417 |
|
average will match the ensemble average, therefore two similar |
418 |
|
trajectories in phase space should give matching statistical averages. |
419 |
|
|
420 |
< |
\subsection{\label{introSec:MDfurtheeeeer}Further Considerations} |
420 |
> |
\subsection{\label{introSec:MDfurther}Further Considerations} |
421 |
|
In the simulations presented in this research, a few additional |
422 |
|
parameters are needed to describe the motions. The simulations |
423 |
|
involving water and phospholipids in Chapt.~\ref{chaptLipids} are |
428 |
|
$z$-axis, and $\theta$ is a rotation about the new $x$-axis, and |
429 |
|
$\psi$ is a final rotation about the new $z$-axis (see |
430 |
|
Fig.~\ref{introFig:euleerAngles}). This sequence of rotations can be |
431 |
< |
accumulated into a single $3\time3$ matrix $\underline{\mathbf{A}}$ |
431 |
> |
accumulated into a single $3 \times 3$ matrix $\mathbf{A}$ |
432 |
|
defined as follows: |
433 |
|
\begin{equation} |
434 |
|
eq here |
443 |
|
\end{equation} |
444 |
|
Where $\omega^s_i$ is the angular velocity in the lab space frame |
445 |
|
along cartesian coordinate $i$. However, a difficulty arises when |
446 |
< |
attempting to integrate Eq.~\ref{introEq:MDeuleerPhi} and |
446 |
> |
attempting to integrate Eq.~\ref{introEq:MDeulerPhi} and |
447 |
|
Eq.~\ref{introEq:MDeulerPsi}. The $\frac{1}{\sin \theta}$ present in |
448 |
|
both equations means there is a non-physical instability present when |
449 |
|
$\theta$ is 0 or $\pi$. |
450 |
|
|
451 |
|
To correct for this, the simulations integrate the rotation matrix, |
452 |
< |
$\underline{\mathbf{A}}$, directly, thus avoiding the instability. |
452 |
> |
$\mathbf{A}$, directly, thus avoiding the instability. |
453 |
|
This method was proposed by Dullwebber |
454 |
|
\emph{et. al.}\cite{Dullwebber:1997}, and is presented in |
455 |
|
Sec.~\ref{introSec:MDsymplecticRot}. |
456 |
|
|
457 |
|
\subsubsection{\label{introSec:MDliouville}Liouville Propagator} |
458 |
|
|
459 |
+ |
Before discussing the integration of the rotation matrix, it is |
460 |
+ |
necessary to understand the construction of a ``good'' integration |
461 |
+ |
scheme. It has been previously |
462 |
+ |
discussed(Sec.~\ref{introSec:MDintegrate}) how it is desirable for an |
463 |
+ |
integrator to be symplectic, or time reversible. The following is an |
464 |
+ |
outline of the Trotter factorization of the Liouville Propagator as a |
465 |
+ |
scheme for generating symplectic integrators. \cite{Tuckerman:1992} |
466 |
|
|
467 |
+ |
For a system with $f$ degrees of freedom the Liouville operator can be |
468 |
+ |
defined as, |
469 |
+ |
\begin{equation} |
470 |
+ |
eq here |
471 |
+ |
\label{introEq:LiouvilleOperator} |
472 |
+ |
\end{equation} |
473 |
+ |
Here, $r_j$ and $p_j$ are the position and conjugate momenta of a |
474 |
+ |
degree of freedom, and $f_j$ is the force on that degree of freedom. |
475 |
+ |
$\Gamma$ is defined as the set of all positions nad conjugate momenta, |
476 |
+ |
$\{r_j,p_j\}$, and the propagator, $U(t)$, is defined |
477 |
+ |
\begin {equation} |
478 |
+ |
eq here |
479 |
+ |
\label{introEq:Lpropagator} |
480 |
+ |
\end{equation} |
481 |
+ |
This allows the specification of $\Gamma$ at any time $t$ as |
482 |
+ |
\begin{equation} |
483 |
+ |
eq here |
484 |
+ |
\label{introEq:Lp2} |
485 |
+ |
\end{equation} |
486 |
+ |
It is important to note, $U(t)$ is a unitary operator meaning |
487 |
+ |
\begin{equation} |
488 |
+ |
U(-t)=U^{-1}(t) |
489 |
+ |
\label{introEq:Lp3} |
490 |
+ |
\end{equation} |
491 |
+ |
|
492 |
+ |
Decomposing $L$ into two parts, $iL_1$ and $iL_2$, one can use the |
493 |
+ |
Trotter theorem to yield |
494 |
+ |
\begin{equation} |
495 |
+ |
eq here |
496 |
+ |
\label{introEq:Lp4} |
497 |
+ |
\end{equation} |
498 |
+ |
Where $\Delta t = \frac{t}{P}$. |
499 |
+ |
With this, a discrete time operator $G(\Delta t)$ can be defined: |
