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4   \usepackage{endfloat}
5 < \usepackage{amsmath}
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7   \usepackage{epsf}
8   \usepackage{times}
9 < \usepackage{mathptm}
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10   \usepackage{setspace}
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13 + \usepackage{booktabs}
14 + \usepackage{bibentry}
15 + \usepackage{mathrsfs}
16   \usepackage[ref]{overcite}
17   \pagestyle{plain}
18   \pagenumbering{arabic}
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25  
26   \begin{document}
27  
28 < \title{On the necessity of the Ewald Summation in molecular simulations.}
28 > \title{Is the Ewald Summation necessary? Pairwise alternatives to the accepted standard for long-range electrostatics}
29  
30 < \author{Christopher J. Fennell and J. Daniel Gezelter \\
30 > \author{Christopher J. Fennell and J. Daniel Gezelter\footnote{Corresponding author. \ Electronic mail:
31 > gezelter@nd.edu} \\
32   Department of Chemistry and Biochemistry\\
33   University of Notre Dame\\
34   Notre Dame, Indiana 46556}
# Line 30 | Line 36 | Notre Dame, Indiana 46556}
36   \date{\today}
37  
38   \maketitle
39 < %\doublespacing
39 > \doublespacing
40  
41 + \nobibliography{}
42   \begin{abstract}
43 + A new method for accumulating electrostatic interactions was derived
44 + from the previous efforts described in \bibentry{Wolf99} and
45 + \bibentry{Zahn02} as a possible replacement for lattice sum methods in
46 + molecular simulations.  Comparisons were performed with this and other
47 + pairwise electrostatic summation techniques against the smooth
48 + particle mesh Ewald (SPME) summation to see how well they reproduce
49 + the energetics and dynamics of a variety of simulation types.  The
50 + newly derived Shifted-Force technique shows a remarkable ability to
51 + reproduce the behavior exhibited in simulations using SPME with an
52 + $\mathscr{O}(N)$ computational cost, equivalent to merely the
53 + real-space portion of the lattice summation.
54 +
55   \end{abstract}
56  
57 + \newpage
58 +
59   %\narrowtext
60  
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62   %                              BODY OF TEXT
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64  
65   \section{Introduction}
66  
67 + In molecular simulations, proper accumulation of the electrostatic
68 + interactions is essential and is one of the most
69 + computationally-demanding tasks.  The common molecular mechanics force
70 + fields represent atomic sites with full or partial charges protected
71 + by Lennard-Jones (short range) interactions.  This means that nearly
72 + every pair interaction involves a calculation of charge-charge forces.
73 + Coupled with relatively long-ranged $r^{-1}$ decay, the monopole
74 + interactions quickly become the most expensive part of molecular
75 + simulations.  Historically, the electrostatic pair interaction would
76 + not have decayed appreciably within the typical box lengths that could
77 + be feasibly simulated.  In the larger systems that are more typical of
78 + modern simulations, large cutoffs should be used to incorporate
79 + electrostatics correctly.
80 +
81 + There have been many efforts to address the proper and practical
82 + handling of electrostatic interactions, and these have resulted in a
83 + variety of techniques.\cite{Roux99,Sagui99,Tobias01} These are
84 + typically classified as implicit methods (i.e., continuum dielectrics,
85 + static dipolar fields),\cite{Born20,Grossfield00} explicit methods
86 + (i.e., Ewald summations, interaction shifting or
87 + truncation),\cite{Ewald21,Steinbach94} or a mixture of the two (i.e.,
88 + reaction field type methods, fast multipole
89 + methods).\cite{Onsager36,Rokhlin85} The explicit or mixed methods are
90 + often preferred because they physically incorporate solvent molecules
91 + in the system of interest, but these methods are sometimes difficult
92 + to utilize because of their high computational cost.\cite{Roux99} In
93 + addition to the computational cost, there have been some questions
94 + regarding possible artifacts caused by the inherent periodicity of the
95 + explicit Ewald summation.\cite{Tobias01}
96 +
97 + In this paper, we focus on a new set of shifted methods devised by
98 + Wolf {\it et al.},\cite{Wolf99} which we further extend.  These
99 + methods along with a few other mixed methods (i.e. reaction field) are
100 + compared with the smooth particle mesh Ewald
101 + sum,\cite{Onsager36,Essmann99} which is our reference method for
102 + handling long-range electrostatic interactions. The new methods for
103 + handling electrostatics have the potential to scale linearly with
104 + increasing system size since they involve only a simple modification
105 + to the direct pairwise sum.  They also lack the added periodicity of
106 + the Ewald sum, so they can be used for systems which are non-periodic
107 + or which have one- or two-dimensional periodicity.  Below, these
108 + methods are evaluated using a variety of model systems to establish
109 + their usability in molecular simulations.
110 +
111 + \subsection{The Ewald Sum}
112 + The complete accumulation electrostatic interactions in a system with
113 + periodic boundary conditions (PBC) requires the consideration of the
114 + effect of all charges within a (cubic) simulation box as well as those
115 + in the periodic replicas,
116 + \begin{equation}
117 + V_\textrm{elec} = \frac{1}{2} {\sum_{\mathbf{n}}}^\prime \left[ \sum_{i=1}^N\sum_{j=1}^N \phi\left( \mathbf{r}_{ij} + L\mathbf{n},\bm{\Omega}_i,\bm{\Omega}_j\right) \right],
118 + \label{eq:PBCSum}
119 + \end{equation}
120 + where the sum over $\mathbf{n}$ is a sum over all periodic box
121 + replicas with integer coordinates $\mathbf{n} = (l,m,n)$, and the
122 + prime indicates $i = j$ are neglected for $\mathbf{n} =
123 + 0$.\cite{deLeeuw80} Within the sum, $N$ is the number of electrostatic
124 + particles, $\mathbf{r}_{ij}$ is $\mathbf{r}_j - \mathbf{r}_i$, $L$ is
125 + the cell length, $\bm{\Omega}_{i,j}$ are the Euler angles for $i$ and
126 + $j$, and $\phi$ is the solution to Poisson's equation
127 + ($\phi(\mathbf{r}_{ij}) = q_i q_j |\mathbf{r}_{ij}|^{-1}$ for
128 + charge-charge interactions). In the case of monopole electrostatics,
129 + eq. (\ref{eq:PBCSum}) is conditionally convergent and is divergent for
130 + non-neutral systems.
