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2   %\documentclass[aps,prb,preprint]{revtex4}
3   \documentclass[11pt]{article}
4   \usepackage{endfloat}
5 < \usepackage{amsmath}
5 > \usepackage{amsmath,bm}
6   \usepackage{amssymb}
7   \usepackage{epsf}
8   \usepackage{times}
# Line 65 | Line 65 | In molecular simulations, proper accumulation of the e
65   \section{Introduction}
66  
67   In molecular simulations, proper accumulation of the electrostatic
68 < interactions is considered one of the most essential and
69 < computationally demanding tasks.  The common molecular mechanics force
70 < fields are founded on representation of the atomic sites centered on
71 < full or partial charges shielded by Lennard-Jones type interactions.
72 < This means that nearly every pair interaction involves an
73 < charge-charge calculation.  Coupled with $r^{-1}$ decay, the monopole
74 < interactions quickly become a burden for molecular systems of all
75 < sizes.  For example, in small systems, the electrostatic pair
76 < interaction may not have decayed appreciably within the box length
77 < leading to an effect excluded from the pair interactions within a unit
78 < box.  In large systems, excessively large cutoffs need to be used to
79 < accurately incorporate their effect, and since the computational cost
80 < increases proportionally with the cutoff sphere, it quickly becomes an
81 < impractical task to perform these calculations.
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 < blah blah blah Ewald Sum Important blah blah blah
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 system sizes that could be
158 + simulated feasibly, the entire simulation box was replicated to
159 + convergence.  In more modern simulations, the systems have grown large
160 + enough that a real-space cutoff could potentially give convergent
161 + behavior.  Indeed, it has been observed that with the choice of a
162 + small $\alpha$, the reciprocal-space portion of the Ewald sum can be
163 + rapidly convergent and small relative to the real-space
164 + portion.\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
94 < calculated structure factor is used to sum out to great distance, and
95 < a surrounding dielectric term is included.}
168 > \includegraphics[width = \linewidth]{./ewaldProgression2.pdf}
169 > \caption{The change in the application of the Ewald sum with
170 > increasing computational power.  Initially, only small systems could
171 > be studied, and the Ewald sum replicated the simulation box to
172 > convergence.  Now, much larger systems of charges are investigated
173 > with fixed-distance cutoffs.}
174   \label{fig:ewaldTime}
175   \end{figure}
176  
177 + The original Ewald summation is an $\mathscr{O}(N^2)$ algorithm.  The
178 + convergence parameter $(\alpha)$ plays an important role in balancing
179 + the computational cost between the direct and reciprocal-space
180 + portions of the summation.  The choice of this value allows one to
181 + select whether the real-space or reciprocal space portion of the
182 + summation is an $\mathscr{O}(N^2)$ calculation (with the other being
183 + $\mathscr{O}(N)$).\cite{Sagui99} With the appropriate choice of
184 + $\alpha$ and thoughtful algorithm development, this cost can be
185 + reduced to $\mathscr{O}(N^{3/2})$.\cite{Perram88} The typical route
186 + taken to reduce the cost of the Ewald summation even further is to set
187 + $\alpha$ such that the real-space interactions decay rapidly, allowing
188 + for a short spherical cutoff. Then the reciprocal space summation is
189 + optimized.  These optimizations usually involve utilization of the
190 + fast Fourier transform (FFT),\cite{Hockney81} leading to the
191 + particle-particle particle-mesh (P3M) and particle mesh Ewald (PME)
192 + methods.\cite{Shimada93,Luty94,Luty95,Darden93,Essmann95} In these
193 + methods, the cost of the reciprocal-space portion of the Ewald
194 + summation is reduced from $\mathscr{O}(N^2)$ down to $\mathscr{O}(N
195 + \log N)$.
196 +
197 + These developments and optimizations have made the use of the Ewald
198 + summation routine in simulations with periodic boundary
199 + conditions. However, in certain systems, such as vapor-liquid
200 + interfaces and membranes, the intrinsic three-dimensional periodicity
201 + can prove problematic.  The Ewald sum has been reformulated to handle
202 + 2D systems,\cite{Parry75,Parry76,Heyes77,deLeeuw79,Rhee89}, but the
203 + new methods are computationally expensive.\cite{Spohr97,Yeh99}
204 + Inclusion of a correction term in the Ewald summation is a possible
205 + direction for handling 2D systems while still enabling the use of the
206 + modern optimizations.\cite{Yeh99}
207 +
208 + Several studies have recognized that the inherent periodicity in the
209 + Ewald sum can also have an effect on three-dimensional
210 + systems.\cite{Roberts94,Roberts95,Luty96,Hunenberger99a,Hunenberger99b,Weber00}
211 + Solvated proteins are essentially kept at high concentration due to
212 + the periodicity of the electrostatic summation method.  In these
213 + systems, the more compact folded states of a protein can be
214 + artificially stabilized by the periodic replicas introduced by the
215 + Ewald summation.\cite{Weber00} Thus, care must be taken when
216 + considering the use of the Ewald summation where the assumed
217 + periodicity would introduce spurious effects in the system dynamics.
218 +
219   \subsection{The Wolf and Zahn Methods}
220   In a recent paper by Wolf \textit{et al.}, a procedure was outlined
221 < for an accurate accumulation of electrostatic interactions in an
222 < efficient pairwise fashion.\cite{Wolf99} Wolf \textit{et al.} observed
223 < that the electrostatic interaction is effectively short-ranged in
224 < condensed phase systems and that neutralization of the charge
225 < contained within the cutoff radius is crucial for potential
221 > for the accurate accumulation of electrostatic interactions in an
222 > efficient pairwise fashion.  This procedure lacks the inherent
223 > periodicity of the Ewald summation.\cite{Wolf99} Wolf \textit{et al.}
224 > observed that the electrostatic interaction is effectively
225 > short-ranged in condensed phase systems and that neutralization of the
226 > charge contained within the cutoff radius is crucial for potential
227   stability. They devised a pairwise summation method that ensures
228 < charge neutrality and gives results similar to those obtained with
229 < the Ewald summation.  The resulting shifted Coulomb potential
228 > charge neutrality and gives results similar to those obtained with the
229 > Ewald summation.  The resulting shifted Coulomb potential
230   (Eq. \ref{eq:WolfPot}) includes image-charges subtracted out through
231   placement on the cutoff sphere and a distance-dependent damping
232   function (identical to that seen in the real-space portion of the
233   Ewald sum) to aid convergence
234   \begin{equation}
235 < V^{\textrm{Wolf}}(r_{ij})= \frac{q_iq_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\}.
235 > 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\}.
236   \label{eq:WolfPot}
237   \end{equation}
238   Eq. (\ref{eq:WolfPot}) is essentially the common form of a shifted
239   potential.  However, neutralizing the charge contained within each
240   cutoff sphere requires the placement of a self-image charge on the
241   surface of the cutoff sphere.  This additional self-term in the total
242 < potential enables Wolf {\it et al.}  to obtain excellent estimates of
242 > potential enabled Wolf {\it et al.}  to obtain excellent estimates of
243   Madelung energies for many crystals.
244  
245   In order to use their charge-neutralized potential in molecular
# Line 126 | Line 247 | procedure gives an expression for the forces,
247   derivative of this potential prior to evaluation of the limit.  This
248   procedure gives an expression for the forces,
249   \begin{equation}
250 < F^{\textrm{Wolf}}(r_{ij}) = q_i q_j\left\{-\left[\frac{\textrm{erfc}(\alpha r_{ij})}{r^2_{ij}}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp{(-\alpha^2r_{ij}^2)}}{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\},
250 > 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\},
251   \label{eq:WolfForces}
252   \end{equation}
253   that incorporates both image charges and damping of the electrostatic
# Line 134 | Line 255 | force expressions for use in simulations involving wat
255  
256   More recently, Zahn \textit{et al.} investigated these potential and
257   force expressions for use in simulations involving water.\cite{Zahn02}
258 < In their work, they pointed out that the method that the forces and
259 < derivative of the potential are not commensurate.  Attempts to use
260 < both Eqs. (\ref{eq:WolfPot}) and (\ref{eq:WolfForces}) together will
261 < lead to poor energy conservation.  They correctly observed that taking
262 < the limit shown in equation (\ref{eq:WolfPot}) {\it after} calculating
263 < the derivatives is mathematically invalid.
