3096 |
+ |
where the type of gradient to enforce at the boundary between |
| 3097 |
+ |
materials is unclear. |
| 3098 |
+ |
|
| 3099 |
+ |
{\it Reverse} Non-Equilibrium Molecular Dynamics (RNEMD) methods adopt a |
| 3100 |
+ |
different approach in that an unphysical {\it flux} is imposed between |
| 3101 |
+ |
different regions or ``slabs'' of the simulation box. The response of |
| 3102 |
+ |
the system is to develop a temperature or momentum {\it gradient} |
| 3103 |
+ |
between the two regions. Since the amount of the applied flux is known |
| 3104 |
+ |
exactly, and the measurement of gradient is generally less |
| 3105 |
+ |
complicated, imposed-flux methods typically take shorter simulation |
| 3106 |
+ |
times to obtain converged results for transport properties. |
| 3107 |
+ |
|
| 3108 |
+ |
%RNEMD figure |
| 3109 |
|
|
| 3110 |
|
|
| 3111 |
+ |
RNEMD methods further its advantages by utilizing momentum- and |
| 3112 |
+ |
energy-conserving approaches to apply fluxes. The original |
| 3113 |
+ |
``swapping'' approach by Muller-Plathe {\it et al.} %CITATIONS |
| 3114 |
+ |
can be seen as an imaginary elastic collision between selected |
| 3115 |
+ |
particles for each momentum exchange. This simple to implement |
| 3116 |
+ |
algorithm turned out to be quite useful in many simulations. However, |
| 3117 |
+ |
the approach inherently perturbs the ideal Maxwell-Boltzmann |
| 3118 |
+ |
distributions, which leads to undesirable side-effects when the |
| 3119 |
+ |
applied exchanged flux becomes quite large. %CITATION |
| 3120 |
+ |
This limits the range of flux available to the method, and also its |
| 3121 |
+ |
applications. |
| 3122 |
+ |
|
| 3123 |
+ |
In OpenMD, we improve the above method by introducing two alternative |
| 3124 |
+ |
approaches: |
| 3125 |
+ |
|
| 3126 |
+ |
Non-Isotropic Velocity Scaling (NIVS): %CITATION |
| 3127 |
+ |
Instead of have two individual particles involved in momentum |
| 3128 |
+ |
exchange, this algorithm applies scaling to all the particles in |
| 3129 |
+ |
particular regions: |
| 3130 |
+ |
|
| 3131 |
+ |
%NIVS equations |
| 3132 |
+ |
|
| 3133 |
+ |
Although the above matrices can be diagonal as shown, these |
| 3134 |
+ |
coefficients cannot be always the same, in order to satisfy the linear |
| 3135 |
+ |
momentum and kinetic energy conservation constraints: |
| 3136 |
+ |
|
| 3137 |
+ |
%Conservation equations |
| 3138 |
+ |
|
| 3139 |
+ |
And to apply a kinetic energy exchange between the two regions, the |
| 3140 |
+ |
following should be satisfied as well: |
| 3141 |
+ |
|
| 3142 |
+ |
%Flux equations |
| 3143 |
+ |
|
| 3144 |
+ |
Mathematically, any points in the 3-dimensional space of the solution |
| 3145 |
+ |
set would satisfy the equations. However, to avoid solving an |
| 3146 |
+ |
ill-conditioned high-order polynomial in actual practice, another |
| 3147 |
+ |
constraint, ${x_c=y_c}$, is applied, taking into consideration of its |
| 3148 |
+ |
physical relevance. Therefore, a quartic equation is solved in actual |
| 3149 |
+ |
practice to determine the sets of possible coefficients. To determine |
| 3150 |
+ |
which set is actually used to perform the scaling, two criteria are |
| 3151 |
+ |
mainly considered: 1. ${x,y,z\rightarrow 1}$ so that the perturbation |
| 3152 |
+ |
could be as gentle as possible. 2. ${K^x, K^y, K^z}$ have minimal |
| 3153 |
+ |
difference among each other, so that the anisotropy introduced by the |
| 3154 |
+ |
algorithm can be offset to some extend. One set of scaling |
| 3155 |
+ |
coefficients is chosen against these criteria, and the best one is |
| 3156 |
+ |
used to perform the scaling for that particular step. However, if no |
| 3157 |
+ |
solution found, the NIVS move is not performed in that step. |
| 3158 |
+ |
|
| 3159 |
+ |
Although the NIVS algorithm can also be applied to impose a |
| 3160 |
+ |
directional momentum flux, thermal anisotropy was observed in |
| 3161 |
+ |
relatively high flux simulations. %This is because... |
| 3162 |
+ |
However, the gentleness and ability to apply a wide range of kinetic |
| 3163 |
+ |
energy flux makes the method useful in thermal transport simulations, |
| 3164 |
+ |
particularly for complex and heterogeneous systems including |
| 3165 |
+ |
interfaces. %CITATION |
| 3166 |
+ |
|
| 3167 |
+ |
Velocity Shearing and Scaling (VSS): %CITATION |
| 3168 |
+ |