131 +
132 + The electrostatic summation problem was originally studied by Ewald
133 + for the case of an infinite crystal.\cite{Ewald21}. The approach he
134 + took was to convert this conditionally convergent sum into two
135 + absolutely convergent summations: a short-ranged real-space summation
136 + and a long-ranged reciprocal-space summation,
137 + \begin{equation}
138 + \begin{split}
139 + V_\textrm{elec} = \frac{1}{2}& \sum_{i=1}^N\sum_{j=1}^N \Biggr[ q_i q_j\Biggr( {\sum_{\mathbf{n}}}^\prime \frac{\textrm{erfc}\left( \alpha|\mathbf{r}_{ij}+\mathbf{n}|\right)}{|\mathbf{r}_{ij}+\mathbf{n}|} \\ &+ \frac{1}{\pi L^3}\sum_{\mathbf{k}\ne 0}\frac{4\pi^2}{|\mathbf{k}|^2} \exp{\left(-\frac{\pi^2|\mathbf{k}|^2}{\alpha^2}\right) \cos\left(\mathbf{k}\cdot\mathbf{r}_{ij}\right)}\Biggr)\Biggr] \\ &- \frac{\alpha}{\pi^{1/2}}\sum_{i=1}^N q_i^2 + \frac{2\pi}{(2\epsilon_\textrm{S}+1)L^3}\left|\sum_{i=1}^N q_i\mathbf{r}_i\right|^2,
140 + \end{split}
141 + \label{eq:EwaldSum}
142 + \end{equation}
143 + where $\alpha$ is the damping or convergence parameter with units of
144 + \AA$^{-1}$, $\mathbf{k}$ are the reciprocal vectors and are equal to
145 + $2\pi\mathbf{n}/L^2$, and $\epsilon_\textrm{S}$ is the dielectric
146 + constant of the surrounding medium. The final two terms of
147 + eq. (\ref{eq:EwaldSum}) are a particle-self term and a dipolar term
148 + for interacting with a surrounding dielectric.\cite{Allen87} This
149 + dipolar term was neglected in early applications in molecular
150 + simulations,\cite{Brush66,Woodcock71} until it was introduced by de
151 + Leeuw {\it et al.} to address situations where the unit cell has a
152 + dipole moment which is magnified through replication of the periodic
153 + images.\cite{deLeeuw80,Smith81} If this term is taken to be zero, the
154 + system is said to be using conducting (or ``tin-foil'') boundary
155 + conditions, $\epsilon_{\rm S} = \infty$. Figure
156 + \ref{fig:ewaldTime} shows how the Ewald sum has been applied over
157 + time.  Initially, due to the small sizes of the systems that could be
158 + feasibly simulated, the entire simulation box was replicated to
159 + convergence.  In more modern simulations, the simulation boxes have
160 + grown large enough that a real-space cutoff could potentially give
161 + convergent behavior.  Indeed, it has often been observed that the
162 + reciprocal-space portion of the Ewald sum can be small and rapidly
163 + convergent compared to the real-space portion with the choice of small
164 + $\alpha$.\cite{Karasawa89,Kolafa92}
165 +
166 + \begin{figure}
167 + \centering
168 + \includegraphics[width = \linewidth]{./ewaldProgression.pdf}
169 + \caption{How the application of the Ewald summation has changed with
170 + the increase in computer power.  Initially, only small numbers of
171 + particles could be studied, and the Ewald sum acted to replicate the
172 + unit cell charge distribution out to convergence.  Now, much larger
173 + systems of charges are investigated with fixed distance cutoffs.  The
174 + calculated structure factor is used to sum out to great distance, and
175 + a surrounding dielectric term is included.}
176 + \label{fig:ewaldTime}
177 + \end{figure}
178 +
179 + The original Ewald summation is an $\mathscr{O}(N^2)$ algorithm.  The
180 + convergence parameter $(\alpha)$ plays an important role in balancing
181 + the computational cost between the direct and reciprocal-space
182 + portions of the summation.  The choice of this value allows one to
183 + select whether the real-space or reciprocal space portion of the
184 + summation is an $\mathscr{O}(N^2)$ calculation (with the other being
185 + $\mathscr{O}(N)$).\cite{Sagui99} With the appropriate choice of
186 + $\alpha$ and thoughtful algorithm development, this cost can be
187 + reduced to $\mathscr{O}(N^{3/2})$.\cite{Perram88} The typical route
188 + taken to reduce the cost of the Ewald summation even further is to set
189 + $\alpha$ such that the real-space interactions decay rapidly, allowing
190 + for a short spherical cutoff. Then the reciprocal space summation is
191 + optimized.  These optimizations usually involve utilization of the
192 + fast Fourier transform (FFT),\cite{Hockney81} leading to the
193 + particle-particle particle-mesh (P3M) and particle mesh Ewald (PME)
194 + methods.\cite{Shimada93,Luty94,Luty95,Darden93,Essmann95} In these
195 + methods, the cost of the reciprocal-space portion of the Ewald
196 + summation is reduced from $\mathscr{O}(N^2)$ down to $\mathscr{O}(N
197 + \log N)$.
198 +
199 + These developments and optimizations have made the use of the Ewald
200 + summation routine in simulations with periodic boundary
201 + conditions. However, in certain systems, such as vapor-liquid
202 + interfaces and membranes, the intrinsic three-dimensional periodicity
203 + can prove problematic.  The Ewald sum has been reformulated to handle
204 + 2D systems,\cite{Parry75,Parry76,Heyes77,deLeeuw79,Rhee89}, but the
205 + new methods are computationally expensive.\cite{Spohr97,Yeh99}
206 + Inclusion of a correction term in the Ewald summation is a possible
207 + direction for handling 2D systems while still enabling the use of the
208 + modern optimizations.\cite{Yeh99}
209 +
210 + Several studies have recognized that the inherent periodicity in the
211 + Ewald sum can also have an effect on three-dimensional
212 + systems.\cite{Roberts94,Roberts95,Luty96,Hunenberger99a,Hunenberger99b,Weber00}
213 + Solvated proteins are essentially kept at high concentration due to
214 + the periodicity of the electrostatic summation method.  In these
215 + systems, the more compact folded states of a protein can be
216 + artificially stabilized by the periodic replicas introduced by the
217 + Ewald summation.\cite{Weber00} Thus, care must be taken when
218 + considering the use of the Ewald summation where the assumed
219 + periodicity would introduce spurious effects in the system dynamics.
220 +
221 + \subsection{The Wolf and Zahn Methods}
222 + In a recent paper by Wolf \textit{et al.}, a procedure was outlined
223 + for the accurate accumulation of electrostatic interactions in an
224 + efficient pairwise fashion.  This procedure lacks the inherent
225 + periodicity of the Ewald summation.\cite{Wolf99} Wolf \textit{et al.}
226 + observed that the electrostatic interaction is effectively
227 + short-ranged in condensed phase systems and that neutralization of the
228 + charge contained within the cutoff radius is crucial for potential
229 + stability. They devised a pairwise summation method that ensures
230 + charge neutrality and gives results similar to those obtained with the
231 + Ewald summation.  The resulting shifted Coulomb potential
232 + (Eq. \ref{eq:WolfPot}) includes image-charges subtracted out through
233 + placement on the cutoff sphere and a distance-dependent damping
234 + function (identical to that seen in the real-space portion of the
235 + Ewald sum) to aid convergence
236 + \begin{equation}
237 + V_{\textrm{Wolf}}(r_{ij})= \frac{q_i q_j \textrm{erfc}(\alpha r_{ij})}{r_{ij}}-\lim_{r_{ij}\rightarrow R_\textrm{c}}\left\{\frac{q_iq_j \textrm{erfc}(\alpha r_{ij})}{r_{ij}}\right\}.
238 + \label{eq:WolfPot}
239 + \end{equation}
240 + Eq. (\ref{eq:WolfPot}) is essentially the common form of a shifted
241 + potential.  However, neutralizing the charge contained within each
242 + cutoff sphere requires the placement of a self-image charge on the
243 + surface of the cutoff sphere.  This additional self-term in the total
244 + potential enabled Wolf {\it et al.}  to obtain excellent estimates of
245 + Madelung energies for many crystals.
246 +
247 + In order to use their charge-neutralized potential in molecular
248 + dynamics simulations, Wolf \textit{et al.} suggested taking the
249 + derivative of this potential prior to evaluation of the limit.  This
250 + procedure gives an expression for the forces,
251 + \begin{equation}
252 + F_{\textrm{Wolf}}(r_{ij}) = q_i q_j\left\{\left[\frac{\textrm{erfc}\left(\alpha r_{ij}\right)}{r^2_{ij}}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp{\left(-\alpha^2r_{ij}^2\right)}}{r_{ij}}\right]-\left[\frac{\textrm{erfc}\left(\alpha R_{\textrm{c}}\right)}{R_{\textrm{c}}^2}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp{\left(-\alpha^2R_{\textrm{c}}^2\right)}}{R_{\textrm{c}}}\right]\right\},
253 + \label{eq:WolfForces}
254 + \end{equation}
255 + that incorporates both image charges and damping of the electrostatic
256 + interaction.
257 +
258 + More recently, Zahn \textit{et al.} investigated these potential and
259 + force expressions for use in simulations involving water.\cite{Zahn02}
260 + In their work, they pointed out that the forces and derivative of
261 + the potential are not commensurate.  Attempts to use both
262 + eqs. (\ref{eq:WolfPot}) and (\ref{eq:WolfForces}) together will lead
263 + to poor energy conservation.  They correctly observed that taking the
264 + limit shown in equation (\ref{eq:WolfPot}) {\it after} calculating the
265 + derivatives gives forces for a different potential energy function
266 + than the one shown in eq. (\ref{eq:WolfPot}).
267 +
268 + Zahn \textit{et al.} introduced a modified form of this summation
269 + method as a way to use the technique in Molecular Dynamics
270 + simulations.  They proposed a new damped Coulomb potential,
271 + \begin{equation}
272 + V_{\textrm{Zahn}}(r_{ij}) = q_iq_j\left\{\frac{\mathrm{erfc}\left(\alpha r_{ij}\right)}{r_{ij}}-\left[\frac{\mathrm{erfc}\left(\alpha R_\mathrm{c}\right)}{R_\mathrm{c}^2}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp\left(-\alpha^2R_\mathrm{c}^2\right)}{R_\mathrm{c}}\right]\left(r_{ij}-R_\mathrm{c}\right)\right\},
273 + \label{eq:ZahnPot}
274 + \end{equation}
275 + and showed that this potential does fairly well at capturing the
276 + structural and dynamic properties of water compared the same
277 + properties obtained using the Ewald sum.