258 > In their work, they pointed out that the forces and derivative of
259 > the potential are not commensurate.  Attempts to use both
260 > eqs. (\ref{eq:WolfPot}) and (\ref{eq:WolfForces}) together will lead
261 > to poor energy conservation.  They correctly observed that taking the
262 > limit shown in equation (\ref{eq:WolfPot}) {\it after} calculating the
263 > derivatives gives forces for a different potential energy function
264 > than the one shown in eq. (\ref{eq:WolfPot}).
265  
266 < Zahn \textit{et al.} proposed a modified form of this ``Wolf summation
267 < method'' as a way to use this technique in Molecular Dynamics
268 < simulations.  Taking the integral of the forces shown in equation
147 < \ref{eq:WolfForces}, they proposed a new damped Coulomb
148 < potential,
266 > Zahn \textit{et al.} introduced a modified form of this summation
267 > method as a way to use the technique in Molecular Dynamics
268 > simulations.  They proposed a new damped Coulomb potential,
269   \begin{equation}
270 < 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\}.
270 > 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\},
271   \label{eq:ZahnPot}
272   \end{equation}
273 < They showed that this potential does fairly well at capturing the
273 > and showed that this potential does fairly well at capturing the
274   structural and dynamic properties of water compared the same
275   properties obtained using the Ewald sum.
276  
# Line 158 | Line 278 | al.} are constructed using two different (and separabl
278  
279   The potentials proposed by Wolf \textit{et al.} and Zahn \textit{et
280   al.} are constructed using two different (and separable) computational
281 < tricks: \begin{itemize}
281 > tricks: \begin{enumerate}
282   \item shifting through the use of image charges, and
283   \item damping the electrostatic interaction.
284 < \end{itemize}  Wolf \textit{et al.} treated the
284 > \end{enumerate}  Wolf \textit{et al.} treated the
285   development of their summation method as a progressive application of
286   these techniques,\cite{Wolf99} while Zahn \textit{et al.} founded
287   their damped Coulomb modification (Eq. (\ref{eq:ZahnPot})) on the
# Line 181 | Line 301 | shifted potential,
301   \textit{et al.}  and Zahn \textit{et al.} by considering the standard
302   shifted potential,
303   \begin{equation}
304 < v^\textrm{SP}(r) =      \begin{cases}
304 > V_\textrm{SP}(r) =      \begin{cases}
305   v(r)-v_\textrm{c} &\quad r\leqslant R_\textrm{c} \\ 0 &\quad r >
306   R_\textrm{c}  
307   \end{cases},
# Line 189 | Line 309 | and shifted force,
309   \end{equation}
310   and shifted force,
311   \begin{equation}
312 < v^\textrm{SF}(r) =      \begin{cases}
313 < v(r)-v_\textrm{c}-\left(\frac{\textrm{d}v(r)}{\textrm{d}r}\right)_{r=R_\textrm{c}}(r-R_\textrm{c})
312 > V_\textrm{SF}(r) =      \begin{cases}
313 > v(r)-v_\textrm{c}-\left(\frac{d v(r)}{d r}\right)_{r=R_\textrm{c}}(r-R_\textrm{c})
314   &\quad r\leqslant R_\textrm{c} \\ 0 &\quad r > R_\textrm{c}
315                                                  \end{cases},
316   \label{eq:shiftingForm}
# Line 202 | Line 322 | potential is smooth at the cutoff radius
322   potential is smooth at the cutoff radius
323   ($R_\textrm{c}$).\cite{Allen87}
324  
325 <
326 <
207 <
208 < If the derivative term is taken to be zero, we are left with the shifted Coulomb potential devised by Wolf \textit{et al.},\cite{Wolf99}
325 > The forces associated with the shifted potential are simply the forces
326 > of the unshifted potential itself (when inside the cutoff sphere),
327   \begin{equation}
328 < V^\textrm{SP}(r_{ij}) = q_iq_j\left(\frac{1}{r_{ij}}-\frac{1}{R_\textrm{c}}\right) \quad r_{ij}\leqslant R_\textrm{c}.                          \label{eq:WolfSP}
328 > F_{\textrm{SP}} = -\left( \frac{d v(r)}{dr} \right),
329   \end{equation}
330 < The forces associated with this potential are obtained by taking the derivative, resulting in the following,
330 > and are zero outside.  Inside the cutoff sphere, the forces associated
331 > with the shifted force form can be written,
332   \begin{equation}
333 < F^\textrm{SP}(r_{ij}) = q_iq_j\left(-\frac{1}{r_{ij}^2}\right) \quad r_{ij}\leqslant R_\textrm{c}.
334 < \label{eq:FWolfSP}
333 > F_{\textrm{SF}} = -\left( \frac{d v(r)}{dr} \right) + \left(\frac{d
334 > v(r)}{dr} \right)_{r=R_\textrm{c}}.
335   \end{equation}
336 < These forces are identical to the forces of the standard electrostatic interaction, and this was addressed by Wolf \textit{et al.} as undesirable.  They pointed out that the effect of the image charges is neglected in the forces when they would expect there to be some pressure exerted due to their presence.\cite{Wolf99}  As a consequence the forces, though mathematically valid, may not be physically correct due to this missing component.  Additionally, there is a discontinuity in the forces.  This can be remedied with the use of a switching function to zero the potential and forces smoothly as particles near $R_\textrm{c}$.  
336 >
337 > If the potential, $v(r)$, is taken to be the normal Coulomb potential,
338 > \begin{equation}
339 > v(r) = \frac{q_i q_j}{r},
340 > \label{eq:Coulomb}
341 > \end{equation}
342 > then the Shifted Potential ({\sc sp}) forms will give Wolf {\it et
343 > al.}'s undamped prescription:
344 > \begin{equation}
345 > V_\textrm{SP}(r) =
346 > q_iq_j\left(\frac{1}{r}-\frac{1}{R_\textrm{c}}\right) \quad
347 > r\leqslant R_\textrm{c},
348 > \label{eq:SPPot}
349 > \end{equation}
350 > with associated forces,
351 > \begin{equation}
352 > F_\textrm{SP}(r) = q_iq_j\left(\frac{1}{r^2}\right) \quad r\leqslant R_\textrm{c}.
353 > \label{eq:SPForces}
354 > \end{equation}
355 > These forces are identical to the forces of the standard Coulomb
356 > interaction, and cutting these off at $R_c$ was addressed by Wolf
357 > \textit{et al.} as undesirable.  They pointed out that the effect of
358 > the image charges is neglected in the forces when this form is
359 > used,\cite{Wolf99} thereby eliminating any benefit from the method in
360 > molecular dynamics.  Additionally, there is a discontinuity in the
361 > forces at the cutoff radius which results in energy drift during MD
362 > simulations.
363  
364 < If the derivative term in equation \ref{eq:shiftingForm} is evaluated, we obtain an hitherto undiscussed shifted force Coulomb potential,
364 > The shifted force ({\sc sf}) form using the normal Coulomb potential
365 > will give,
366   \begin{equation}
367 < V^\textrm{SF}(r_{ij}) = q_iq_j\left[\frac{1}{r_{ij}}-\frac{1}{R_\textrm{c}}+\left(\frac{1}{R_\textrm{c}^2}\right)(r_{ij}-R_\textrm{c})\right] \quad r_{ij}\leqslant R_\textrm{c}.
367 > 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}.
368   \label{eq:SFPot}
369   \end{equation}
370 < Taking the derivative of this shifted force potential gives the
225 < following forces,
370 > with associated forces,
371   \begin{equation}
372 < F^\textrm{SF}(r_{ij} =  q_iq_j\left(-\frac{1}{r_{ij}^2}+\frac{1}{R_\textrm{c}^2}\right) \quad r_{ij}\leqslant R_\textrm{c}.
372 > 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}.
