18 |
|
responsible for the evaluation of its own bonded interaction |
19 |
|
(i.e.~bonds, bends, and torsions). |
20 |
|
|
21 |
< |
As stated previously, one of the features that sets {\sc OOPSE} apart |
21 |
> |
As stated previously, one of the features that sets {\sc oopse} apart |
22 |
|
from most of the current molecular simulation packages is the ability |
23 |
|
to handle rigid body dynamics. Rigid bodies are non-spherical |
24 |
|
particles or collections of particles that have a constant internal |
25 |
|
potential and move collectively.\cite{Goldstein01} They are not |
26 |
< |
included in most simulation packages because of the need to |
27 |
< |
consider orientational degrees of freedom and include an integrator |
28 |
< |
that accurately propagates these motions in time. |
26 |
> |
included in most simulation packages because of the requirement to |
27 |
> |
propagate the orientational degrees of freedom. Until recently, |
28 |
> |
integrators which propagate orientational motion have been lacking. |
29 |
|
|
30 |
|
Moving a rigid body involves determination of both the force and |
31 |
|
torque applied by the surroundings, which directly affect the |
32 |
< |
translation and rotation in turn. In order to accumulate the total |
33 |
< |
force on a rigid body, the external forces must first be calculated |
34 |
< |
for all the internal particles. The total force on the rigid body is |
35 |
< |
simply the sum of these external forces. Accumulation of the total |
36 |
< |
torque on the rigid body is more complex than the force in that it is |
37 |
< |
the torque applied on the center of mass that dictates rotational |
38 |
< |
motion. The summation of this torque is given by |
32 |
> |
translational and rotational motion in turn. In order to accumulate |
33 |
> |
the total force on a rigid body, the external forces and torques must |
34 |
> |
first be calculated for all the internal particles. The total force on |
35 |
> |
the rigid body is simply the sum of these external forces. |
36 |
> |
Accumulation of the total torque on the rigid body is more complex |
37 |
> |
than the force in that it is the torque applied on the center of mass |
38 |
> |
that dictates rotational motion. The torque on rigid body {\it i} is |
39 |
|
\begin{equation} |
40 |
< |
\mathbf{\tau}_i= |
41 |
< |
\sum_{a}(\mathbf{r}_{ia}-\mathbf{r}_i)\times \mathbf{f}_{ia}, |
40 |
> |
\boldsymbol{\tau}_i= |
41 |
> |
\sum_{a}(\mathbf{r}_{ia}-\mathbf{r}_i)\times \mathbf{f}_{ia} |
42 |
> |
+ \boldsymbol{\tau}_{ia}, |
43 |
|
\label{eq:torqueAccumulate} |
44 |
|
\end{equation} |
45 |
< |
where $\mathbf{\tau}_i$ and $\mathbf{r}_i$ are the torque about and |
46 |
< |
position of the center of mass respectively, while $\mathbf{f}_{ia}$ |
47 |
< |
and $\mathbf{r}_{ia}$ are the force on and position of the component |
48 |
< |
particles of the rigid body.\cite{allen87:csl} |
45 |
> |
where $\boldsymbol{\tau}_i$ and $\mathbf{r}_i$ are the torque on and |
46 |
> |
position of the center of mass respectively, while $\mathbf{f}_{ia}$, |
47 |
> |
$\mathbf{r}_{ia}$, and $\boldsymbol{\tau}_{ia}$ are the force on, |
48 |
> |
position of, and torque on the component particles of the rigid body. |
49 |
|
|
50 |
< |
The application of the total torque is done in the body fixed axis of |
50 |
> |
The summation of the total torque is done in the body fixed axis of |
51 |
|
the rigid body. In order to move between the space fixed and body |
52 |
|
fixed coordinate axes, parameters describing the orientation must be |
53 |
|
maintained for each rigid body. At a minimum, the rotation matrix |