278 +
279 + \subsection{Simple Forms for Pairwise Electrostatics}
280 +
281 + The potentials proposed by Wolf \textit{et al.} and Zahn \textit{et
282 + al.} are constructed using two different (and separable) computational
283 + tricks: \begin{enumerate}
284 + \item shifting through the use of image charges, and
285 + \item damping the electrostatic interaction.
286 + \end{enumerate}  Wolf \textit{et al.} treated the
287 + development of their summation method as a progressive application of
288 + these techniques,\cite{Wolf99} while Zahn \textit{et al.} founded
289 + their damped Coulomb modification (Eq. (\ref{eq:ZahnPot})) on the
290 + post-limit forces (Eq. (\ref{eq:WolfForces})) which were derived using
291 + both techniques.  It is possible, however, to separate these
292 + tricks and study their effects independently.
293 +
294 + Starting with the original observation that the effective range of the
295 + electrostatic interaction in condensed phases is considerably less
296 + than $r^{-1}$, either the cutoff sphere neutralization or the
297 + distance-dependent damping technique could be used as a foundation for
298 + a new pairwise summation method.  Wolf \textit{et al.} made the
299 + observation that charge neutralization within the cutoff sphere plays
300 + a significant role in energy convergence; therefore we will begin our
301 + analysis with the various shifted forms that maintain this charge
302 + neutralization.  We can evaluate the methods of Wolf
303 + \textit{et al.}  and Zahn \textit{et al.} by considering the standard
304 + shifted potential,
305 + \begin{equation}
306 + V_\textrm{SP}(r) =      \begin{cases}
307 + v(r)-v_\textrm{c} &\quad r\leqslant R_\textrm{c} \\ 0 &\quad r >
308 + R_\textrm{c}  
309 + \end{cases},
310 + \label{eq:shiftingPotForm}
311 + \end{equation}
312 + and shifted force,
313 + \begin{equation}
314 + V_\textrm{SF}(r) =      \begin{cases}
315 + v(r)-v_\textrm{c}-\left(\frac{d v(r)}{d r}\right)_{r=R_\textrm{c}}(r-R_\textrm{c})
316 + &\quad r\leqslant R_\textrm{c} \\ 0 &\quad r > R_\textrm{c}
317 +                                                \end{cases},
318 + \label{eq:shiftingForm}
319 + \end{equation}
320 + functions where $v(r)$ is the unshifted form of the potential, and
321 + $v_c$ is $v(R_\textrm{c})$.  The Shifted Force ({\sc sf}) form ensures
322 + that both the potential and the forces goes to zero at the cutoff
323 + radius, while the Shifted Potential ({\sc sp}) form only ensures the
324 + potential is smooth at the cutoff radius
325 + ($R_\textrm{c}$).\cite{Allen87}
326 +
327 + The forces associated with the shifted potential are simply the forces
328 + of the unshifted potential itself (when inside the cutoff sphere),
329 + \begin{equation}
330 + F_{\textrm{SP}} = -\left( \frac{d v(r)}{dr} \right),
331 + \end{equation}
332 + and are zero outside.  Inside the cutoff sphere, the forces associated
333 + with the shifted force form can be written,
334 + \begin{equation}
335 + F_{\textrm{SF}} = -\left( \frac{d v(r)}{dr} \right) + \left(\frac{d
336 + v(r)}{dr} \right)_{r=R_\textrm{c}}.
337 + \end{equation}
338 +
339 + If the potential, $v(r)$, is taken to be the normal Coulomb potential,
340 + \begin{equation}
341 + v(r) = \frac{q_i q_j}{r},
342 + \label{eq:Coulomb}
343 + \end{equation}
344 + then the Shifted Potential ({\sc sp}) forms will give Wolf {\it et
345 + al.}'s undamped prescription:
346 + \begin{equation}
347 + V_\textrm{SP}(r) =
348 + q_iq_j\left(\frac{1}{r}-\frac{1}{R_\textrm{c}}\right) \quad
349 + r\leqslant R_\textrm{c},
350 + \label{eq:SPPot}
351 + \end{equation}
352 + with associated forces,
353 + \begin{equation}
354 + F_\textrm{SP}(r) = q_iq_j\left(\frac{1}{r^2}\right) \quad r\leqslant R_\textrm{c}.
355 + \label{eq:SPForces}
356 + \end{equation}
357 + These forces are identical to the forces of the standard Coulomb
358 + interaction, and cutting these off at $R_c$ was addressed by Wolf
359 + \textit{et al.} as undesirable.  They pointed out that the effect of
360 + the image charges is neglected in the forces when this form is
361 + used,\cite{Wolf99} thereby eliminating any benefit from the method in
362 + molecular dynamics.  Additionally, there is a discontinuity in the
363 + forces at the cutoff radius which results in energy drift during MD
364 + simulations.
365 +
366 + The shifted force ({\sc sf}) form using the normal Coulomb potential
367 + will give,
368 + \begin{equation}
369 + V_\textrm{SF}(r) = q_iq_j\left[\frac{1}{r}-\frac{1}{R_\textrm{c}}+\left(\frac{1}{R_\textrm{c}^2}\right)(r-R_\textrm{c})\right] \quad r\leqslant R_\textrm{c}.
370 + \label{eq:SFPot}
371 + \end{equation}
372 + with associated forces,
373 + \begin{equation}
374 + F_\textrm{SF}(r) =  q_iq_j\left(\frac{1}{r^2}-\frac{1}{R_\textrm{c}^2}\right) \quad r\leqslant R_\textrm{c}.
375 + \label{eq:SFForces}
376 + \end{equation}
377 + This formulation has the benefits that there are no discontinuities at
378 + the cutoff radius, while the neutralizing image charges are present in
379 + both the energy and force expressions.  It would be simple to add the
380 + self-neutralizing term back when computing the total energy of the
381 + system, thereby maintaining the agreement with the Madelung energies.
382 + A side effect of this treatment is the alteration in the shape of the
383 + potential that comes from the derivative term.  Thus, a degree of
384 + clarity about agreement with the empirical potential is lost in order
385 + to gain functionality in dynamics simulations.
386 +
387 + Wolf \textit{et al.} originally discussed the energetics of the
388 + shifted Coulomb potential (Eq. \ref{eq:SPPot}) and found that it was
389 + insufficient for accurate determination of the energy with reasonable
390 + cutoff distances.  The calculated Madelung energies fluctuated around
391 + the expected value as the cutoff radius was increased, but the
392 + oscillations converged toward the correct value.\cite{Wolf99} A
393 + damping function was incorporated to accelerate the convergence; and
394 + though alternative forms for the damping function could be
395 + used,\cite{Jones56,Heyes81} the complimentary error function was
396 + chosen to mirror the effective screening used in the Ewald summation.
397 + Incorporating this error function damping into the simple Coulomb
398 + potential,
399 + \begin{equation}
400 + v(r) = \frac{\mathrm{erfc}\left(\alpha r\right)}{r},
401 + \label{eq:dampCoulomb}
402 + \end{equation}
403 + the shifted potential (eq. (\ref{eq:SPPot})) becomes
404 + \begin{equation}
405 + V_{\textrm{DSP}}(r) = q_iq_j\left(\frac{\textrm{erfc}\left(\alpha r\right)}{r}-\frac{\textrm{erfc}\left(\alpha R_\textrm{c}\right)}{R_\textrm{c}}\right) \quad r\leqslant R_\textrm{c},
406 + \label{eq:DSPPot}
407 + \end{equation}
408 + with associated forces,
409 + \begin{equation}
410 + F_{\textrm{DSP}}(r) = q_iq_j\left(\frac{\textrm{erfc}\left(\alpha r\right)}{r^2}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp{\left(-\alpha^2r^2\right)}}{r}\right) \quad r\leqslant R_\textrm{c}.
411 + \label{eq:DSPForces}
412 + \end{equation}
413 + Again, this damped shifted potential suffers from a
414 + force-discontinuity at the cutoff radius, and the image charges play
415 + no role in the forces.  To remedy these concerns, one may derive a
416 + {\sc sf} variant by including the derivative term in
417 + eq. (\ref{eq:shiftingForm}),
418 + \begin{equation}
419 + \begin{split}
420 + V_\mathrm{DSF}(r) = q_iq_j\Biggr{[}&\frac{\mathrm{erfc}\left(\alpha r\right)}{r}-\frac{\mathrm{erfc}\left(\alpha R_\mathrm{c}\right)}{R_\mathrm{c}} \\ &\left.+\left(\frac{\mathrm{erfc}\left(\alpha R_\mathrm{c}\right)}{R_\mathrm{c}^2}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp\left(-\alpha^2R_\mathrm{c}^2\right)}{R_\mathrm{c}}\right)\left(r-R_\mathrm{c}\right)\ \right] \quad r\leqslant R_\textrm{c}.