373   \label{eq:SFForces}
374   \end{equation}
375 < Using this formulation rather than the simple shifted potential
376 < (Eq. \ref{eq:WolfSP}) means that there are no discontinuities in the
377 < forces in addition to the potential.  This form also has the benefit
378 < that the image charges have a force presence, addressing the concerns
379 < about a missing physical component.  One side effect of this treatment
380 < is a slight alteration in the shape of the potential that comes about
381 < from the derivative term.  Thus, a degree of clarity about the
382 < original formulation of the potential is lost in order to gain
383 < functionality in dynamics simulations.
375 > This formulation has the benefits that there are no discontinuities at
376 > the cutoff radius, while the neutralizing image charges are present in
377 > both the energy and force expressions.  It would be simple to add the
378 > self-neutralizing term back when computing the total energy of the
379 > system, thereby maintaining the agreement with the Madelung energies.
380 > A side effect of this treatment is the alteration in the shape of the
381 > potential that comes from the derivative term.  Thus, a degree of
382 > clarity about agreement with the empirical potential is lost in order
383 > to gain functionality in dynamics simulations.
384  
385   Wolf \textit{et al.} originally discussed the energetics of the
386 < shifted Coulomb potential (Eq. \ref{eq:WolfSP}), and they found that
387 < it was still insufficient for accurate determination of the energy.
388 < The energy would fluctuate around the expected value with increasing
389 < cutoff radius, but the oscillations appeared to be converging toward
390 < the correct value.\cite{Wolf99} A damping function was incorporated to
391 < accelerate convergence; and though alternative functional forms could
392 < be used,\cite{Jones56,Heyes81} the complimentary error function was
393 < chosen to draw parallels to the Ewald summation.  Incorporating
394 < damping into the simple Coulomb potential,
386 > shifted Coulomb potential (Eq. \ref{eq:SPPot}) and found that it was
387 > insufficient for accurate determination of the energy with reasonable
388 > cutoff distances.  The calculated Madelung energies fluctuated around
389 > the expected value as the cutoff radius was increased, but the
390 > oscillations converged toward the correct value.\cite{Wolf99} A
391 > damping function was incorporated to accelerate the convergence; and
392 > though alternative forms for the damping function could be
393 > used,\cite{Jones56,Heyes81} the complimentary error function was
394 > chosen to mirror the effective screening used in the Ewald summation.
395 > Incorporating this error function damping into the simple Coulomb
396 > potential,
397   \begin{equation}
398 < v(r_{ij}) = \frac{\mathrm{erfc}\left(\alpha r_{ij}\right)}{r_{ij}},
398 > v(r) = \frac{\mathrm{erfc}\left(\alpha r\right)}{r},
399   \label{eq:dampCoulomb}
400   \end{equation}
401 < the shifted potential (Eq. \ref{eq:WolfSP}) can be rederived
255 < \textit{via} equation \ref{eq:shiftingForm},
401 > the shifted potential (eq. (\ref{eq:SPPot})) becomes
402   \begin{equation}
403 < V^{\textrm{DSP}}(r_{ij}) = q_iq_j\left(\frac{\textrm{erfc}(\alpha r_{ij})}{r_{ij}}-\frac{\textrm{erfc}(\alpha R_\textrm{c})}{R_\textrm{c}}\right) \quad r_{ij}\leqslant R_\textrm{c}.
403 > 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},
404   \label{eq:DSPPot}
405   \end{equation}
406 < The derivative of this Shifted-Potential can be taken to obtain forces
261 < for use in MD,
406 > with associated forces,
407   \begin{equation}
408 < F^{\textrm{DSP}}(r_{ij}) = q_iq_j\left(-\frac{\textrm{erfc}(\alpha r_{ij})}{r^2_{ij}}-\frac{2\alpha}{\pi^{1/2}}\frac{\exp{(-\alpha^2r_{ij}^2)}}{r_{ij}}\right) \quad r_{ij}\leqslant R_\textrm{c}.
408 > 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}.
409   \label{eq:DSPForces}
410   \end{equation}
411 < Again, this Shifted-Potential suffers from a discontinuity in the
412 < forces, and a lack of an image-charge component in the forces.  To
413 < remedy these concerns, a Shifted-Force variant is obtained by
414 < inclusion of the derivative term in equation \ref{eq:shiftingForm} to
415 < give,
411 > Again, this damped shifted potential suffers from a
412 > force-discontinuity at the cutoff radius, and the image charges play
413 > no role in the forces.  To remedy these concerns, one may derive a
414 > {\sc sf} variant by including the derivative term in
415 > eq. (\ref{eq:shiftingForm}),
416   \begin{equation}
417   \begin{split}
418 < V^\mathrm{DSF}(r_{ij}) = q_iq_j\Biggr{[}&\frac{\mathrm{erfc}\left(\alpha r_{ij}\right)}{r_{ij}}-\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_{ij}-R_\mathrm{c}\right)\ \right] \quad r_{ij}\leqslant R_\textrm{c}.
418 > 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}.
419   \label{eq:DSFPot}
420   \end{split}
421   \end{equation}
422 < The derivative of the above potential gives the following forces,
422 > The derivative of the above potential will lead to the following forces,
423   \begin{equation}
424   \begin{split}
425 < F^\mathrm{DSF}(r_{ij}) = q_iq_j\Biggr{[}&-\left(\frac{\textrm{erfc}(\alpha r_{ij})}{r^2_{ij}}+\frac{2\alpha}{\pi^{1/2}}\frac{\exp{(-\alpha^2r_{ij}^2)}}{r_{ij}}\right) \\ &\left.+\left(\frac{\textrm{erfc}(\alpha R_{\textrm{c}})}{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_{ij}\leqslant R_\textrm{c}.
425 > 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}.
426   \label{eq:DSFForces}
427   \end{split}
428   \end{equation}
429 + If the damping parameter $(\alpha)$ is set to zero, the undamped case,
430 + eqs. (\ref{eq:SPPot} through \ref{eq:SFForces}) are correctly
431 + recovered from eqs. (\ref{eq:DSPPot} through \ref{eq:DSFForces}).
432  
433 < This new Shifted-Force potential is similar to equation
434 < \ref{eq:ZahnPot} derived by Zahn \textit{et al.}; however, there are
435 < two important differences.\cite{Zahn02} First, the $v_\textrm{c}$ term
436 < from equation \ref{eq:shiftingForm} is equal to equation
437 < \ref{eq:dampCoulomb} with $R_\textrm{c}$ supplied for $r_{ij}$.  This
438 < term is not present in the Zahn potential, resulting in a
439 < discontinuity as particles cross $R_\textrm{c}$.  Second, the sign of
440 < the derivative portion is different.  The constant $v_\textrm{c}$ term
441 < is not going to have a presence in the forces after performing the
442 < derivative, but the negative sign does effect the derivative.  In
443 < fact, it introduces a discontinuity in the forces at the cutoff,
433 > This new {\sc sf} potential is similar to equation \ref{eq:ZahnPot}
434 > derived by Zahn \textit{et al.}; however, there are two important
435 > differences.\cite{Zahn02} First, the $v_\textrm{c}$ term from
436 > eq. (\ref{eq:shiftingForm}) is equal to eq. (\ref{eq:dampCoulomb})
437 > with $r$ replaced by $R_\textrm{c}$.  This term is {\it not} present
438 > in the Zahn potential, resulting in a potential discontinuity as
439 > particles cross $R_\textrm{c}$.  Second, the sign of the derivative
440 > portion is different.  The missing $v_\textrm{c}$ term would not
441 > affect molecular dynamics simulations (although the computed energy
442 > would be expected to have sudden jumps as particle distances crossed
443 > $R_c$).  The sign problem is a potential source of errors, however.
444 > In fact, it introduces a discontinuity in the forces at the cutoff,
445   because the force function is shifted in the wrong direction and
446 < doesn't cross zero at $R_\textrm{c}$.  Thus, these alterations make
298 < for an electrostatic summation method that is continuous in both the
299 < potential and forces and incorporates the pairwise sum considerations
300 < stressed by Wolf \textit{et al.}\cite{Wolf99}
446 > doesn't cross zero at $R_\textrm{c}$.