54 |
< |
(\textbf{A}) can be described and propagated by the three Euler angles |
55 |
< |
($\phi, \theta, \text{and} \psi$), where \textbf{A} is composed of |
54 |
> |
(\textbf{A}) can be described by the three Euler angles ($\phi, |
55 |
> |
\theta,$ and $\psi$), where the elements of \textbf{A} are composed of |
56 |
|
trigonometric operations involving $\phi, \theta,$ and |
57 |
< |
$\psi$.\cite{Goldstein01} In order to avoid rotational limitations |
57 |
> |
$\psi$.\cite{Goldstein01} In order to avoid numerical instabilities |
58 |
|
inherent in using the Euler angles, the four parameter ``quaternion'' |
59 |
< |
scheme can be used instead, where \textbf{A} is composed of arithmetic |
60 |
< |
operations involving the four components of a quaternion ($q_0, q_1, |
61 |
< |
q_2, \text{and} q_3$).\cite{allen87:csl} Use of quaternions also leads |
62 |
< |
to performance enhancements, particularly for very small |
59 |
> |
scheme is often used. The elements of \textbf{A} can be expressed as |
60 |
> |
arithmetic operations involving the four quaternions ($q_0, q_1, q_2,$ |
61 |
> |
and $q_3$).\cite{allen87:csl} Use of quaternions also leads to |
62 |
> |
performance enhancements, particularly for very small |
63 |
|
systems.\cite{Evans77} |
64 |
|
|
65 |
< |
{\sc OOPSE} utilizes a relatively new scheme that uses the entire nine |
66 |
< |
parameter rotation matrix internally. Further discussion on this |
67 |
< |
choice can be found in Sec.~\ref{sec:integrate}. |
65 |
> |
{\sc oopse} utilizes a relatively new scheme that propagates the |
66 |
> |
entire nine parameter rotation matrix internally. Further discussion |
67 |
> |
on this choice can be found in Sec.~\ref{sec:integrate}. |
68 |
|
|
69 |
|
\subsection{\label{sec:LJPot}The Lennard Jones Potential} |
70 |
|
|
271 |
|
\subsection{\label{sec:SSD}The {\sc DUFF} Water Models: SSD/E and SSD/RF} |
272 |
|
|
273 |
|
In the interest of computational efficiency, the default solvent used |
274 |
< |
in {\sc oopse} is the Soft Sticky Dipole (SSD) water model. SSD was |
275 |
< |
developed by Ichiye \emph{et al.} as a modified form of the |
276 |
< |
hard-sphere water model proposed by Bratko, Blum, and |
274 |
> |
by {\sc oopse} is the extended Soft Sticky Dipole (SSD/E) water |
275 |
> |
model.\cite{Gezelter04} The original SSD was developed by Ichiye |
276 |
> |
\emph{et al.}\cite{Ichiye96} as a modified form of the hard-sphere |
277 |
> |
water model proposed by Bratko, Blum, and |
278 |
|
Luzar.\cite{Bratko85,Bratko95} It consists of a single point dipole |
279 |
|
with a Lennard-Jones core and a sticky potential that directs the |
280 |
|
particles to assume the proper hydrogen bond orientation in the first |
333 |
|
{\it charged} multi-point models. In the original Monte Carlo |
334 |
|
simulations using this model, Ichiye {\it et al.} reported that using |
335 |
|
SSD decreased computer time by a factor of 6-7 compared to other |
336 |
< |
models.\cite{Ichiye96} What is most impressive is that this savings |
336 |
> |
models.\cite{Ichiye96} What is most impressive is that these savings |
337 |
|
did not come at the expense of accurate depiction of the liquid state |
338 |
|
properties. Indeed, SSD maintains reasonable agreement with the Soper |
339 |
< |
data for the structural features of liquid |
339 |
> |
diffraction data for the structural features of liquid |
340 |
|
water.\cite{Soper86,Ichiye96} Additionally, the dynamical properties |
341 |
|
exhibited by SSD agree with experiment better than those of more |
342 |
|