421 + \label{eq:DSFPot}
422 + \end{split}
423 + \end{equation}
424 + The derivative of the above potential will lead to the following forces,
425 + \begin{equation}
426 + \begin{split}
427 + F_\mathrm{DSF}(r) = q_iq_j\Biggr{[}&\left(\frac{\textrm{erfc}\left(\alpha r\right)}{r^2}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp{\left(-\alpha^2r^2\right)}}{r}\right) \\ &\left.-\left(\frac{\textrm{erfc}\left(\alpha R_{\textrm{c}}\right)}{R_{\textrm{c}}^2}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp{\left(-\alpha^2R_{\textrm{c}}^2\right)}}{R_{\textrm{c}}}\right)\right] \quad r\leqslant R_\textrm{c}.
428 + \label{eq:DSFForces}
429 + \end{split}
430 + \end{equation}
431 + If the damping parameter $(\alpha)$ is set to zero, the undamped case,
432 + eqs. (\ref{eq:SPPot} through \ref{eq:SFForces}) are correctly
433 + recovered from eqs. (\ref{eq:DSPPot} through \ref{eq:DSFForces}).
434 +
435 + This new {\sc sf} potential is similar to equation \ref{eq:ZahnPot}
436 + derived by Zahn \textit{et al.}; however, there are two important
437 + differences.\cite{Zahn02} First, the $v_\textrm{c}$ term from
438 + eq. (\ref{eq:shiftingForm}) is equal to eq. (\ref{eq:dampCoulomb})
439 + with $r$ replaced by $R_\textrm{c}$.  This term is {\it not} present
440 + in the Zahn potential, resulting in a potential discontinuity as
441 + particles cross $R_\textrm{c}$.  Second, the sign of the derivative
442 + portion is different.  The missing $v_\textrm{c}$ term would not
443 + affect molecular dynamics simulations (although the computed energy
444 + would be expected to have sudden jumps as particle distances crossed
445 + $R_c$).  The sign problem is a potential source of errors, however.
446 + In fact, it introduces a discontinuity in the forces at the cutoff,
447 + because the force function is shifted in the wrong direction and
448 + doesn't cross zero at $R_\textrm{c}$.
449 +
450 + Eqs. (\ref{eq:DSFPot}) and (\ref{eq:DSFForces}) result in an
451 + electrostatic summation method in which the potential and forces are
452 + continuous at the cutoff radius and which incorporates the damping
453 + function proposed by Wolf \textit{et al.}\cite{Wolf99} In the rest of
454 + this paper, we will evaluate exactly how good these methods ({\sc sp},
455 + {\sc sf}, damping) are at reproducing the correct electrostatic
456 + summation performed by the Ewald sum.
457 +
458 + \subsection{Other alternatives}
459 + In addition to the methods described above, we considered some other
460 + techniques that are commonly used in molecular simulations.  The
461 + simplest of these is group-based cutoffs.  Though of little use for
462 + charged molecules, collecting atoms into neutral groups takes
463 + advantage of the observation that the electrostatic interactions decay
464 + faster than those for monopolar pairs.\cite{Steinbach94} When
465 + considering these molecules as neutral groups, the relative
466 + orientations of the molecules control the strength of the interactions
467 + at the cutoff radius.  Consequently, as these molecular particles move
468 + through $R_\textrm{c}$, the energy will drift upward due to the
469 + anisotropy of the net molecular dipole interactions.\cite{Rahman71} To
470 + maintain good energy conservation, both the potential and derivative
471 + need to be smoothly switched to zero at $R_\textrm{c}$.\cite{Adams79}
472 + This is accomplished using a standard switching function.  If a smooth
473 + second derivative is desired, a fifth (or higher) order polynomial can
474 + be used.\cite{Andrea83}
475 +
476 + Group-based cutoffs neglect the surroundings beyond $R_\textrm{c}$,
477 + and to incorporate the effects of the surroundings, a method like
478 + Reaction Field ({\sc rf}) can be used.  The original theory for {\sc
479 + rf} was originally developed by Onsager,\cite{Onsager36} and it was
480 + applied in simulations for the study of water by Barker and
481 + Watts.\cite{Barker73} In modern simulation codes, {\sc rf} is simply
482 + an extension of the group-based cutoff method where the net dipole
483 + within the cutoff sphere polarizes an external dielectric, which
484 + reacts back on the central dipole.  The same switching function
485 + considerations for group-based cutoffs need to made for {\sc rf}, with
486 + the additional pre-specification of a dielectric constant.
487 +
488   \section{Methods}
489 +
490 + In classical molecular mechanics simulations, there are two primary
491 + techniques utilized to obtain information about the system of
492 + interest: Monte Carlo (MC) and Molecular Dynamics (MD).  Both of these
493 + techniques utilize pairwise summations of interactions between
494 + particle sites, but they use these summations in different ways.
495 +
496 + In MC, the potential energy difference between configurations dictates
497 + the progression of MC sampling.  Going back to the origins of this
498 + method, the acceptance criterion for the canonical ensemble laid out
499 + by Metropolis \textit{et al.} states that a subsequent configuration
500 + is accepted if $\Delta E < 0$ or if $\xi < \exp(-\Delta E/kT)$, where
501 + $\xi$ is a random number between 0 and 1.\cite{Metropolis53}
502 + Maintaining the correct $\Delta E$ when using an alternate method for
503 + handling the long-range electrostatics will ensure proper sampling
504 + from the ensemble.
505 +
506 + In MD, the derivative of the potential governs how the system will
507 + progress in time.  Consequently, the force and torque vectors on each
508 + body in the system dictate how the system evolves.  If the magnitude
509 + and direction of these vectors are similar when using alternate
510 + electrostatic summation techniques, the dynamics in the short term
511 + will be indistinguishable.  Because error in MD calculations is
512 + cumulative, one should expect greater deviation at longer times,
513 + although methods which have large differences in the force and torque
514 + vectors will diverge from each other more rapidly.
515 +
516 + \subsection{Monte Carlo and the Energy Gap}\label{sec:MCMethods}
517 +
518 + The pairwise summation techniques (outlined in section
519 + \ref{sec:ESMethods}) were evaluated for use in MC simulations by
520 + studying the energy differences between conformations.  We took the
521 + SPME-computed energy difference between two conformations to be the
522 + correct behavior. An ideal performance by an alternative method would
523 + reproduce these energy differences exactly (even if the absolute
524 + energies calculated by the methods are different).  Since none of the
525 + methods provide exact energy differences, we used linear least squares
526 + regressions of energy gap data to evaluate how closely the methods
527 + mimicked the Ewald energy gaps.  Unitary results for both the
528 + correlation (slope) and correlation coefficient for these regressions
529 + indicate perfect agreement between the alternative method and SPME.
530 + Sample correlation plots for two alternate methods are shown in
531 + Fig. \ref{fig:linearFit}.
532 +
533 + \begin{figure}
534 + \centering
535 + \includegraphics[width = \linewidth]{./dualLinear.pdf}
536 + \caption{Example least squares regressions of the configuration energy
537 + differences for SPC/E water systems. The upper plot shows a data set
538 + with a poor correlation coefficient ($R^2$), while the lower plot
539 + shows a data set with a good correlation coefficient.}
540 + \label{fig:linearFit}
541 + \end{figure}
542 +
543 + Each system type (detailed in section \ref{sec:RepSims}) was
544 + represented using 500 independent configurations.  Additionally, we
545 + used seven different system types, so each of the alternative
546 + (non-Ewald) electrostatic summation methods was evaluated using
547 + 873,250 configurational energy differences.
548 +
549 + Results and discussion for the individual analysis of each of the
550 + system types appear in the supporting information, while the
551 + cumulative results over all the investigated systems appears below in
552 + section \ref{sec:EnergyResults}.
553 +
554 + \subsection{Molecular Dynamics and the Force and Torque Vectors}\label{sec:MDMethods}
555 + We evaluated the pairwise methods (outlined in section
556 + \ref{sec:ESMethods}) for use in MD simulations by
557 + comparing the force and torque vectors with those obtained using the
558 + reference Ewald summation (SPME).  Both the magnitude and the
559 + direction of these vectors on each of the bodies in the system were
560 + analyzed.  For the magnitude of these vectors, linear least squares
561 + regression analyses were performed as described previously for
562 + comparing $\Delta E$ values.  Instead of a single energy difference
563 + between two system configurations, we compared the magnitudes of the
564 + forces (and torques) on each molecule in each configuration.  For a
565 + system of 1000 water molecules and 40 ions, there are 1040 force
566 + vectors and 1000 torque vectors.  With 500 configurations, this
567 + results in 520,000 force and 500,000 torque vector comparisons.
