17 |
|
\textwidth 6.5in |
18 |
|
\brokenpenalty=10000 |
19 |
|
\renewcommand{\baselinestretch}{1.2} |
20 |
+ |
\usepackage[square, comma, sort&compress]{natbib} |
21 |
+ |
\bibpunct{[}{]}{,}{n}{}{;} |
22 |
|
|
23 |
+ |
|
24 |
|
%\renewcommand\citemid{\ } % no comma in optional reference note |
25 |
|
\lstset{language=C,frame=TB,basicstyle=\tiny,basicstyle=\ttfamily, % |
26 |
|
xleftmargin=0.25in, xrightmargin=0.25in,captionpos=b, % |
41 |
|
\newcolumntype{H}{p{0.75in}} |
42 |
|
\newcolumntype{I}{p{5in}} |
43 |
|
|
44 |
+ |
\newcolumntype{J}{p{1.5in}} |
45 |
+ |
\newcolumntype{K}{p{1.2in}} |
46 |
+ |
\newcolumntype{L}{p{1.5in}} |
47 |
+ |
\newcolumntype{M}{p{1.55in}} |
48 |
|
|
42 |
– |
\title{{\sc OpenMD}: Molecular Dynamics in the Open} |
49 |
|
|
50 |
< |
\author{Kelsey M. Stocker, Shenyu Kuang, Charles F. Vardeman II, \\ |
51 |
< |
Teng Lin, Christopher J. Fennell, Xiuquan Sun, \\ |
50 |
> |
\title{{\sc OpenMD-2}: Molecular Dynamics in the Open} |
51 |
> |
|
52 |
> |
\author{Shenyu Kuang, Joseph Michalka, Kelsey Stocker, James Marr, \\ |
53 |
> |
Teng Lin, Charles F. Vardeman II, Christopher J. Fennell, Xiuquan Sun, \\ |
54 |
|
Chunlei Li, Kyle Daily, Yang Zheng, Matthew A. Meineke, and \\ |
55 |
|
J. Daniel Gezelter \\ |
56 |
|
Department of Chemistry and Biochemistry\\ |
499 |
|
\endhead |
500 |
|
\hline |
501 |
|
\endfoot |
502 |
< |
{\tt forceField} & string & Sets the force field. & Possible force |
503 |
< |
fields are DUFF, WATER, LJ, EAM, SC, and CLAY. \\ |
502 |
> |
{\tt forceField} & string & Sets the base name for the force field file & |
503 |
> |
OpenMD appends a {\tt .frc} to the end of this to look for a force |
504 |
> |
field file.\\ |
505 |
|
{\tt component} & & Defines the molecular components of the system & |
506 |
|
Every {\tt $<$MetaData$>$} block must have a component statement. \\ |
507 |
|
{\tt minimizer} & string & Chooses a minimizer & Possible minimizers |
2630 |
|
|
2631 |
|
\section{Constant Pressure without periodic boundary conditions (The LangevinHull)} |
2632 |
|
|
2633 |
< |
The Langevin Hull uses an external bath at a fixed constant pressure |
2633 |
> |
The Langevin Hull\cite{Vardeman2011} uses an external bath at a fixed constant pressure |
2634 |
|
($P$) and temperature ($T$) with an effective solvent viscosity |
2635 |
|
($\eta$). This bath interacts only with the objects on the exterior |
2636 |
|
hull of the system. Defining the hull of the atoms in a simulation is |
2942 |
|
\label{table:zconParams} |
2943 |
|
\end{longtable} |
2944 |
|
|
2945 |
< |
\chapter{\label{section:restraints}Restraints} |
2946 |
< |
Restraints are external potentials that are added to a system to keep |
2947 |
< |
particular molecules or collections of particles close to some |
2948 |
< |
reference structure. A restraint can be a collective |
2945 |
> |
% \chapter{\label{section:restraints}Restraints} |
2946 |
> |
% Restraints are external potentials that are added to a system to |
2947 |
> |
% keep particular molecules or collections of particles close to some |
2948 |
> |
% reference structure. A restraint can be a collective |
2949 |
|
|
2950 |
|
\chapter{\label{section:thermInt}Thermodynamic Integration} |
2951 |
|
|
3083 |
|
\mbox{rad}^{-2}$ & & spring constant for rotation around z-axis in |
3084 |
|
Einstein crystal |
3085 |
|
\label{table:thermIntParams} |
3086 |
+ |
\end{longtable} |
3087 |
+ |
|
3088 |
+ |
\chapter{\label{section:rnemd}RNEMD} |
3089 |
+ |
|
3090 |
+ |
There are many ways to compute transport properties from molecular |
3091 |
+ |
dynamics simulations. Equilibrium Molecular Dynamics (EMD) |
3092 |
+ |
simulations can be used by computing relevant time correlation |
3093 |
+ |
functions and assuming linear response theory holds. These approaches |
3094 |
+ |
are generally subject to noise and poor convergence of the relevant |
3095 |
