Skip to content

Commit 94db13d

Browse files
authored
Merge pull request #61 from MobleyLab/samar_edits
Samar edits and figure additions
2 parents 7753c90 + e61f30b commit 94db13d

File tree

4 files changed

+16
-4
lines changed

4 files changed

+16
-4
lines changed

paper/basic_training.pdf

27.6 KB
Binary file not shown.

paper/basic_training.tex

Lines changed: 16 additions & 4 deletions
Original file line numberDiff line numberDiff line change
@@ -1051,13 +1051,17 @@ \subsubsection{Motivation}
10511051

10521052
\subsubsection{ Ewald Summation}
10531053

1054-
One way of handling the aforementioned issues in an efficient manner is to use the Ewald summation technique (ref, Ewald 1921). To understand this technique, lets represent the relation between the charge distriution and the coulombic potential in the differntial form (Poisson equation) :
1054+
One way of handling the aforementioned issues in an efficient manner is to use the Ewald summation technique (ref, Ewald 1921). To understand this technique, lets represent the relation between the charge distribution and the coulombic potential in the differential form (Poisson equation) :
10551055

10561056
\[
10571057
\Delta \phi(\boldsymbol{x}) = - \frac{1}{\epsilon} \rho(\boldsymbol{x})
10581058
\]
10591059

1060-
where, $ \boldsymbol{x} \epsilon R^3 $ , $\phi(\boldsymbol{x})$ is the potential at point $\boldsymbol{x}$, $\rho(\boldsymbol{x})$ is the charge at point $\boldsymbol{x}$ and $\epsilon$ is the permissivity of the medium. This equation is an elliptical partial differential equation(pde) of the second order. The standard way to determine the potential from this equation is a two step method - discretization of the equation followed by solution. These techniques however depend on the smoothness of the functions - $\rho$ and $\phi$ - involved. However, in the case of charge distribution in our simulation system, $\rho$ is a set of delta functions which are clearly not smooth! As $\rho$ is not smooth, $\phi$ is not smooth either. \\
1060+
where, $\phi(\boldsymbol{x})$ is the potential at point $\boldsymbol{x}$, $\rho(\boldsymbol{x})$ is the charge density at point $\boldsymbol{x}$ and $\epsilon$ is the permissivity of the medium.
1061+
This equation is an elliptical partial differential equation(pde) of the second order.
1062+
The standard way to determine the potential from this equation is a two step method - discretization of the equation followed by solution. These techniques however depend on the smoothness of the functions - $\rho$ and $\phi$ - involved.
1063+
However, in the case of charge distribution in our simulation system, $\rho$ is a set of delta functions which are clearly not smooth!
1064+
As $\rho$ is not smooth, $\phi$ is not smooth either. \\
10611065

10621066

10631067
Ewald method is based on replacing the point charge distributions by smooth charge distributions in order to use the fast solvation techniques of the pde. The most common smooth function used in Ewald method is the gaussian distribution although other distributions have been used as well. Thus,
@@ -1071,8 +1075,8 @@ \subsubsection{ Ewald Summation}
10711075

10721076
\begin{figure}[h]
10731077
\centering
1074-
\includegraphics[width=\linewidth]{charges_ewald.pdf}
1075-
\caption{Point charges can be split into Direct space and reciprocal space charges. Direct space charge consists of the original charges and gaussian-distributed screening charge. Reciprocal space charge is only the gaussian-distributed charge.}
1078+
\includegraphics[width=\linewidth]{ewald.pdf}
1079+
\caption{Screening charge distribution. (top) Original charge distribution. (bottom)Point charges can be split into Direct space(blue) and Reciprocal space charges(red). Direct space charge consists of the original charges and gaussian-distributed screening charge. Reciprocal space charge is only the gaussian-distributed charge. }
10761080
\label{charges_ewald}
10771081
\end{figure}
10781082

@@ -1083,6 +1087,14 @@ \subsubsection{ Ewald Summation}
10831087

10841088
Unlike the potential due to the original charge, the potential due to direct space charge decays rapidly as shown in the figure. This is due to erfc function which decays very fast. Infact, it decays even faster than the Van der Waals term $r^{-6}$ and hence the cutoff used for Van der Waals can be used for direct space coulombic potential calculation as well.
10851089

1090+
\begin{figure}[h]
1091+
\centering
1092+
\includegraphics[width=\linewidth]{decay_comparison.pdf}
1093+
\caption{Comparison of decay of original $r^{-1}$ term(blue,*), erfc(r) in direct space(black,-) and $r^{-6}$ in van der waals term (red, -.). }
1094+
\label{charges_ewald}
1095+
\end{figure}
1096+
1097+
10861098
Potential due to the long range charge however doesn't decay rapidly and if calculated in the direct space would require summation over the infinite images. However, as we discussed earlier, the smoothness of the charge $\rho^{lr}$ (and hence potential ($\phi^{lr}$) allows the use of fast pde solvers. Fourier based solvers use the important result that differentiation operation in direct space corresponds to multiplication by (ik) in reciprocal space!
10871099

10881100
\[

paper/decay_comparison.pdf

3.15 KB
Binary file not shown.

paper/ewald.pdf

33.7 KB
Binary file not shown.

0 commit comments

Comments
 (0)