568 + Additionally, data from seven different system types was aggregated
569 + before the comparison was made.
570 +
571 + The {\it directionality} of the force and torque vectors was
572 + investigated through measurement of the angle ($\theta$) formed
573 + between those computed from the particular method and those from SPME,
574 + \begin{equation}
575 + \theta_f = \cos^{-1} \left(\hat{F}_\textrm{SPME} \cdot \hat{F}_\textrm{M}\right),
576 + \end{equation}
577 + where $\hat{f}_\textrm{M}$ is the unit vector pointing along the force
578 + vector computed using method M.  Each of these $\theta$ values was
579 + accumulated in a distribution function and weighted by the area on the
580 + unit sphere.  Non-linear Gaussian fits were used to measure the width
581 + of the resulting distributions.
582 + %
583 + %\begin{figure}
584 + %\centering
585 + %\includegraphics[width = \linewidth]{./gaussFit.pdf}
586 + %\caption{Sample fit of the angular distribution of the force vectors
587 + %accumulated using all of the studied systems.  Gaussian fits were used
588 + %to obtain values for the variance in force and torque vectors.}
589 + %\label{fig:gaussian}
590 + %\end{figure}
591 + %
592 + %Figure \ref{fig:gaussian} shows an example distribution with applied
593 + %non-linear fits.  The solid line is a Gaussian profile, while the
594 + %dotted line is a Voigt profile, a convolution of a Gaussian and a
595 + %Lorentzian.  
596 + %Since this distribution is a measure of angular error between two
597 + %different electrostatic summation methods, there is no {\it a priori}
598 + %reason for the profile to adhere to any specific shape.
599 + %Gaussian fits was used to compare all the tested methods.  
600 + The variance ($\sigma^2$) was extracted from each of these fits and
601 + was used to compare distribution widths.  Values of $\sigma^2$ near
602 + zero indicate vector directions indistinguishable from those
603 + calculated when using the reference method (SPME).
604  
605 + \subsection{Short-time Dynamics}
606 +
607 + The effects of the alternative electrostatic summation methods on the
608 + short-time dynamics of charged systems were evaluated by considering a
609 + NaCl crystal at a temperature of 1000 K.  A subset of the best
610 + performing pairwise methods was used in this comparison.  The NaCl
611 + crystal was chosen to avoid possible complications from the treatment
612 + of orientational motion in molecular systems.  All systems were
613 + started with the same initial positions and velocities.  Simulations
614 + were performed under the microcanonical ensemble, and velocity
615 + autocorrelation functions (Eq. \ref{eq:vCorr}) were computed for each
616 + of the trajectories,
617 + \begin{equation}
618 + C_v(t) = \frac{\langle v_i(0)\cdot v_i(t)\rangle}{\langle v_i(0)\cdot v_i(0)\rangle}.
619 + \label{eq:vCorr}
620 + \end{equation}
621 + Velocity autocorrelation functions require detailed short time data,
622 + thus velocity information was saved every 2 fs over 10 ps
623 + trajectories. Because the NaCl crystal is composed of two different
624 + atom types, the average of the two resulting velocity autocorrelation
625 + functions was used for comparisons.
626 +
627 + \subsection{Long-Time and Collective Motion}\label{sec:LongTimeMethods}
628 +
629 + The effects of the same subset of alternative electrostatic methods on
630 + the {\it long-time} dynamics of charged systems were evaluated using
631 + the same model system (NaCl crystals at 1000K).  The power spectrum
632 + ($I(\omega)$) was obtained via Fourier transform of the velocity
633 + autocorrelation function, \begin{equation} I(\omega) =
634 + \frac{1}{2\pi}\int^{\infty}_{-\infty}C_v(t)e^{-i\omega t}dt,
635 + \label{eq:powerSpec}
636 + \end{equation}
637 + where the frequency, $\omega=0,\ 1,\ ...,\ N-1$. Again, because the
638 + NaCl crystal is composed of two different atom types, the average of
639 + the two resulting power spectra was used for comparisons. Simulations
640 + were performed under the microcanonical ensemble, and velocity
641 + information was saved every 5 fs over 100 ps trajectories.
642 +
643 + \subsection{Representative Simulations}\label{sec:RepSims}
644 + A variety of representative simulations were analyzed to determine the
645 + relative effectiveness of the pairwise summation techniques in
646 + reproducing the energetics and dynamics exhibited by SPME.  We wanted
647 + to span the space of modern simulations (i.e. from liquids of neutral
648 + molecules to ionic crystals), so the systems studied were:
649 + \begin{enumerate}
650 + \item liquid water (SPC/E),\cite{Berendsen87}
651 + \item crystalline water (Ice I$_\textrm{c}$ crystals of SPC/E),
652 + \item NaCl crystals,
653 + \item NaCl melts,
654 + \item a low ionic strength solution of NaCl in water (0.11 M),
655 + \item a high ionic strength solution of NaCl in water (1.1 M), and
656 + \item a 6 \AA\  radius sphere of Argon in water.
657 + \end{enumerate}
658 + By utilizing the pairwise techniques (outlined in section
659 + \ref{sec:ESMethods}) in systems composed entirely of neutral groups,
660 + charged particles, and mixtures of the two, we hope to discern under
661 + which conditions it will be possible to use one of the alternative
662 + summation methodologies instead of the Ewald sum.
663 +
664 + For the solid and liquid water configurations, configurations were
665 + taken at regular intervals from high temperature trajectories of 1000
666 + SPC/E water molecules.  Each configuration was equilibrated
667 + independently at a lower temperature (300~K for the liquid, 200~K for
668 + the crystal).  The solid and liquid NaCl systems consisted of 500
669 + $\textrm{Na}^{+}$ and 500 $\textrm{Cl}^{-}$ ions.  Configurations for
670 + these systems were selected and equilibrated in the same manner as the
671 + water systems.  The equilibrated temperatures were 1000~K for the NaCl
672 + crystal and 7000~K for the liquid. The ionic solutions were made by
673 + solvating 4 (or 40) ions in a periodic box containing 1000 SPC/E water
674 + molecules.  Ion and water positions were then randomly swapped, and
675 + the resulting configurations were again equilibrated individually.
676 + Finally, for the Argon / Water ``charge void'' systems, the identities
677 + of all the SPC/E waters within 6 \AA\ of the center of the
678 + equilibrated water configurations were converted to argon.
679 + %(Fig. \ref{fig:argonSlice}).
680 +
681 + These procedures guaranteed us a set of representative configurations
682 + from chemically-relevant systems sampled from an appropriate
683 + ensemble. Force field parameters for the ions and Argon were taken
684 + from the force field utilized by {\sc oopse}.\cite{Meineke05}
685 +
686 + %\begin{figure}
687 + %\centering
688 + %\includegraphics[width = \linewidth]{./slice.pdf}
689 + %\caption{A slice from the center of a water box used in a charge void
690 + %simulation.  The darkened region represents the boundary sphere within
691 + %which the water molecules were converted to argon atoms.}
692 + %\label{fig:argonSlice}
693 + %\end{figure}
694 +
695 + \subsection{Comparison of Summation Methods}\label{sec:ESMethods}
696 + We compared the following alternative summation methods with results
697 + from the reference method (SPME):
698 + \begin{itemize}
699 + \item {\sc sp} with damping parameters ($\alpha$) of 0.0, 0.1, 0.2,
700 + and 0.3 \AA$^{-1}$,
701 + \item {\sc sf} with damping parameters ($\alpha$) of 0.0, 0.1, 0.2,
702 + and 0.3 \AA$^{-1}$,
703 + \item reaction field with an infinite dielectric constant, and
704 + \item an unmodified cutoff.
705 + \end{itemize}
706 + Group-based cutoffs with a fifth-order polynomial switching function
707 + were utilized for the reaction field simulations.  Additionally, we
708 + investigated the use of these cutoffs with the SP, SF, and pure
709 + cutoff.  The SPME electrostatics were performed using the TINKER
710 + implementation of SPME,\cite{Ponder87} while all other method
711 + calculations were performed using the OOPSE molecular mechanics
712 + package.\cite{Meineke05} All other portions of the energy calculation
713 + (i.e. Lennard-Jones interactions) were handled in exactly the same
714 + manner across all systems and configurations.