Learning from NIVS that imposing directional momentum flux by velocity |
| 3169 |
+ |
scaling could cause problem, we shift the approach to combine the move |
| 3170 |
+ |
of velocity shearing and scaling: |
| 3171 |
+ |
|
| 3172 |
+ |
%VSS equations |
| 3173 |
+ |
|
| 3174 |
+ |
It turned out that this approach results in a set of simpler-to-solve |
| 3175 |
+ |
equations for conservation and to satisfy momentum exchange: |
| 3176 |
+ |
|
| 3177 |
+ |
%conservation equations |
| 3178 |
+ |
|
| 3179 |
+ |
Furthermore, isotropic scaling is now possible, with the presence of |
| 3180 |
+ |
velocity shearing quantities. Only a set of simple quadratic equations |
| 3181 |
+ |
need to be solved, and the positive set of coefficients are chosen, in |
| 3182 |
+ |
order to reach minimal perturbations. Similar to the NIVS method, no |
| 3183 |
+ |
VSS is performed in a step given that no solution can be found. |
| 3184 |
+ |
|
| 3185 |
+ |
The VSS approach turned out to be versatile in both thermal and |
| 3186 |
+ |
directional momentum transport simulations. It is found that the |
| 3187 |
+ |
perturbation is minimal and undesired side-effects like thermal |
| 3188 |
+ |
anisotropy can be avoided. Another nice feature of VSS is its ability |
| 3189 |
+ |
to combine a thermal and a directional momentum flux. This feature has |
| 3190 |
+ |
been utilized to map out the shear viscosity of SPC/E water in a wide |
| 3191 |
+ |
range of temperature (90~K) just with one single simulation. Possible |
| 3192 |
+ |
applications may also include the studies of thermal-momentum coupled |
| 3193 |
+ |
transport phenomena. VSS also allows the directional momentum flux to |
| 3194 |
+ |
have quite arbitary directions, which could benefit researches of |
| 3195 |
+ |
anisotropic systems. |
| 3196 |
+ |
|
| 3197 |
+ |
Table \ref{table:rnemd} summarizes the parameters used in RNEMD |
| 3198 |
+ |
simulations. |
| 3199 |
+ |
|
| 3200 |
+ |
\begin{longtable}[c]{JKLM} |
| 3201 |
+ |
\caption{The following keywords must be enclosed inside a {\tt RNEMD\{\}} block} |
| 3202 |
+ |
\\ |
| 3203 |
+ |
{\bf keyword} & {\bf units} & {\bf use} & {\bf remarks} \\ \hline |
| 3204 |
+ |
\endhead |
| 3205 |
+ |
\hline |
| 3206 |
+ |
\endfoot |
| 3207 |
+ |
{\tt useRNEMD} & logical & perform RNEMD? & default is ``false'' \\ |
| 3208 |
+ |
{\tt objectSelection} & string & see section \ref{section:syntax} |
| 3209 |
+ |
for selection syntax & default is ``select all'' \\ |
| 3210 |
+ |
{\tt method} & string & exchange method & one of the following: |
| 3211 |
+ |
{\tt Swap, NIVS,} or {\tt VSS} (default is {\tt VSS}) \\ |
| 3212 |
+ |
{\tt fluxType} & string & what is being exchanged between slabs? & one |
| 3213 |
+ |
of the following: {\tt KE, Px, Py, Pz, Pvector, KE+Px, KE+Py, KE+Pvector} \\ |
| 3214 |
+ |
{\tt kineticFlux} & kcal mol$^{-1}$ \AA$^{-2}$ fs$^{-1}$ & specify the kinetic energy flux & \\ |
| 3215 |
+ |
{\tt momentumFlux} & amu \AA$^{-1}$ fs$^{-2}$ & specify the momentum flux & \\ |
| 3216 |
+ |
{\tt momentumFluxVector} & amu \AA$^{-1}$ fs$^{-2}$ & specify the momentum flux when |
| 3217 |
+ |
{\tt Pvector} is part of the exchange & Vector3d input\\ |
| 3218 |
+ |
{\tt exchangeTime} & fs & how often to perform the exchange & default is 100 fs\\ |
| 3219 |
+ |
|
| 3220 |
+ |
{\tt slabWidth} & $\mbox{\AA}$ & width of the two exchange slabs & default is $\mathsf{H}_{zz} / 10.0$ \\ |
| 3221 |
+ |
{\tt slabAcenter} & $\mbox{\AA}$ & center of the end slab & default is 0 \\ |
| 3222 |
+ |
{\tt slabBcenter} & $\mbox{\AA}$ & center of the middle slab & default is $\mathsf{H}_{zz} / 2$ \\ |
| 3223 |
+ |
{\tt outputFileName} & string & file name for output histograms & default is the same prefix as the |
| 3224 |
+ |
.md file, but with the {\tt .rnemd} extension \\ |
| 3225 |
+ |
{\tt outputBins} & int & number of $z$-bins in the output histogram & |
| 3226 |
+ |
default is 20 \\ |
| 3227 |
+ |
{\tt outputFields} & string & columns to print in the {\tt .rnemd} |
| 3228 |
+ |
file where each column is separated by a pipe ($\mid$) symbol. & Allowed column names are: {\sc z, temperature, velocity, density}} \\ |
| 3229 |
+ |
\label{table:rnemd} |
| 3230 |
+ |
\end{longtable} |
| 3231 |
+ |
|
| 3232 |
+ |
|
| 3233 |
|
\chapter{\label{section:minimizer}Energy Minimization} |
| 3234 |
|
|
| 3235 |
|
As one of the basic procedures of molecular modeling, energy |