+ |
correlation functions. Traditional Non-equilibrium Molecular Dynamics |
3096 |
+ |
(NEMD) methods impose a gradient (e.g. thermal or momentum) on a |
3097 |
+ |
simulation. However, the resulting flux is often difficult to |
3098 |
+ |
measure. Furthermore, problems arise for NEMD simulations of |
3099 |
+ |
heterogeneous systems, such as phase-phase boundaries or interfaces, |
3100 |
+ |
where the type of gradient to enforce at the boundary between |
3101 |
+ |
materials is unclear. |
3102 |
+ |
|
3103 |
+ |
{\it Reverse} Non-Equilibrium Molecular Dynamics (RNEMD) methods adopt |
3104 |
+ |
a different approach in that an unphysical {\it flux} is imposed |
3105 |
+ |
between different regions or ``slabs'' of the simulation box. The |
3106 |
+ |
response of the system is to develop a temperature or momentum {\it |
3107 |
+ |
gradient} between the two regions. Since the amount of the applied |
3108 |
+ |
flux is known exactly, and the measurement of gradient is generally |
3109 |
+ |
less complicated, imposed-flux methods typically take shorter |
3110 |
+ |
simulation times to obtain converged results for transport properties. |
3111 |
+ |
|
3112 |
+ |
\begin{figure} |
3113 |
+ |
\includegraphics[width=\linewidth]{rnemdDemo} |
3114 |
+ |
\caption{The (VSS) RNEMD approach imposes unphysical transfer of both |
3115 |
+ |
linear momentum and kinetic energy between a ``hot'' slab and a |
3116 |
+ |
``cold'' slab in the simulation box. The system responds to this |
3117 |
+ |
imposed flux by generating both momentum and temperature gradients. |
3118 |
+ |
The slope of the gradients can then be used to compute transport |
3119 |
+ |
properties (e.g. shear viscosity and thermal conductivity).} |
3120 |
+ |
\label{rnemdDemo} |
3121 |
+ |
\end{figure} |
3122 |
+ |
|
3123 |
+ |
The original ``swapping'' approaches by M\"{u}ller-Plathe {\it et |
3124 |
+ |
al.}\cite{ISI:000080382700030,MullerPlathe:1997xw} can be understood |
3125 |
+ |
as a sequence of imaginary elastic collisions between particles in |
3126 |
+ |
opposite slabs. In each collision, the entire momentum vectors of |
3127 |
+ |
both particles may be exchanged to generate a thermal |
3128 |
+ |
flux. Alternatively, a single component of the momentum vectors may be |
3129 |
+ |
exchanged to generate a shear flux. This algorithm turns out to be |
3130 |
+ |
quite useful in many simulations. However, the M\"{u}ller-Plathe |
3131 |
+ |
swapping approach perturbs the system away from ideal |
3132 |
+ |
Maxwell-Boltzmann distributions, and this may leads to undesirable |
3133 |
+ |
side-effects when the applied flux becomes large.\cite{Maginn:2010} |
3134 |
+ |
This limits the application of the swapping algorithm, so in OpenMD, |
3135 |
+ |
we implement two additional algorithms for RNEMD in addition to the |
3136 |
+ |
original swapping approach. |
3137 |
+ |
|
3138 |
+ |
{\bf Non-Isotropic Velocity Scaling (NIVS):}\cite{kuang:164101} |
3139 |
+ |
Instead of having momentum exchange between {\it individual particles} |
3140 |
+ |
in each slab, the NIVS algorithm applies velocity scaling to all of |
3141 |
+ |
the selected particles in both slabs. A combination of linear |
3142 |
+ |
momentum, kinetic energy, and flux constraint equations governs the |
3143 |
+ |
amount of velocity scaling performed at each step. Interested readers |
3144 |
+ |
should consult ref. \citealp{kuang:164101} for further details on the |
3145 |
+ |
methodology. |
3146 |
+ |
|
3147 |
+ |
NIVS has been shown to be very effective at producing thermal |
3148 |
+ |
gradients and for computing thermal conductivities, particularly for |
3149 |
+ |
heterogeneous interfaces. Although the NIVS algorithm can also be |
3150 |
+ |
applied to impose a directional momentum flux, thermal anisotropy was |
3151 |
+ |
observed in relatively high flux simulations, and the method is not |