715 +
716 + The althernative methods were also evaluated with three different
717 + cutoff radii (9, 12, and 15 \AA).  As noted previously, the
718 + convergence parameter ($\alpha$) plays a role in the balance of the
719 + real-space and reciprocal-space portions of the Ewald calculation.
720 + Typical molecular mechanics packages set this to a value dependent on
721 + the cutoff radius and a tolerance (typically less than $1 \times
722 + 10^{-4}$ kcal/mol).  Smaller tolerances are typically associated with
723 + increased accuracy at the expense of increased time spent calculating
724 + the reciprocal-space portion of the
725 + summation.\cite{Perram88,Essmann95} The default TINKER tolerance of $1
726 + \times 10^{-8}$ kcal/mol was used in all SPME calculations, resulting
727 + in Ewald Coefficients of 0.4200, 0.3119, and 0.2476 \AA$^{-1}$ for
728 + cutoff radii of 9, 12, and 15 \AA\ respectively.
729 +
730   \section{Results and Discussion}
731 +
732 + \subsection{Configuration Energy Differences}\label{sec:EnergyResults}
733 + In order to evaluate the performance of the pairwise electrostatic
734 + summation methods for Monte Carlo simulations, the energy differences
735 + between configurations were compared to the values obtained when using
736 + SPME.  The results for the subsequent regression analysis are shown in
737 + figure \ref{fig:delE}.
738 +
739 + \begin{figure}
740 + \centering
741 + \includegraphics[width=5.5in]{./delEplot.pdf}
742 + \caption{Statistical analysis of the quality of configurational energy
743 + differences for a given electrostatic method compared with the
744 + reference Ewald sum.  Results with a value equal to 1 (dashed line)
745 + indicate $\Delta E$ values indistinguishable from those obtained using
746 + SPME.  Different values of the cutoff radius are indicated with
747 + different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ =
748 + inverted triangles).}
749 + \label{fig:delE}
750 + \end{figure}
751 +
752 + The most striking feature of this plot is how well the Shifted Force
753 + ({\sc sf}) and Shifted Potential ({\sc sp}) methods capture the energy
754 + differences.  For the undamped {\sc sf} method, and the
755 + moderately-damped {\sc sp} methods, the results are nearly
756 + indistinguishable from the Ewald results.  The other common methods do
757 + significantly less well.  
758 +
759 + The unmodified cutoff method is essentially unusable.  This is not
760 + surprising since hard cutoffs give large energy fluctuations as atoms
761 + or molecules move in and out of the cutoff
762 + radius.\cite{Rahman71,Adams79} These fluctuations can be alleviated to
763 + some degree by using group based cutoffs with a switching
764 + function.\cite{Adams79,Steinbach94,Leach01} However, we do not see
765 + significant improvement using the group-switched cutoff because the
766 + salt and salt solution systems contain non-neutral groups.  Interested
767 + readers can consult the accompanying supporting information for a
768 + comparison where all groups are neutral.
769 +
770 + For the {\sc sp} method, inclusion of potential damping improves the
771 + agreement with Ewald, and using an $\alpha$ of 0.2 \AA $^{-1}$ shows
772 + an excellent correlation and quality of fit with the SPME results,
773 + particularly with a cutoff radius greater than 12
774 + \AA .  Use of a larger damping parameter is more helpful for the
775 + shortest cutoff shown, but it has a detrimental effect on simulations
776 + with larger cutoffs.  
777 +
778 + In the {\sc sf} sets, increasing damping results in progressively
779 + worse correlation with Ewald.  Overall, the undamped case is the best
780 + performing set, as the correlation and quality of fits are
781 + consistently superior regardless of the cutoff distance.  The undamped
782 + case is also less computationally demanding (because no evaluation of
783 + the complementary error function is required).
784 +
785 + The reaction field results illustrates some of that method's
786 + limitations, primarily that it was developed for use in homogenous
787 + systems; although it does provide results that are an improvement over
788 + those from an unmodified cutoff.
789 +
790 + \subsection{Magnitudes of the Force and Torque Vectors}
791 +
792 + Evaluation of pairwise methods for use in Molecular Dynamics
793 + simulations requires consideration of effects on the forces and
794 + torques.  Investigation of the force and torque vector magnitudes
795 + provides a measure of the strength of these values relative to SPME.
796 + Figures \ref{fig:frcMag} and \ref{fig:trqMag} respectively show the
797 + force and torque vector magnitude regression results for the
798 + accumulated analysis over all the system types.
799 +
800 + \begin{figure}
801 + \centering
802 + \includegraphics[width=5.5in]{./frcMagplot.pdf}
803 + \caption{Statistical analysis of the quality of the force vector
804 + magnitudes for a given electrostatic method compared with the
805 + reference Ewald sum.  Results with a value equal to 1 (dashed line)
806 + indicate force magnitude values indistinguishable from those obtained
807 + using SPME.  Different values of the cutoff radius are indicated with
808 + different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ =
809 + inverted triangles).}
810 + \label{fig:frcMag}
811 + \end{figure}
812 +
813 + Figure \ref{fig:frcMag}, for the most part, parallels the results seen
814 + in the previous $\Delta E$ section.  The unmodified cutoff results are
815 + poor, but using group based cutoffs and a switching function provides
816 + a improvement much more significant than what was seen with $\Delta
817 + E$.  Looking at the {\sc sp} sets, the slope and $R^2$
818 + improve with the use of damping to an optimal result of 0.2 \AA
819 + $^{-1}$ for the 12 and 15 \AA\ cutoffs.  Further increases in damping,
820 + while beneficial for simulations with a cutoff radius of 9 \AA\ , is
821 + detrimental to simulations with larger cutoff radii.  The undamped
822 + {\sc sf} method gives forces in line with those obtained using
823 + SPME, and use of a damping function results in minor improvement.  The
824 + reaction field results are surprisingly good, considering the poor
825 + quality of the fits for the $\Delta E$ results.  There is still a
826 + considerable degree of scatter in the data, but it correlates well in
827 + general.  To be fair, we again note that the reaction field
828 + calculations do not encompass NaCl crystal and melt systems, so these
829 + results are partly biased towards conditions in which the method
830 + performs more favorably.
831 +
832 + \begin{figure}
833 + \centering
834 + \includegraphics[width=5.5in]{./trqMagplot.pdf}
835 + \caption{Statistical analysis of the quality of the torque vector
836 + magnitudes for a given electrostatic method compared with the
837 + reference Ewald sum.  Results with a value equal to 1 (dashed line)
838 + indicate torque magnitude values indistinguishable from those obtained
839 + using SPME.  Different values of the cutoff radius are indicated with
840 + different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ =
841 + inverted triangles).}
842 + \label{fig:trqMag}
843 + \end{figure}
844 +
845 + To evaluate the torque vector magnitudes, the data set from which
846 + values are drawn is limited to rigid molecules in the systems
847 + (i.e. water molecules).  In spite of this smaller sampling pool, the
848 + torque vector magnitude results in figure \ref{fig:trqMag} are still
849 + similar to those seen for the forces; however, they more clearly show
850 + the improved behavior that comes with increasing the cutoff radius.
851 + Moderate damping is beneficial to the {\sc sp} and helpful
852 + yet possibly unnecessary with the {\sc sf} method, and they also
853 + show that over-damping adversely effects all cutoff radii rather than
854 + showing an improvement for systems with short cutoffs.  The reaction
855 + field method performs well when calculating the torques, better than
856 + the Shifted Force method over this limited data set.
857 +
858 + \subsection{Directionality of the Force and Torque Vectors}
859 +
860 + Having force and torque vectors with magnitudes that are well
861 + correlated to SPME is good, but if they are not pointing in the proper
862 + direction the results will be incorrect.  These vector directions were
863 + investigated through measurement of the angle formed between them and
864 + those from SPME.  The results (Fig. \ref{fig:frcTrqAng}) are compared
865 + through the variance ($\sigma^2$) of the Gaussian fits of the angle
866 + error distributions of the combined set over all system types.
867  
868 + \begin{figure}
869 + \centering
870 + \includegraphics[width=5.5in]{./frcTrqAngplot.pdf}
871 + \caption{Statistical analysis of the quality of the Gaussian fit of
872 + the force and torque vector angular distributions for a given
873 + electrostatic method compared with the reference Ewald sum.  Results
874 + with a variance ($\sigma^2$) equal to zero (dashed line) indicate
875 + force and torque directions indistinguishable from those obtained
876 + using SPME.  Different values of the cutoff radius are indicated with
877 + different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ =
878 + inverted triangles).}
879 + \label{fig:frcTrqAng}
880 + \end{figure}
881 +
882 + Both the force and torque $\sigma^2$ results from the analysis of the
883 + total accumulated system data are tabulated in figure
884 + \ref{fig:frcTrqAng}.  All of the sets, aside from the over-damped case
885 + show the improvement afforded by choosing a longer simulation cutoff.