computationally expensive models (like TIP3P and |
347 |
|
Recent constant pressure simulations revealed issues in the original |
348 |
|
SSD model that led to lower than expected densities at all target |
349 |
|
pressures.\cite{Ichiye03,Gezelter04} The default model in {\sc oopse} |
350 |
< |
is SSD/E, a density corrected derivative of SSD that exhibits improved |
351 |
< |
liquid structure and transport behavior. If the use of a reaction |
352 |
< |
field long-range interaction correction is desired, it is recommended |
353 |
< |
that the parameters be modified to those of the SSD/RF model. Solvent |
354 |
< |
parameters can be easily modified in an accompanying {\sc BASS} file |
355 |
< |
as illustrated in the scheme below. A table of the parameter values |
356 |
< |
and the drawbacks and benefits of the different density corrected SSD |
357 |
< |
models can be found in reference \ref{Gezelter04}. |
350 |
> |
is therefore SSD/E, a density corrected derivative of SSD that |
351 |
> |
exhibits improved liquid structure and transport behavior. If the use |
352 |
> |
of a reaction field long-range interaction correction is desired, it |
353 |
> |
is recommended that the parameters be modified to those of the SSD/RF |
354 |
> |
model. Solvent parameters can be easily modified in an accompanying |
355 |
> |
{\sc BASS} file as illustrated in the scheme below. A table of the |
356 |
> |
parameter values and the drawbacks and benefits of the different |
357 |
> |
density corrected SSD models can be found in reference |
358 |
> |
\ref{Gezelter04}. |
359 |
|
|
360 |
|
!!!Place a {\sc BASS} scheme showing SSD parameters around here!!! |
361 |
|
|
390 |
|
$\rho_{i}$. $\phi_{ij}$ is a primarily repulsive pairwise interaction |
391 |
|
between atoms $i$ and $j$. In the original formulation of |
392 |
|
{\sc eam} cite{Daw84}, $\phi_{ij}$ was an entirely repulsive term, however |
393 |
< |
in later refinements to EAM have shown that nonuniqueness between $F$ |
393 |
> |
in later refinements to EAM have shown that non-uniqueness between $F$ |
394 |
|
and $\phi$ allow for more general forms for $\phi$.\cite{Daw89} |
395 |
|
There is a cutoff distance, $r_{cut}$, which limits the |
396 |
|
summations in the {\sc eam} equation to the few dozen atoms |
399 |
|
|
400 |
|
|
401 |
|
\subsection{\label{Sec:pbc}Periodic Boundary Conditions} |
402 |
+ |
|
403 |
+ |
\newcommand{\roundme}{\operatorname{round}} |
404 |
|
|
405 |
|
\textit{Periodic boundary conditions} are widely used to simulate truly |
406 |
|
macroscopic systems with a relatively small number of particles. The |
433 |
|
\end{equation} |
434 |
|
And then, each element of $\mathbf{s}$ is wrapped to lie between -0.5 to 0.5, |
435 |
|
\begin{equation} |
436 |
< |
s_{i}^{\prime}=s_{i}-round(s_{i}) |
436 |
> |
s_{i}^{\prime}=s_{i}-\roundme(s_{i}) |
437 |
|
\end{equation} |
438 |
|
where |
439 |
|
|
440 |
|
% |
441 |
|
|
442 |
|
\begin{equation} |
443 |
< |
round(x)=\left\{ |
444 |
< |
\begin{array}[c]{c}% |
443 |
> |
\roundme(x)=\left\{ |
444 |
> |
\begin{array}{cc} |
445 |
|
\lfloor{x+0.5}\rfloor & \text{if \ }x\geqslant0\\ |
446 |
|
\lceil{x-0.5}\rceil & \text{otherwise}% |
447 |
|
\end{array} |
448 |
|
\right. |
449 |
|
\end{equation} |
450 |
+ |
For example, $\roundme(3.6)=4$, $\roundme(3.1)=3$, $\roundme(-3.6)=-4$, |
451 |
+ |
$\roundme(-3.1)=-3$. |
452 |
|
|
446 |
– |
|
447 |
– |
For example, $round(3.6)=4$,$round(3.1)=3$, $round(-3.6)=-4$, |
448 |
– |
$round(-3.1)=-3$. |
449 |
– |
|
453 |
|
Finally, we obtain the minimum image coordinates by transforming back |
454 |
|
to real space,% |
455 |
|
|