447  
448 + Eqs. (\ref{eq:DSFPot}) and (\ref{eq:DSFForces}) result in an
449 + electrostatic summation method in which the potential and forces are
450 + continuous at the cutoff radius and which incorporates the damping
451 + function proposed by Wolf \textit{et al.}\cite{Wolf99} In the rest of
452 + this paper, we will evaluate exactly how good these methods ({\sc sp},
453 + {\sc sf}, damping) are at reproducing the correct electrostatic
454 + summation performed by the Ewald sum.
455 +
456 + \subsection{Other alternatives}
457 + In addition to the methods described above, we considered some other
458 + techniques that are commonly used in molecular simulations.  The
459 + simplest of these is group-based cutoffs.  Though of little use for
460 + charged molecules, collecting atoms into neutral groups takes
461 + advantage of the observation that the electrostatic interactions decay
462 + faster than those for monopolar pairs.\cite{Steinbach94} When
463 + considering these molecules as neutral groups, the relative
464 + orientations of the molecules control the strength of the interactions
465 + at the cutoff radius.  Consequently, as these molecular particles move
466 + through $R_\textrm{c}$, the energy will drift upward due to the
467 + anisotropy of the net molecular dipole interactions.\cite{Rahman71} To
468 + maintain good energy conservation, both the potential and derivative
469 + need to be smoothly switched to zero at $R_\textrm{c}$.\cite{Adams79}
470 + This is accomplished using a standard switching function.  If a smooth
471 + second derivative is desired, a fifth (or higher) order polynomial can
472 + be used.\cite{Andrea83}
473 +
474 + Group-based cutoffs neglect the surroundings beyond $R_\textrm{c}$,
475 + and to incorporate the effects of the surroundings, a method like
476 + Reaction Field ({\sc rf}) can be used.  The original theory for {\sc
477 + rf} was originally developed by Onsager,\cite{Onsager36} and it was
478 + applied in simulations for the study of water by Barker and
479 + Watts.\cite{Barker73} In modern simulation codes, {\sc rf} is simply
480 + an extension of the group-based cutoff method where the net dipole
481 + within the cutoff sphere polarizes an external dielectric, which
482 + reacts back on the central dipole.  The same switching function
483 + considerations for group-based cutoffs need to made for {\sc rf}, with
484 + the additional pre-specification of a dielectric constant.
485 +
486   \section{Methods}
487  
304 \subsection{What Qualities are Important?}\label{sec:Qualities}
488   In classical molecular mechanics simulations, there are two primary
489   techniques utilized to obtain information about the system of
490   interest: Monte Carlo (MC) and Molecular Dynamics (MD).  Both of these
491   techniques utilize pairwise summations of interactions between
492   particle sites, but they use these summations in different ways.
493  
494 < In MC, the potential energy difference between two subsequent
495 < configurations dictates the progression of MC sampling.  Going back to
496 < the origins of this method, the Canonical ensemble acceptance criteria
497 < laid out by Metropolis \textit{et al.} states that a subsequent
498 < configuration is accepted if $\Delta E < 0$ or if $\xi < \exp(-\Delta
499 < E/kT)$, where $\xi$ is a random number between 0 and
500 < 1.\cite{Metropolis53} Maintaining a consistent $\Delta E$ when using
501 < an alternate method for handling the long-range electrostatics ensures
502 < proper sampling within the ensemble.
494 > In MC, the potential energy difference between configurations dictates
495 > the progression of MC sampling.  Going back to the origins of this
496 > method, the acceptance criterion for the canonical ensemble laid out
497 > by Metropolis \textit{et al.} states that a subsequent configuration
498 > is accepted if $\Delta E < 0$ or if $\xi < \exp(-\Delta E/kT)$, where
499 > $\xi$ is a random number between 0 and 1.\cite{Metropolis53}
500 > Maintaining the correct $\Delta E$ when using an alternate method for
501 > handling the long-range electrostatics will ensure proper sampling
502 > from the ensemble.
503  
504 < In MD, the derivative of the potential directs how the system will
504 > In MD, the derivative of the potential governs how the system will
505   progress in time.  Consequently, the force and torque vectors on each
506 < body in the system dictate how it develops as a whole.  If the
507 < magnitude and direction of these vectors are similar when using
508 < alternate electrostatic summation techniques, the dynamics in the near
509 < term will be indistinguishable.  Because error in MD calculations is
510 < cumulative, one should expect greater deviation in the long term
511 < trajectories with greater differences in these vectors between
512 < configurations using different long-range electrostatics.
506 > body in the system dictate how the system evolves.  If the magnitude
507 > and direction of these vectors are similar when using alternate
508 > electrostatic summation techniques, the dynamics in the short term
509 > will be indistinguishable.  Because error in MD calculations is
510 > cumulative, one should expect greater deviation at longer times,
511 > although methods which have large differences in the force and torque
512 > vectors will diverge from each other more rapidly.
513  
514   \subsection{Monte Carlo and the Energy Gap}\label{sec:MCMethods}
332 Evaluation of the pairwise summation techniques (outlined in section
333 \ref{sec:ESMethods}) for use in MC simulations was performed through
334 study of the energy differences between conformations.  Considering
335 the SPME results to be the correct or desired behavior, ideal
336 performance of a tested method was taken to be agreement between the
337 energy differences calculated.  Linear least squares regression of the
338 $\Delta E$ values between configurations using SPME against $\Delta E$
339 values using tested methods provides a quantitative comparison of this
340 agreement.  Unitary results for both the correlation and correlation
341 coefficient for these regressions indicate equivalent energetic
342 results between the methods.  The correlation is the slope of the
343 plotted data while the correlation coefficient ($R^2$) is a measure of
344 the of the data scatter around the fitted line and tells about the
345 quality of the fit (Fig. \ref{fig:linearFit}).
515  
516 + The pairwise summation techniques (outlined in section
517 + \ref{sec:ESMethods}) were evaluated for use in MC simulations by
518 + studying the energy differences between conformations.  We took the
519 + SPME-computed energy difference between two conformations to be the
520 + correct behavior. An ideal performance by an alternative method would
521 + reproduce these energy differences exactly (even if the absolute
522 + energies calculated by the methods are different).  Since none of the
523 + methods provide exact energy differences, we used linear least squares
524 + regressions of energy gap data to evaluate how closely the methods
525 + mimicked the Ewald energy gaps.  Unitary results for both the
526 + correlation (slope) and correlation coefficient for these regressions
527 + indicate perfect agreement between the alternative method and SPME.
528 + Sample correlation plots for two alternate methods are shown in
529 + Fig. \ref{fig:linearFit}.
530 +
531   \begin{figure}
532   \centering
533   \includegraphics[width = \linewidth]{./dualLinear.pdf}
534 < \caption{Example least squares regressions of the configuration energy differences for SPC/E water systems. The upper plot shows a data set with a poor correlation coefficient ($R^2$), while the lower plot shows a data set with a good correlation coefficient.}
535 < \label{fig:linearFit}
534 > \caption{Example least squares regressions of the configuration energy
535 > differences for SPC/E water systems. The upper plot shows a data set
536 > with a poor correlation coefficient ($R^2$), while the lower plot
537 > shows a data set with a good correlation coefficient.}
538 > \label{fig:linearFit}
539   \end{figure}
540  
541 < Each system type (detailed in section \ref{sec:RepSims}) studied
542 < consisted of 500 independent configurations, each equilibrated from
543 < higher temperature trajectories. Thus, 124,750 $\Delta E$ data points
544 < are used in a regression of a single system type.  Results and
545 < discussion for the individual analysis of each of the system types
359 < appear in the supporting information, while the cumulative results
360 < over all the investigated systems appears below in section
361 < \ref{sec:EnergyResults}.
541 > Each system type (detailed in section \ref{sec:RepSims}) was
542 > represented using 500 independent configurations.  Additionally, we
543 > used seven different system types, so each of the alternative
544 > (non-Ewald) electrostatic summation methods was evaluated using
545 > 873,250 configurational energy differences.
546  
547 + Results and discussion for the individual analysis of each of the
548 + system types appear in the supporting information, while the
549 + cumulative results over all the investigated systems appears below in
550 + section \ref{sec:EnergyResults}.