886 + Increasing the cutoff from 9 to 12 \AA\ typically results in a halving
887 + of the distribution widths, with a similar improvement going from 12
888 + to 15 \AA .  The undamped {\sc sf}, Group Based Cutoff, and
889 + Reaction Field methods all do equivalently well at capturing the
890 + direction of both the force and torque vectors.  Using damping
891 + improves the angular behavior significantly for the {\sc sp}
892 + and moderately for the {\sc sf} methods.  Increasing the damping
893 + too far is destructive for both methods, particularly to the torque
894 + vectors.  Again it is important to recognize that the force vectors
895 + cover all particles in the systems, while torque vectors are only
896 + available for neutral molecular groups.  Damping appears to have a
897 + more beneficial effect on non-neutral bodies, and this observation is
898 + investigated further in the accompanying supporting information.
899 +
900 + \begin{table}[htbp]
901 +   \centering
902 +   \caption{Variance ($\sigma^2$) of the force (top set) and torque
903 + (bottom set) vector angle difference distributions for the Shifted Potential and Shifted Force methods.  Calculations were performed both with (Y) and without (N) group based cutoffs and a switching function.  The $\alpha$ values have units of \AA$^{-1}$ and the variance values have units of degrees$^2$.}      
904 +   \begin{tabular}{@{} ccrrrrrrrr @{}}
905 +      \\
906 +      \toprule
907 +      & & \multicolumn{4}{c}{Shifted Potential} & \multicolumn{4}{c}{Shifted Force} \\
908 +      \cmidrule(lr){3-6}
909 +      \cmidrule(l){7-10}
910 +            $R_\textrm{c}$ & Groups & $\alpha = 0$ & $\alpha = 0.1$ & $\alpha = 0.2$ & $\alpha = 0.3$ & $\alpha = 0$ & $\alpha = 0.1$ & $\alpha = 0.2$ & $\alpha = 0.3$\\
911 +      \midrule
912 +    
913 + 9 \AA   & N & 29.545 & 12.003 & 5.489 & 0.610 & 2.323 & 2.321 & 0.429 & 0.603 \\
914 +        & \textbf{Y} & \textbf{2.486} & \textbf{2.160} & \textbf{0.667} & \textbf{0.608} & \textbf{1.768} & \textbf{1.766} & \textbf{0.676} & \textbf{0.609} \\
915 + 12 \AA  & N & 19.381 & 3.097 & 0.190 & 0.608 & 0.920 & 0.736 & 0.133 & 0.612 \\
916 +        & \textbf{Y} & \textbf{0.515} & \textbf{0.288} & \textbf{0.127} & \textbf{0.586} & \textbf{0.308} & \textbf{0.249} & \textbf{0.127} & \textbf{0.586} \\
917 + 15 \AA  & N & 12.700 & 1.196 & 0.123 & 0.601 & 0.339 & 0.160 & 0.123 & 0.601 \\
918 +        & \textbf{Y} & \textbf{0.228} & \textbf{0.099} & \textbf{0.121} & \textbf{0.598} & \textbf{0.144} & \textbf{0.090} & \textbf{0.121} & \textbf{0.598} \\      
919 +
920 +      \midrule
921 +      
922 + 9 \AA   & N & 262.716 & 116.585 & 5.234 & 5.103 & 2.392 & 2.350 & 1.770 & 5.122 \\
923 +        & \textbf{Y} & \textbf{2.115} & \textbf{1.914} & \textbf{1.878} & \textbf{5.142} & \textbf{2.076} & \textbf{2.039} & \textbf{1.972} & \textbf{5.146} \\
924 + 12 \AA  & N & 129.576 & 25.560 & 1.369 & 5.080 & 0.913 & 0.790 & 1.362 & 5.124 \\
925 +        & \textbf{Y} & \textbf{0.810} & \textbf{0.685} & \textbf{1.352} & \textbf{5.082} & \textbf{0.765} & \textbf{0.714} & \textbf{1.360} & \textbf{5.082} \\
926 + 15 \AA  & N & 87.275 & 4.473 & 1.271 & 5.000 & 0.372 & 0.312 & 1.271 & 5.000 \\
927 +        & \textbf{Y} & \textbf{0.282} & \textbf{0.294} & \textbf{1.272} & \textbf{4.999} & \textbf{0.324} & \textbf{0.318} & \textbf{1.272} & \textbf{4.999} \\
928 +
929 +      \bottomrule
930 +   \end{tabular}
931 +   \label{tab:groupAngle}
932 + \end{table}
933 +
934 + Although not discussed previously, group based cutoffs can be applied
935 + to both the {\sc sp} and {\sc sf} methods.  Use off a
936 + switching function corrects for the discontinuities that arise when
937 + atoms of a group exit the cutoff before the group's center of mass.
938 + Though there are no significant benefit or drawbacks observed in
939 + $\Delta E$ and vector magnitude results when doing this, there is a
940 + measurable improvement in the vector angle results.  Table
941 + \ref{tab:groupAngle} shows the angular variance values obtained using
942 + group based cutoffs and a switching function alongside the standard
943 + results seen in figure \ref{fig:frcTrqAng} for comparison purposes.
944 + The {\sc sp} shows much narrower angular distributions for
945 + both the force and torque vectors when using an $\alpha$ of 0.2
946 + \AA$^{-1}$ or less, while {\sc sf} shows improvements in the
947 + undamped and lightly damped cases.  Thus, by calculating the
948 + electrostatic interactions in terms of molecular pairs rather than
949 + atomic pairs, the direction of the force and torque vectors are
950 + determined more accurately.
951 +
952 + One additional trend to recognize in table \ref{tab:groupAngle} is
953 + that the $\sigma^2$ values for both {\sc sp} and
954 + {\sc sf} converge as $\alpha$ increases, something that is easier
955 + to see when using group based cutoffs.  Looking back on figures
956 + \ref{fig:delE}, \ref{fig:frcMag}, and \ref{fig:trqMag}, show this
957 + behavior clearly at large $\alpha$ and cutoff values.  The reason for
958 + this is that the complimentary error function inserted into the
959 + potential weakens the electrostatic interaction as $\alpha$ increases.
960 + Thus, at larger values of $\alpha$, both the summation method types
961 + progress toward non-interacting functions, so care is required in
962 + choosing large damping functions lest one generate an undesirable loss
963 + in the pair interaction.  Kast \textit{et al.}  developed a method for
964 + choosing appropriate $\alpha$ values for these types of electrostatic
965 + summation methods by fitting to $g(r)$ data, and their methods
966 + indicate optimal values of 0.34, 0.25, and 0.16 \AA$^{-1}$ for cutoff
967 + values of 9, 12, and 15 \AA\ respectively.\cite{Kast03} These appear
968 + to be reasonable choices to obtain proper MC behavior
969 + (Fig. \ref{fig:delE}); however, based on these findings, choices this
970 + high would introduce error in the molecular torques, particularly for
971 + the shorter cutoffs.  Based on the above findings, empirical damping
972 + up to 0.2 \AA$^{-1}$ proves to be beneficial, but damping is arguably
973 + unnecessary when using the {\sc sf} method.
974 +
975 + \subsection{Short-Time Dynamics: Velocity Autocorrelation Functions of NaCl Crystals}
976 +
977 + In the previous studies using a {\sc sf} variant of the damped
978 + Wolf coulomb potential, the structure and dynamics of water were
979 + investigated rather extensively.\cite{Zahn02,Kast03} Their results
980 + indicated that the damped {\sc sf} method results in properties
981 + very similar to those obtained when using the Ewald summation.
982 + Considering the statistical results shown above, the good performance
983 + of this method is not that surprising.  Rather than consider the same
984 + systems and simply recapitulate their results, we decided to look at
985 + the solid state dynamical behavior obtained using the best performing
986 + summation methods from the above results.