3152 |
+ |
suitable for imposing a shear flux. |
3153 |
+ |
|
3154 |
+ |
{\bf Velocity Shearing and Scaling (VSS)}:\cite{2012MolPh.110..691K} |
3155 |
+ |
The third RNEMD algorithm implemented in OpenMD utilizes a series of |
3156 |
+ |
simultaneous velocity shearing and scaling exchanges between the two |
3157 |
+ |
slabs. This method results in a set of simpler equations to satisfy |
3158 |
+ |
the conservation constraints while creating a desired flux between the |
3159 |
+ |
two slabs. |
3160 |
+ |
|
3161 |
+ |
The VSS approach is versatile in that it may be used to implement both |
3162 |
+ |
thermal and shear transport either separately or simultaneously. |
3163 |
+ |
Perturbations of velocities away from the ideal Maxwell-Boltzmann |
3164 |
+ |
distributions are minimal, and thermal anisotropy is kept to a |
3165 |
+ |
minimum. This ability to generate simultaneous thermal and shear |
3166 |
+ |
fluxes has been utilized to map out the shear viscosity of SPC/E water |
3167 |
+ |
in a wide range of temperature (90~K) just with a single simulation. |
3168 |
+ |
VSS-RNEMD also allows the directional momentum flux to have quite |
3169 |
+ |
arbitary directions, which could aid in the study of anisotropic solid |
3170 |
+ |
surfaces in contact with liquid environments. |
3171 |
+ |
|
3172 |
+ |
{\bf What the user needs to specify:} To carry out a RNEMD simulation, |
3173 |
+ |
a user must specify a number of parameters in the MetaData (.md) file. |
3174 |
+ |
Because the RNEMD methods have a large number of parameters, these |
3175 |
+ |
must be enclosed in a {\tt RNEMD\{...\}} block. The most important |
3176 |
+ |
parameters to specify are the {\tt useRNEMD}, {\tt fluxType} and flux |
3177 |
+ |
parameters. Most other parameters (summarized in table |
3178 |
+ |
\ref{table:rnemd}) have reasonable default values. {\tt fluxType} |
3179 |
+ |
sets up the kind of exchange that will be carried out between the two |
3180 |
+ |
slabs (either Kinetic Energy ({\tt KE}) or momentum ({\tt Px, Py, Pz, |
3181 |
+ |
Pvector}), or some combination of these). The flux is specified |
3182 |
+ |
with the use of three possible parameters: {\tt kineticFlux} for |
3183 |
+ |
kinetic energy exchange, as well as {\tt momentumFlux} or {\tt |
3184 |
+ |
momentumFluxVector} for simulations with directional exchange. |
3185 |
+ |
|
3186 |
+ |
{\bf How to process the results:} OpenMD will generate a {\tt .rnemd} |
3187 |
+ |
file with the same prefix as the original {\tt .md} file. This file |
3188 |
+ |
contains a running average of properties of interest computed within a |
3189 |
+ |
set of bins that divide the simulation cell along the $z$-axis. The |
3190 |
+ |
first column of the {\tt .rnemd} file is the $z$ coordinate of the |
3191 |
+ |
center of each bin, while following columns may contain the average |
3192 |
+ |
temperature, velocity, or density within each bin. The output format |
3193 |
+ |
in the {\tt .rnemd} file can be altered with the {\tt outputFields}, |
3194 |
+ |
{\tt outputBins}, and {\tt outputFileName} parameters. A report at |
3195 |
+ |
the top of the {\tt .rnemd} file contains the current exchange totals |
3196 |
+ |
as well as the average flux applied during the simulation. Using the |
3197 |
+ |
slope of the temperature or velocity gradient obtaine from the {\tt |
3198 |
+ |
.rnemd} file along with the applied flux, the user can very simply |
3199 |
+ |
arrive at estimates of thermal conductivities ($\lambda$), |
3200 |
+ |
\begin{equation} |
3201 |
+ |
J_z = -\lambda \frac{\partial T}{\partial z}, |
3202 |
+ |
\end{equation} |
3203 |
+ |
and shear viscosities ($\eta$), |
3204 |
+ |
\begin{equation} |
3205 |
+ |
j_z(p_x) = -\eta \frac{\partial \langle v_x \rangle}{\partial z}. |
3206 |
+ |
\end{equation} |
3207 |
+ |
Here, the quantities on the left hand side are the actual flux values |