551 +
552   \subsection{Molecular Dynamics and the Force and Torque Vectors}\label{sec:MDMethods}
553 < Evaluation of the pairwise methods (outlined in section
554 < \ref{sec:ESMethods}) for use in MD simulations was performed through
555 < comparison of the force and torque vectors obtained with those from
556 < SPME.  Both the magnitude and the direction of these vectors on each
557 < of the bodies in the system were analyzed.  For the magnitude of these
558 < vectors, linear least squares regression analysis can be performed as
559 < described previously for comparing $\Delta E$ values. Instead of a
560 < single value between two system configurations, there is a value for
561 < each particle in each configuration.  For a system of 1000 water
562 < molecules and 40 ions, there are 1040 force vectors and 1000 torque
563 < vectors.  With 500 configurations, this results in 520,000 force and
564 < 500,000 torque vector comparisons samples for each system type.
553 > We evaluated the pairwise methods (outlined in section
554 > \ref{sec:ESMethods}) for use in MD simulations by
555 > comparing the force and torque vectors with those obtained using the
556 > reference Ewald summation (SPME).  Both the magnitude and the
557 > direction of these vectors on each of the bodies in the system were
558 > analyzed.  For the magnitude of these vectors, linear least squares
559 > regression analyses were performed as described previously for
560 > comparing $\Delta E$ values.  Instead of a single energy difference
561 > between two system configurations, we compared the magnitudes of the
562 > forces (and torques) on each molecule in each configuration.  For a
563 > system of 1000 water molecules and 40 ions, there are 1040 force
564 > vectors and 1000 torque vectors.  With 500 configurations, this
565 > results in 520,000 force and 500,000 torque vector comparisons.
566 > Additionally, data from seven different system types was aggregated
567 > before the comparison was made.
568  
569 < The force and torque vector directions were investigated through
570 < measurement of the angle ($\theta$) formed between those from the
571 < particular method and those from SPME
569 > The {\it directionality} of the force and torque vectors was
570 > investigated through measurement of the angle ($\theta$) formed
571 > between those computed from the particular method and those from SPME,
572   \begin{equation}
573 < \theta_F = \frac{\vec{F}_\textrm{SPME}}{|\vec{F}_\textrm{SPME}|}\cdot\frac{\vec{F}_\textrm{Method}}{|\vec{F}_\textrm{Method}|}.
573 > \theta_f = \cos^{-1} \left(\hat{F}_\textrm{SPME} \cdot \hat{F}_\textrm{M}\right),
574   \end{equation}
575 < Each of these $\theta$ values was accumulated in a distribution
576 < function, weighted by the area on the unit sphere.  Non-linear fits
577 < were used to measure the shape of the resulting distributions.
575 > where $\hat{f}_\textrm{M}$ is the unit vector pointing along the force
576 > vector computed using method M.  Each of these $\theta$ values was
577 > accumulated in a distribution function and weighted by the area on the
578 > unit sphere.  Since this distribution is a measure of angular error
579 > between two different electrostatic summation methods, there is no
580 > {\it a priori} reason for the profile to adhere to any specific
581 > shape. Thus, gaussian fits were used to measure the width of the
582 > resulting distributions.
583 > %
584 > %\begin{figure}
585 > %\centering
586 > %\includegraphics[width = \linewidth]{./gaussFit.pdf}
587 > %\caption{Sample fit of the angular distribution of the force vectors
588 > %accumulated using all of the studied systems.  Gaussian fits were used
589 > %to obtain values for the variance in force and torque vectors.}
590 > %\label{fig:gaussian}
591 > %\end{figure}
592 > %
593 > %Figure \ref{fig:gaussian} shows an example distribution with applied
594 > %non-linear fits.  The solid line is a Gaussian profile, while the
595 > %dotted line is a Voigt profile, a convolution of a Gaussian and a
596 > %Lorentzian.  
597 > %Since this distribution is a measure of angular error between two
598 > %different electrostatic summation methods, there is no {\it a priori}
599 > %reason for the profile to adhere to any specific shape.
600 > %Gaussian fits was used to compare all the tested methods.  
601 > The variance ($\sigma^2$) was extracted from each of these fits and
602 > was used to compare distribution widths.  Values of $\sigma^2$ near
603 > zero indicate vector directions indistinguishable from those
604 > calculated when using the reference method (SPME).
605  
606 < \begin{figure}
388 < \centering
389 < \includegraphics[width = \linewidth]{./gaussFit.pdf}
390 < \caption{Sample fit of the angular distribution of the force vectors over all of the studied systems.  Gaussian fits were used to obtain values for the variance in force and torque vectors used in the following figure.}
391 < \label{fig:gaussian}
392 < \end{figure}
606 > \subsection{Short-time Dynamics}
607  
608 < Figure \ref{fig:gaussian} shows an example distribution with applied
609 < non-linear fits.  The solid line is a Gaussian profile, while the
610 < dotted line is a Voigt profile, a convolution of a Gaussian and a
611 < Lorentzian.  Since this distribution is a measure of angular error
612 < between two different electrostatic summation methods, there is
613 < particular reason for the profile to adhere to a specific shape.
614 < Because of this and the Gaussian profile's more statistically
615 < meaningful properties, Gaussian fits was used to compare all the
616 < tested methods.  The variance ($\sigma^2$) was extracted from each of
617 < these fits and was used to compare distribution widths.  Values of
404 < $\sigma^2$ near zero indicate vector directions indistinguishable from
405 < those calculated when using SPME.
406 <
407 < \subsection{Long-Time and Collective Motion}\label{sec:LongTimeMethods}
408 < Evaluation of the long-time dynamics of charged systems was performed
409 < by considering the NaCl crystal system while using a subset of the
410 < best performing pairwise methods.  The NaCl crystal was chosen to
411 < avoid possible complications involving the propagation techniques of
412 < orientational motion in molecular systems.  To enhance the atomic
413 < motion, these crystals were equilibrated at 1000 K, near the
414 < experimental $T_m$ for NaCl.  Simulations were performed under the
415 < microcanonical ensemble, and velocity autocorrelation functions
416 < (Eq. \ref{eq:vCorr}) were computed for each of the trajectories,
608 > The effects of the alternative electrostatic summation methods on the
609 > short-time dynamics of charged systems were evaluated by considering a
610 > NaCl crystal at a temperature of 1000 K.  A subset of the best
611 > performing pairwise methods was used in this comparison.  The NaCl
612 > crystal was chosen to avoid possible complications from the treatment
613 > of orientational motion in molecular systems.  All systems were
614 > started with the same initial positions and velocities.  Simulations
615 > were performed under the microcanonical ensemble, and velocity
616 > autocorrelation functions (Eq. \ref{eq:vCorr}) were computed for each
617 > of the trajectories,
618   \begin{equation}
619 < C_v(t) = \langle v_i(0)\cdot v_i(t)\rangle.
619 > C_v(t) = \frac{\langle v_i(0)\cdot v_i(t)\rangle}{\langle v_i(0)\cdot v_i(0)\rangle}.
620   \label{eq:vCorr}
621   \end{equation}
622 < Velocity autocorrelation functions require detailed short time data
623 < and long trajectories for good statistics, thus velocity information
624 < was saved every 5 fs over 100 ps trajectories.  The power spectrum
625 < ($I(\omega)$) is obtained via Fourier transform of the autocorrelation
626 < function
627 < \begin{equation}
628 < I(\omega) = \frac{1}{2\pi}\int^{\infty}_{-\infty}C_v(t)e^{-i\omega t}dt,
622 > Velocity autocorrelation functions require detailed short time data,
623 > thus velocity information was saved every 2 fs over 10 ps
624 > trajectories. Because the NaCl crystal is composed of two different
625 > atom types, the average of the two resulting velocity autocorrelation
626 > functions was used for comparisons.
627 >
628 > \subsection{Long-Time and Collective Motion}\label{sec:LongTimeMethods}
629 >
630 > The effects of the same subset of alternative electrostatic methods on
631 > the {\it long-time} dynamics of charged systems were evaluated using
632 > the same model system (NaCl crystals at 1000K).  The power spectrum
633 > ($I(\omega)$) was obtained via Fourier transform of the velocity
634 > autocorrelation function, \begin{equation} I(\omega) =
635 > \frac{1}{2\pi}\int^{\infty}_{-\infty}C_v(t)e^{-i\omega t}dt,
636   \label{eq:powerSpec}
637   \end{equation}
638 < where the frequency, $\omega=0,\ 1,\ ...,\ N-1$.