987 +
988 + \begin{figure}
989 + \centering
990 + \includegraphics[width = \linewidth]{./vCorrPlot.pdf}
991 + \caption{Velocity auto-correlation functions of NaCl crystals at
992 + 1000 K while using SPME, {\sc sf} ($\alpha$ = 0.0, 0.1, \& 0.2), and
993 + {\sc sp} ($\alpha$ = 0.2). The inset is a magnification of the first
994 + trough. The times to first collision are nearly identical, but the
995 + differences can be seen in the peaks and troughs, where the undamped
996 + to weakly damped methods are stiffer than the moderately damped and
997 + SPME methods.}
998 + \label{fig:vCorrPlot}
999 + \end{figure}
1000 +
1001 + The short-time decays through the first collision are nearly identical
1002 + in figure \ref{fig:vCorrPlot}, but the peaks and troughs of the
1003 + functions show how the methods differ.  The undamped {\sc sf} method
1004 + has deeper troughs (see inset in Fig. \ref{fig:vCorrPlot}) and higher
1005 + peaks than any of the other methods.  As the damping function is
1006 + increased, these peaks are smoothed out, and approach the SPME
1007 + curve. The damping acts as a distance dependent Gaussian screening of
1008 + the point charges for the pairwise summation methods; thus, the
1009 + collisions are more elastic in the undamped {\sc sf} potential, and the
1010 + stiffness of the potential is diminished as the electrostatic
1011 + interactions are softened by the damping function.  With $\alpha$
1012 + values of 0.2 \AA$^{-1}$, the {\sc sf} and {\sc sp} functions are
1013 + nearly identical and track the SPME features quite well.  This is not
1014 + too surprising in that the differences between the {\sc sf} and {\sc
1015 + sp} potentials are mitigated with increased damping.  However, this
1016 + appears to indicate that once damping is utilized, the form of the
1017 + potential seems to play a lesser role in the crystal dynamics.
1018 +
1019 + \subsection{Collective Motion: Power Spectra of NaCl Crystals}
1020 +
1021 + The short time dynamics were extended to evaluate how the differences
1022 + between the methods affect the collective long-time motion.  The same
1023 + electrostatic summation methods were used as in the short time
1024 + velocity autocorrelation function evaluation, but the trajectories
1025 + were sampled over a much longer time. The power spectra of the
1026 + resulting velocity autocorrelation functions were calculated and are
1027 + displayed in figure \ref{fig:methodPS}.
1028 +
1029 + \begin{figure}
1030 + \centering
1031 + \includegraphics[width = \linewidth]{./spectraSquare.pdf}
1032 + \caption{Power spectra obtained from the velocity auto-correlation
1033 + functions of NaCl crystals at 1000 K while using SPME, {\sc sf}
1034 + ($\alpha$ = 0, 0.1, \& 0.2), and {\sc sp} ($\alpha$ = 0.2).
1035 + Apodization of the correlation functions via a cubic switching
1036 + function between 40 and 50 ps was used to clear up the spectral noise
1037 + resulting from data truncation, and had no noticeable effect on peak
1038 + location or magnitude.  The inset shows the frequency region below 100
1039 + cm$^{-1}$ to highlight where the spectra begin to differ.}
1040 + \label{fig:methodPS}
1041 + \end{figure}
1042 +
1043 + While high frequency peaks of the spectra in this figure overlap,
1044 + showing the same general features, the low frequency region shows how
1045 + the summation methods differ.  Considering the low-frequency inset
1046 + (expanded in the upper frame of figure \ref{fig:dampInc}), at
1047 + frequencies below 100 cm$^{-1}$, the correlated motions are
1048 + blue-shifted when using undamped or weakly damped {\sc sf}.  When
1049 + using moderate damping ($\alpha = 0.2$ \AA$^{-1}$) both the {\sc sf}
1050 + and {\sc sp} methods give near identical correlated motion behavior as
1051 + the Ewald method (which has a damping value of 0.3119).  This
1052 + weakening of the electrostatic interaction with increased damping
1053 + explains why the long-ranged correlated motions are at lower
1054 + frequencies for the moderately damped methods than for undamped or
1055 + weakly damped methods.  To see this effect more clearly, we show how
1056 + damping strength alone affects a simple real-space electrostatic
1057 + potential,
1058 + \begin{equation}
1059 + V_\textrm{damped}=\sum^N_i\sum^N_{j\ne i}q_iq_j\left[\frac{\textrm{erfc}({\alpha r})}{r}\right]S(r),
1060 + \end{equation}
1061 + where $S(r)$ is a switching function that smoothly zeroes the
1062 + potential at the cutoff radius.  Figure \ref{fig:dampInc} shows how
1063 + the low frequency motions are dependent on the damping used in the
1064 + direct electrostatic sum.  As the damping increases, the peaks drop to
1065 + lower frequencies.  Incidentally, use of an $\alpha$ of 0.25
1066 + \AA$^{-1}$ on a simple electrostatic summation results in low
1067 + frequency correlated dynamics equivalent to a simulation using SPME.
1068 + When the coefficient lowers to 0.15 \AA$^{-1}$ and below, these peaks
1069 + shift to higher frequency in exponential fashion.  Though not shown,
1070 + the spectrum for the simple undamped electrostatic potential is
1071 + blue-shifted such that the lowest frequency peak resides near 325
1072 + cm$^{-1}$.  In light of these results, the undamped {\sc sf} method
1073 + producing low-lying motion peaks within 10 cm$^{-1}$ of SPME is quite
1074 + respectable and shows that the shifted force procedure accounts for
1075 + most of the effect afforded through use of the Ewald summation.
1076 + However, it appears as though moderate damping is required for
1077 + accurate reproduction of crystal dynamics.
1078 + \begin{figure}
1079 + \centering
1080 + \includegraphics[width = \linewidth]{./comboSquare.pdf}
1081 + \caption{Regions of spectra showing the low-frequency correlated
1082 + motions for NaCl crystals at 1000 K using various electrostatic
1083 + summation methods.  The upper plot is a zoomed inset from figure
1084 + \ref{fig:methodPS}.  As the damping value for the {\sc sf} potential
1085 + increases, the low-frequency peaks red-shift.  The lower plot is of
1086 + spectra when using SPME and a simple damped Coulombic sum with damping
1087 + coefficients ($\alpha$) ranging from 0.15 to 0.3 \AA$^{-1}$.  As
1088 + $\alpha$ increases, the peaks are red-shifted toward and eventually
1089 + beyond the values given by SPME.  The larger $\alpha$ values weaken
1090 + the real-space electrostatics, explaining this shift towards less
1091 + strongly correlated motions in the crystal.}
1092 + \label{fig:dampInc}
1093 + \end{figure}
1094 +
1095   \section{Conclusions}
1096  
1097 < \section{Acknowledgments}
1097 > This investigation of pairwise electrostatic summation techniques
1098 > shows that there are viable and more computationally efficient
1099 > electrostatic summation techniques than the Ewald summation, chiefly
1100 > methods derived from the damped Coulombic sum originally proposed by
1101 > Wolf \textit{et al.}\cite{Wolf99,Zahn02} In particular, the
1102 > {\sc sf} method, reformulated above as eq. (\ref{eq:DSFPot}),
1103 > shows a remarkable ability to reproduce the energetic and dynamic
1104 > characteristics exhibited by simulations employing lattice summation
1105 > techniques.  The cumulative energy difference results showed the
1106 > undamped {\sc sf} and moderately damped {\sc sp} methods
1107 > produced results nearly identical to SPME.  Similarly for the dynamic
1108 > features, the undamped or moderately damped {\sc sf} and
1109 > moderately damped {\sc sp} methods produce force and torque
1110 > vector magnitude and directions very similar to the expected values.
1111 > These results translate into long-time dynamic behavior equivalent to
1112 > that produced in simulations using SPME.
1113  
1114 < \newpage
1114 > Aside from the computational cost benefit, these techniques have
1115 > applicability in situations where the use of the Ewald sum can prove
1116 > problematic.  Primary among them is their use in interfacial systems,
1117 > where the unmodified lattice sum techniques artificially accentuate
1118 > the periodicity of the system in an undesirable manner.  There have
1119 > been alterations to the standard Ewald techniques, via corrections and
1120 > reformulations, to compensate for these systems; but the pairwise
1121 > techniques discussed here require no modifications, making them
1122 > natural tools to tackle these problems.  Additionally, this
1123 > transferability gives them benefits over other pairwise methods, like
1124 > reaction field, because estimations of physical properties (e.g. the
1125 > dielectric constant) are unnecessary.
1126  
1127 < \bibliographystyle{achemso}
1127 > We are not suggesting any flaw with the Ewald sum; in fact, it is the
1128 > standard by which these simple pairwise sums are judged.  However,
1129 > these results do suggest that in the typical simulations performed
1130 > today, the Ewald summation may no longer be required to obtain the
1131 > level of accuracy most researchers have come to expect
1132 >
1133 > \section{Acknowledgments}
1134 > \newpage
1135 >
1136 > \bibliographystyle{jcp2}
1137   \bibliography{electrostaticMethods}
1138  
1139  

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