3208 |
+ |
(in the header of the {\tt .rnemd} file), while the slopes are |
3209 |
+ |
obtained from linear fits to the gradients observed in the {\tt |
3210 |
+ |
.rnemd} file. |
3211 |
+ |
|
3212 |
+ |
More complicated simulations (including interfaces) require a bit more |
3213 |
+ |
care. Here the second derivative may be required to compute the |
3214 |
+ |
interfacial thermal conductance, |
3215 |
+ |
\begin{align} |
3216 |
+ |
G^\prime &= \left(\nabla\lambda \cdot \mathbf{\hat{n}}\right)_{z_0} \\ |
3217 |
+ |
&= \frac{\partial}{\partial z}\left(-\frac{J_z}{ |
3218 |
+ |
\left(\frac{\partial T}{\partial z}\right)}\right)_{z_0} \\ |
3219 |
+ |
&= J_z\left(\frac{\partial^2 T}{\partial z^2}\right)_{z_0} \Big/ |
3220 |
+ |
\left(\frac{\partial T}{\partial z}\right)_{z_0}^2. |
3221 |
+ |
\label{derivativeG} |
3222 |
+ |
\end{align} |
3223 |
+ |
where $z_0$ is the location of the interface between two materials and |
3224 |
+ |
$\mathbf{\hat{n}}$ is a unit vector normal to the interface. We |
3225 |
+ |
suggest that users interested in interfacial conductance consult |
3226 |
+ |
reference \citealp{kuang:AuThl} for other approaches to computing $G$. |
3227 |
+ |
Users interested in {\it friction coefficients} at heterogeneous |
3228 |
+ |
interfaces may also find reference \citealp{2012MolPh.110..691K} |
3229 |
+ |
useful. |
3230 |
+ |
|
3231 |
+ |
\newpage |
3232 |
+ |
|
3233 |
+ |
\begin{longtable}[c]{JKLM} |
3234 |
+ |
\caption{The following keywords must be enclosed inside a {\tt RNEMD\{\}} block} |
3235 |
+ |
\\ |
3236 |
+ |
{\bf keyword} & {\bf units} & {\bf use} & {\bf remarks} \\ \hline |
3237 |
+ |
\endhead |
3238 |
+ |
\hline |
3239 |
+ |
\endfoot |
3240 |
+ |
{\tt useRNEMD} & logical & perform RNEMD? & default is ``false'' \\ |
3241 |
+ |
{\tt objectSelection} & string & see section \ref{section:syntax} |
3242 |
+ |
for selection syntax & default is ``select all'' \\ |
3243 |
+ |
{\tt method} & string & exchange method & one of the following: |
3244 |
+ |
{\tt Swap, NIVS,} or {\tt VSS} (default is {\tt VSS}) \\ |
3245 |
+ |
{\tt fluxType} & string & what is being exchanged between slabs? & one |
3246 |
+ |
of the following: {\tt KE, Px, Py, Pz, Pvector, KE+Px, KE+Py, KE+Pvector} \\ |
3247 |
+ |
{\tt kineticFlux} & kcal mol$^{-1}$ \AA$^{-2}$ fs$^{-1}$ & specify the kinetic energy flux & \\ |
3248 |
+ |
{\tt momentumFlux} & amu \AA$^{-1}$ fs$^{-2}$ & specify the momentum flux & \\ |
3249 |
+ |
{\tt momentumFluxVector} & amu \AA$^{-1}$ fs$^{-2}$ & specify the momentum flux when |
3250 |
+ |
{\tt Pvector} is part of the exchange & Vector3d input\\ |
3251 |
+ |
{\tt exchangeTime} & fs & how often to perform the exchange & default is 100 fs\\ |
3252 |
+ |
|
3253 |
+ |
{\tt slabWidth} & $\mbox{\AA}$ & width of the two exchange slabs & default is $\mathsf{H}_{zz} / 10.0$ \\ |
3254 |
+ |
{\tt slabAcenter} & $\mbox{\AA}$ & center of the end slab & default is 0 \\ |
3255 |
+ |
{\tt slabBcenter} & $\mbox{\AA}$ & center of the middle slab & default is $\mathsf{H}_{zz} / 2$ \\ |
3256 |
+ |
{\tt outputFileName} & string & file name for output histograms & default is the same prefix as the |
3257 |
+ |
.md file, but with the {\tt .rnemd} extension \\ |
3258 |
+ |
{\tt outputBins} & int & number of $z$-bins in the output histogram & |
3259 |
+ |
default is 20 \\ |
3260 |
+ |
{\tt outputFields} & string & columns to print in the {\tt .rnemd} |
3261 |
+ |
file where each column is separated by a pipe ($\mid$) symbol. & Allowed column names are: {\sc z, temperature, velocity, density} \\ |
3262 |
+ |
\label{table:rnemd} |
3263 |
|
\end{longtable} |
3264 |
|
|
3265 |
|
|
3936 |
|
DMR-0079647. |
3937 |
|
|
3938 |
|
|
3939 |
< |
\bibliographystyle{jcc} |
3939 |
> |
\bibliographystyle{aip} |
3940 |
|
\bibliography{openmdDoc} |
3941 |
|
|
3942 |
|
\end{document} |