638 > where the frequency, $\omega=0,\ 1,\ ...,\ N-1$. Again, because the
639 > NaCl crystal is composed of two different atom types, the average of
640 > the two resulting power spectra was used for comparisons. Simulations
641 > were performed under the microcanonical ensemble, and velocity
642 > information was saved every 5 fs over 100 ps trajectories.
643  
644   \subsection{Representative Simulations}\label{sec:RepSims}
645 < A variety of common and representative simulations were analyzed to
646 < determine the relative effectiveness of the pairwise summation
647 < techniques in reproducing the energetics and dynamics exhibited by
648 < SPME.  The studied systems were as follows:
645 > A variety of representative simulations were analyzed to determine the
646 > relative effectiveness of the pairwise summation techniques in
647 > reproducing the energetics and dynamics exhibited by SPME.  We wanted
648 > to span the space of modern simulations (i.e. from liquids of neutral
649 > molecules to ionic crystals), so the systems studied were:
650   \begin{enumerate}
651 < \item Liquid Water
652 < \item Crystalline Water (Ice I$_\textrm{c}$)
653 < \item NaCl Crystal
654 < \item NaCl Melt
655 < \item Low Ionic Strength Solution of NaCl in Water
656 < \item High Ionic Strength Solution of NaCl in Water
657 < \item 6 \AA\  Radius Sphere of Argon in Water
651 > \item liquid water (SPC/E),\cite{Berendsen87}
652 > \item crystalline water (Ice I$_\textrm{c}$ crystals of SPC/E),
653 > \item NaCl crystals,
654 > \item NaCl melts,
655 > \item a low ionic strength solution of NaCl in water (0.11 M),
656 > \item a high ionic strength solution of NaCl in water (1.1 M), and
657 > \item a 6 \AA\  radius sphere of Argon in water.
658   \end{enumerate}
659   By utilizing the pairwise techniques (outlined in section
660   \ref{sec:ESMethods}) in systems composed entirely of neutral groups,
661 < charged particles, and mixtures of the two, we can comment on possible
662 < system dependence and/or universal applicability of the techniques.
661 > charged particles, and mixtures of the two, we hope to discern under
662 > which conditions it will be possible to use one of the alternative
663 > summation methodologies instead of the Ewald sum.
664  
665 < Generation of the system configurations was dependent on the system
666 < type.  For the solid and liquid water configurations, configuration
667 < snapshots were taken at regular intervals from higher temperature 1000
668 < SPC/E water molecule trajectories and each equilibrated individually.
669 < The solid and liquid NaCl systems consisted of 500 Na+ and 500 Cl-
670 < ions and were selected and equilibrated in the same fashion as the
671 < water systems.  For the low and high ionic strength NaCl solutions, 4
672 < and 40 ions were first solvated in a 1000 water molecule boxes
673 < respectively.  Ion and water positions were then randomly swapped, and
665 > For the solid and liquid water configurations, configurations were
666 > taken at regular intervals from high temperature trajectories of 1000
667 > SPC/E water molecules.  Each configuration was equilibrated
668 > independently at a lower temperature (300~K for the liquid, 200~K for
669 > the crystal).  The solid and liquid NaCl systems consisted of 500
670 > $\textrm{Na}^{+}$ and 500 $\textrm{Cl}^{-}$ ions.  Configurations for
671 > these systems were selected and equilibrated in the same manner as the
672 > water systems.  The equilibrated temperatures were 1000~K for the NaCl
673 > crystal and 7000~K for the liquid. The ionic solutions were made by
674 > solvating 4 (or 40) ions in a periodic box containing 1000 SPC/E water
675 > molecules.  Ion and water positions were then randomly swapped, and
676   the resulting configurations were again equilibrated individually.
677 < Finally, for the Argon/Water "charge void" systems, the identities of
678 < all the SPC/E waters within 6 \AA\ of the center of the equilibrated
679 < water configurations were converted to argon
680 < (Fig. \ref{fig:argonSlice}).
677 > Finally, for the Argon / Water ``charge void'' systems, the identities
678 > of all the SPC/E waters within 6 \AA\ of the center of the
679 > equilibrated water configurations were converted to argon.
680 > %(Fig. \ref{fig:argonSlice}).
681  
682 < \begin{figure}
683 < \centering
684 < \includegraphics[width = \linewidth]{./slice.pdf}
685 < \caption{A slice from the center of a water box used in a charge void simulation.  The darkened region represents the boundary sphere within which the water molecules were converted to argon atoms.}
470 < \label{fig:argonSlice}
471 < \end{figure}
682 > These procedures guaranteed us a set of representative configurations
683 > from chemically-relevant systems sampled from appropriate
684 > ensembles. Force field parameters for the ions and Argon were taken
685 > from the force field utilized by {\sc oopse}.\cite{Meineke05}
686  
687 < \subsection{Electrostatic Summation Methods}\label{sec:ESMethods}
688 < Electrostatic summation method comparisons were performed using SPME,
689 < the Shifted-Potential and Shifted-Force methods - both with damping
690 < parameters ($\alpha$) of 0.0, 0.1, 0.2, and 0.3 \AA$^{-1}$ (no, weak,
691 < moderate, and strong damping respectively), reaction field with an
692 < infinite dielectric constant, and an unmodified cutoff.  Group-based
693 < cutoffs with a fifth-order polynomial switching function were
694 < necessary for the reaction field simulations and were utilized in the
481 < SP, SF, and pure cutoff methods for comparison to the standard lack of
482 < group-based cutoffs with a hard truncation.  The SPME calculations
483 < were performed using the TINKER implementation of SPME,\cite{Ponder87}
484 < while all other method calculations were performed using the OOPSE
485 < molecular mechanics package.\cite{Meineke05}
687 > %\begin{figure}
688 > %\centering
689 > %\includegraphics[width = \linewidth]{./slice.pdf}
690 > %\caption{A slice from the center of a water box used in a charge void
691 > %simulation.  The darkened region represents the boundary sphere within
692 > %which the water molecules were converted to argon atoms.}
693 > %\label{fig:argonSlice}
694 > %\end{figure}
695  
696 < These methods were additionally evaluated with three different cutoff
697 < radii (9, 12, and 15 \AA) to investigate possible cutoff radius
698 < dependence.  It should be noted that the damping parameter chosen in
699 < SPME, or so called ``Ewald Coefficient", has a significant effect on
700 < the energies and forces calculated.  Typical molecular mechanics
701 < packages default this to a value dependent on the cutoff radius and a
702 < tolerance (typically less than $1 \times 10^{-4}$ kcal/mol).  Smaller
703 < tolerances are typically associated with increased accuracy in the
704 < real-space portion of the summation.\cite{Essmann95} The default
705 < TINKER tolerance of $1 \times 10^{-8}$ kcal/mol was used in all SPME
706 < calculations, resulting in Ewald Coefficients of 0.4200, 0.3119, and
707 < 0.2476 \AA$^{-1}$ for cutoff radii of 9, 12, and 15 \AA\ respectively.
696 > \subsection{Comparison of Summation Methods}\label{sec:ESMethods}
697 > We compared the following alternative summation methods with results
698 > from the reference method (SPME):
699 > \begin{itemize}
700 > \item {\sc sp} with damping parameters ($\alpha$) of 0.0, 0.1, 0.2,
701 > and 0.3 \AA$^{-1}$,
702 > \item {\sc sf} with damping parameters ($\alpha$) of 0.0, 0.1, 0.2,
703 > and 0.3 \AA$^{-1}$,
704 > \item reaction field with an infinite dielectric constant, and
705 > \item an unmodified cutoff.
706 > \end{itemize}
707 > Group-based cutoffs with a fifth-order polynomial switching function
708 > were utilized for the reaction field simulations.  Additionally, we
709 > investigated the use of these cutoffs with the SP, SF, and pure
710 > cutoff.  The SPME electrostatics were performed using the TINKER
711 > implementation of SPME,\cite{Ponder87} while all other calculations
712 > were performed using the {\sc oopse} molecular mechanics
713 > package.\cite{Meineke05} All other portions of the energy calculation
714 > (i.e. Lennard-Jones interactions) were handled in exactly the same
715 > manner across all systems and configurations.
