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 |
|
|
388 |
|
$\rho_{i}$. $\phi_{ij}$ is a primarily repulsive pairwise interaction |
389 |
|
between atoms $i$ and $j$. In the original formulation of |
390 |
|
{\sc eam} cite{Daw84}, $\phi_{ij}$ was an entirely repulsive term, however |
391 |
< |
in later refinements to EAM have shown that nonuniqueness between $F$ |
391 |
> |
in later refinements to EAM have shown that non-uniqueness between $F$ |
392 |
|
and $\phi$ allow for more general forms for $\phi$.\cite{Daw89} |
393 |
|
There is a cutoff distance, $r_{cut}$, which limits the |
394 |
|
summations in the {\sc eam} equation to the few dozen atoms |