500 |
+ |
\begin{equation} |
501 |
+ |
eq here |
502 |
+ |
\label{introEq:Lp5} |
503 |
+ |
\end{equation} |
504 |
+ |
Because $U_1(t)$ and $U_2(t)$ are unitary, $G|\Delta t)$ is also |
505 |
+ |
unitary. Meaning an integrator based on this factorization will be |
506 |
+ |
reversible in time. |
507 |
+ |
|
508 |
+ |
As an example, consider the following decomposition of $L$: |
509 |
+ |
\begin{equation} |
510 |
+ |
eq here |
511 |
+ |
\label{introEq:Lp6} |
512 |
+ |
\end{equation} |
513 |
+ |
Operating $G(\Delta t)$ on $\Gamma)0)$, and utilizing the operator property |
514 |
+ |
\begin{equation} |
515 |
+ |
eq here |
516 |
+ |
\label{introEq:Lp8} |
517 |
+ |
\end{equation} |
518 |
+ |
Where $c$ is independent of $q$. One obtains the following: |
519 |
+ |
\begin{equation} |
520 |
+ |
eq here |
521 |
+ |
\label{introEq:Lp8} |
522 |
+ |
\end{equation} |
523 |
+ |
Or written another way, |
524 |
+ |
\begin{equation} |
525 |
+ |
eq here |
526 |
+ |
\label{intorEq:Lp9} |
527 |
+ |
\end{equation} |
528 |
+ |
This is the velocity Verlet formulation presented in |
529 |
+ |
Sec.~\ref{introSec:MDintegrate}. Because this integration scheme is |
530 |
+ |
comprised of unitary propagators, it is symplectic, and therefore area |
531 |
+ |
preserving in phase space. From the preceeding fatorization, one can |
532 |
+ |
see that the integration of the equations of motion would follow: |
533 |
+ |
\begin{enumerate} |
534 |
+ |
\item calculate the velocities at the half step, $\frac{\Delta t}{2}$, from the forces calculated at the initial position. |
535 |
+ |
|
536 |
+ |
\item Use the half step velocities to move positions one whole step, $\Delta t$. |
537 |
+ |
|
538 |
+ |
\item Evaluate the forces at the new positions, $\mathbf{r}(\Delta t)$, and use the new forces to complete the velocity move. |
539 |
+ |
|
540 |
+ |
\item Repeat from step 1 with the new position, velocities, and forces assuming the roles of the initial values. |
541 |
+ |
\end{enumerate} |
542 |
+ |
|
543 |
+ |
\subsubsection{\label{introSec:MDsymplecticRot} Symplectic Propagation of the Rotation Matrix} |
544 |
+ |
|
545 |
+ |
Based on the factorization from the previous section, |
546 |
+ |
Dullweber\emph{et al.}\cite{Dullweber:1997}~ proposed a scheme for the |
547 |
+ |
symplectic propagation of the rotation matrix, $\mathbf{A}$, as an |
548 |
+ |
alternative method for the integration of orientational degrees of |
549 |
+ |
freedom. The method starts with a straightforward splitting of the |
550 |
+ |
Liouville operator: |
551 |
+ |
\begin{equation} |
552 |
+ |
eq here |
553 |
+ |
\label{introEq:SR1} |
554 |
+ |
\end{equation} |
555 |
+ |
Where $\boldsymbol{\tau}(\mathbf{A})$ are the tourques of the system |
556 |
+ |
due to the configuration, and $\boldsymbol{/pi}$ are the conjugate |
557 |
+ |
angular momenta of the system. The propagator, $G(\Delta t)$, becomes |
558 |
+ |
\begin{equation} |
559 |
+ |
eq here |
560 |
+ |
\label{introEq:SR2} |
561 |
+ |
\end{equation} |
562 |
+ |
Propagation fo the linear and angular momenta follows as in the Verlet |
563 |
+ |
scheme. The propagation of positions also follows the verlet scheme |
564 |
+ |
with the addition of a further symplectic splitting of the rotation |
565 |
+ |
matrix propagation, $\mathcal{G}_{\text{rot}}(\Delta t)$. |
566 |
+ |
\begin{equation} |
567 |
+ |
eq here |
568 |
+ |
\label{introEq:SR3} |
569 |
+ |
\end{equation} |
570 |
+ |
Where $\mathcal{G}_j$ is a unitary rotation of $\mathbf{A}$ and |
571 |
+ |
$\boldsymbol{\pi}$ about each axis $j$. As all propagations are now |
572 |
+ |
unitary and symplectic, the entire integration scheme is also |
573 |
+ |
symplectic and time reversible. |
574 |
+ |
|
575 |
|
\section{\label{introSec:chapterLayout}Chapter Layout} |
576 |
|
|
577 |
|
\subsection{\label{introSec:RSA}Random Sequential Adsorption} |