716  
717 + The althernative methods were also evaluated with three different
718 + cutoff radii (9, 12, and 15 \AA).  As noted previously, the
719 + convergence parameter ($\alpha$) plays a role in the balance of the
720 + real-space and reciprocal-space portions of the Ewald calculation.
721 + Typical molecular mechanics packages set this to a value dependent on
722 + the cutoff radius and a tolerance (typically less than $1 \times
723 + 10^{-4}$ kcal/mol).  Smaller tolerances are typically associated with
724 + increasing accuracy at the expense of computational time spent on the
725 + reciprocal-space portion of the summation.\cite{Perram88,Essmann95}
726 + The default TINKER tolerance of $1 \times 10^{-8}$ kcal/mol was used
727 + in all SPME calculations, resulting in Ewald coefficients of 0.4200,
728 + 0.3119, and 0.2476 \AA$^{-1}$ for cutoff radii of 9, 12, and 15 \AA\
729 + respectively.
730 +
731   \section{Results and Discussion}
732  
733   \subsection{Configuration Energy Differences}\label{sec:EnergyResults}
# Line 509 | Line 740 | figure \ref{fig:delE}.
740   \begin{figure}
741   \centering
742   \includegraphics[width=5.5in]{./delEplot.pdf}
743 < \caption{Statistical analysis of the quality of configurational energy differences for a given electrostatic method compared with the reference Ewald sum.  Results with a value equal to 1 (dashed line) indicate $\Delta E$ values indistinguishable from those obtained using SPME.  Different values of the cutoff radius are indicated with different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ = inverted triangles).}
743 > \caption{Statistical analysis of the quality of configurational energy
744 > differences for a given electrostatic method compared with the
745 > reference Ewald sum.  Results with a value equal to 1 (dashed line)
746 > indicate $\Delta E$ values indistinguishable from those obtained using
747 > SPME.  Different values of the cutoff radius are indicated with
748 > different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ =
749 > inverted triangles).}
750   \label{fig:delE}
751   \end{figure}
752  
753 < In this figure, it is apparent that it is unreasonable to expect
754 < realistic results using an unmodified cutoff.  This is not all that
755 < surprising since this results in large energy fluctuations as atoms
756 < move in and out of the cutoff radius.  These fluctuations can be
757 < alleviated to some degree by using group based cutoffs with a
758 < switching function.\cite{Steinbach94} The Group Switch Cutoff row
522 < doesn't show a significant improvement in this plot because the salt
523 < and salt solution systems contain non-neutral groups, see the
524 < accompanying supporting information for a comparison where all groups
525 < are neutral.
753 > The most striking feature of this plot is how well the Shifted Force
754 > ({\sc sf}) and Shifted Potential ({\sc sp}) methods capture the energy
755 > differences.  For the undamped {\sc sf} method, and the
756 > moderately-damped {\sc sp} methods, the results are nearly
757 > indistinguishable from the Ewald results.  The other common methods do
758 > significantly less well.  
759  
760 < Correcting the resulting charged cutoff sphere is one of the purposes
761 < of the damped Coulomb summation proposed by Wolf \textit{et
762 < al.},\cite{Wolf99} and this correction indeed improves the results as
763 < seen in the Shifted-Potental rows.  While the undamped case of this
764 < method is a significant improvement over the pure cutoff, it still
765 < doesn't correlate that well with SPME.  Inclusion of potential damping
766 < improves the results, and using an $\alpha$ of 0.2 \AA $^{-1}$ shows
767 < an excellent correlation and quality of fit with the SPME results,
768 < particularly with a cutoff radius greater than 12 \AA .  Use of a
769 < larger damping parameter is more helpful for the shortest cutoff
537 < shown, but it has a detrimental effect on simulations with larger
538 < cutoffs.  In the Shifted-Force sets, increasing damping results in
539 < progressively poorer correlation.  Overall, the undamped case is the
540 < best performing set, as the correlation and quality of fits are
541 < consistently superior regardless of the cutoff distance.  This result
542 < is beneficial in that the undamped case is less computationally
543 < prohibitive do to the lack of complimentary error function calculation
544 < when performing the electrostatic pair interaction.  The reaction
545 < field results illustrates some of that method's limitations, primarily
546 < that it was developed for use in homogenous systems; although it does
547 < provide results that are an improvement over those from an unmodified
548 < cutoff.
760 > The unmodified cutoff method is essentially unusable.  This is not
761 > surprising since hard cutoffs give large energy fluctuations as atoms
762 > or molecules move in and out of the cutoff
763 > radius.\cite{Rahman71,Adams79} These fluctuations can be alleviated to
764 > some degree by using group based cutoffs with a switching
765 > function.\cite{Adams79,Steinbach94,Leach01} However, we do not see
766 > significant improvement using the group-switched cutoff because the
767 > salt and salt solution systems contain non-neutral groups.  Interested
768 > readers can consult the accompanying supporting information for a
769 > comparison where all groups are neutral.
770  
771 + For the {\sc sp} method, inclusion of electrostatic damping improves
772 + the agreement with Ewald, and using an $\alpha$ of 0.2 \AA $^{-1}$
773 + shows an excellent correlation and quality of fit with the SPME
774 + results, particularly with a cutoff radius greater than 12
775 + \AA .  Use of a larger damping parameter is more helpful for the
776 + shortest cutoff shown, but it has a detrimental effect on simulations
777 + with larger cutoffs.  
778 +
779 + In the {\sc sf} sets, increasing damping results in progressively {\it
780 + worse} correlation with Ewald.  Overall, the undamped case is the best
781 + performing set, as the correlation and quality of fits are
782 + consistently superior regardless of the cutoff distance.  The undamped
783 + case is also less computationally demanding (because no evaluation of
784 + the complementary error function is required).
785 +
786 + The reaction field results illustrates some of that method's
787 + limitations, primarily that it was developed for use in homogenous
788 + systems; although it does provide results that are an improvement over
789 + those from an unmodified cutoff.
790 +
791   \subsection{Magnitudes of the Force and Torque Vectors}
792  
793   Evaluation of pairwise methods for use in Molecular Dynamics
794   simulations requires consideration of effects on the forces and
795 < torques.  Investigation of the force and torque vector magnitudes
796 < provides a measure of the strength of these values relative to SPME.
797 < Figures \ref{fig:frcMag} and \ref{fig:trqMag} respectively show the
798 < force and torque vector magnitude regression results for the
558 < accumulated analysis over all the system types.
795 > torques.  Figures \ref{fig:frcMag} and \ref{fig:trqMag} show the
796 > regression results for the force and torque vector magnitudes,
797 > respectively.  The data in these figures was generated from an
798 > accumulation of the statistics from all of 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 magnitudes for a given electrostatic method compared with the reference Ewald sum.  Results with a value equal to 1 (dashed line) indicate force magnitude values indistinguishable from those obtained using SPME.  Different values of the cutoff radius are indicated with different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ = inverted triangles).}
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 + Again, it is striking how well the Shifted Potential and Shifted Force
814 + methods are doing at reproducing the SPME forces.  The undamped and
815 + weakly-damped {\sc sf} method gives the best agreement with Ewald.
816 + This is perhaps expected because this method explicitly incorporates a
817 + smooth transition in the forces at the cutoff radius as well as the
818 + neutralizing image charges.
819 +
820   Figure \ref{fig:frcMag}, for the most part, parallels the results seen
821   in the previous $\Delta E$ section.  The unmodified cutoff results are
822   poor, but using group based cutoffs and a switching function provides
823 < a improvement much more significant than what was seen with $\Delta
824 < E$.  Looking at the Shifted-Potential sets, the slope and $R^2$
825 < improve with the use of damping to an optimal result of 0.2 \AA
826 < $^{-1}$ for the 12 and 15 \AA\ cutoffs.  Further increases in damping,
823 > an improvement much more significant than what was seen with $\Delta
824 > E$.
825 >
826 > With moderate damping and a large enough cutoff radius, the {\sc sp}
827 > method is generating usable forces.  Further increases in damping,
828   while beneficial for simulations with a cutoff radius of 9 \AA\ , is
829 < detrimental to simulations with larger cutoff radii.  The undamped
830 < Shifted-Force method gives forces in line with those obtained using
831 < SPME, and use of a damping function results in minor improvement.  The
578 < reaction field results are surprisingly good, considering the poor
829 > detrimental to simulations with larger cutoff radii.
830 >
831 > The reaction field results are surprisingly good, considering the poor
832   quality of the fits for the $\Delta E$ results.  There is still a
833 < considerable degree of scatter in the data, but it correlates well in
834 < general.  To be fair, we again note that the reaction field
835 < calculations do not encompass NaCl crystal and melt systems, so these
833 > considerable degree of scatter in the data, but the forces correlate
834 > well with the Ewald forces in general.  We note that the reaction
835 > field calculations do not include the pure NaCl systems, so these
836   results are partly biased towards conditions in which the method
837   performs more favorably.
838  
839   \begin{figure}
840   \centering
841   \includegraphics[width=5.5in]{./trqMagplot.pdf}
842 < \caption{Statistical analysis of the quality of the torque vector magnitudes for a given electrostatic method compared with the reference Ewald sum.  Results with a value equal to 1 (dashed line) indicate torque magnitude values indistinguishable from those obtained using SPME.  Different values of the cutoff radius are indicated with different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ = inverted triangles).}
842 > \caption{Statistical analysis of the quality of the torque vector
843 > magnitudes for a given electrostatic method compared with the
844 > reference Ewald sum.  Results with a value equal to 1 (dashed line)
845 > indicate torque magnitude values indistinguishable from those obtained
846 > using SPME.  Different values of the cutoff radius are indicated with
847 > different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ =
848 > inverted triangles).}
849   \label{fig:trqMag}
850   \end{figure}
851  
852 < To evaluate the torque vector magnitudes, the data set from which
853 < values are drawn is limited to rigid molecules in the systems
854 < (i.e. water molecules).  In spite of this smaller sampling pool, the
596 < torque vector magnitude results in figure \ref{fig:trqMag} are still
597 < similar to those seen for the forces; however, they more clearly show
598 < the improved behavior that comes with increasing the cutoff radius.
599 < Moderate damping is beneficial to the Shifted-Potential and helpful
600 < yet possibly unnecessary with the Shifted-Force method, and they also
601 < show that over-damping adversely effects all cutoff radii rather than
602 < showing an improvement for systems with short cutoffs.  The reaction
603 < field method performs well when calculating the torques, better than
604 < the Shifted Force method over this limited data set.
852 > Molecular torques were only available from the systems which contained
853 > rigid molecules (i.e. the systems containing water).  The data in
854 > fig. \ref{fig:trqMag} is taken from this smaller sampling pool.
855  
856 + Torques appear to be much more sensitive to charges at a longer
857 + distance.   The striking feature in comparing the new electrostatic
858 + methods with SPME is how much the agreement improves with increasing
859 + cutoff radius.  Again, the weakly damped and undamped {\sc sf} method
860 + appears to be reproducing the SPME torques most accurately.  
861 +
862 + Water molecules are dipolar, and the reaction field method reproduces
863 + the effect of the surrounding polarized medium on each of the
864 + molecular bodies. Therefore it is not surprising that reaction field
865 + performs best of all of the methods on molecular torques.
866 +
867   \subsection{Directionality of the Force and Torque Vectors}
868  
869 < Having force and torque vectors with magnitudes that are well
870 < correlated to SPME is good, but if they are not pointing in the proper
871 < direction the results will be incorrect.  These vector directions were
872 < investigated through measurement of the angle formed between them and
873 < those from SPME.  The results (Fig. \ref{fig:frcTrqAng}) are compared
874 < through the variance ($\sigma^2$) of the Gaussian fits of the angle
875 < error distributions of the combined set over all system types.
869 > It is clearly important that a new electrostatic method can reproduce
870 > the magnitudes of the force and torque vectors obtained via the Ewald
871 > sum. However, the {\it directionality} of these vectors will also be
872 > vital in calculating dynamical quantities accurately.  Force and
873 > torque directionalities were investigated by measuring the angles
874 > formed between these vectors and the same vectors calculated using
875 > SPME.  The results (Fig. \ref{fig:frcTrqAng}) are compared through the
876 > variance ($\sigma^2$) of the Gaussian fits of the angle error
877 > distributions of the combined set over all system types.
878  
879   \begin{figure}
880   \centering
881   \includegraphics[width=5.5in]{./frcTrqAngplot.pdf}
882 < \caption{Statistical analysis of the quality of the Gaussian fit of the force and torque vector angular distributions for a given electrostatic method compared with the reference Ewald sum.  Results with a variance ($\sigma^2$) equal to zero (dashed line) indicate force and torque directions indistinguishable from those obtained using SPME.  Different values of the cutoff radius are indicated with different symbols (9\AA\ = circles, 12\AA\ = squares, and 15\AA\ = inverted triangles).}
882 > \caption{Statistical analysis of the width of the angular distribution
883 > that the force and torque vectors from a given electrostatic method
884 > make with their counterparts obtained using the reference Ewald sum.
885 > Results with a variance ($\sigma^2$) equal to zero (dashed line)
886 > indicate force and torque directions indistinguishable from those
887 > obtained using SPME.  Different values of the cutoff radius are
888 > indicated with different symbols (9\AA\ = circles, 12\AA\ = squares,
889 > and 15\AA\ = inverted triangles).}
890   \label{fig:frcTrqAng}
891   \end{figure}
892  
893   Both the force and torque $\sigma^2$ results from the analysis of the
894   total accumulated system data are tabulated in figure
895 < \ref{fig:frcTrqAng}.  All of the sets, aside from the over-damped case
896 < show the improvement afforded by choosing a longer simulation cutoff.
897 < Increasing the cutoff from 9 to 12 \AA\ typically results in a halving
898 < of the distribution widths, with a similar improvement going from 12
899 < to 15 \AA .  The undamped Shifted-Force, Group Based Cutoff, and
630 < Reaction Field methods all do equivalently well at capturing the
631 < direction of both the force and torque vectors.  Using damping
632 < improves the angular behavior significantly for the Shifted-Potential
633 < and moderately for the Shifted-Force methods.  Increasing the damping
634 < too far is destructive for both methods, particularly to the torque
635 < vectors.  Again it is important to recognize that the force vectors
636 < cover all particles in the systems, while torque vectors are only
637 < available for neutral molecular groups.  Damping appears to have a
638 < more beneficial effect on non-neutral bodies, and this observation is
639 < investigated further in the accompanying supporting information.
895 > \ref{fig:frcTrqAng}. Here it is clear that the Shifted Potential ({\sc
896 > sp}) method would be essentially unusable for molecular dynamics until
897 > the damping function is added.  The Shifted Force ({\sc sf}) method,
898 > however, is generating force and torque vectors which are within a few
899 > degrees of the Ewald results even with weak (or no) damping.
900  
901 + All of the sets (aside from the over-damped case) show the improvement
902 + afforded by choosing a larger cutoff radius.  Increasing the cutoff
903 + from 9 to 12 \AA\ typically results in a halving of the width of the
904 + distribution, with a similar improvement going from 12 to 15
905 + \AA .
906 +
907 + The undamped {\sc sf}, group-based cutoff, and reaction field methods
908 + all do equivalently well at capturing the direction of both the force
909 + and torque vectors.  Using damping improves the angular behavior
910 + significantly for the {\sc sp} and moderately for the {\sc sf}
911 + methods.  Overdamping is detrimental to both methods.  Again it is
912 + important to recognize that the force vectors cover all particles in
913 + the systems, while torque vectors are only available for neutral
914 + molecular groups.  Damping appears to have a more beneficial effect on
915 + charged bodies, and this observation is investigated further in the
916 + accompanying supporting information.
917 +
918 + Although not discussed previously, group based cutoffs can be applied
919 + to both the {\sc sp} and {\sc sf} methods.  Use of a switching
920 + function corrects for the discontinuities that arise when atoms of the
921 + two groups exit the cutoff radius before the group centers leave each
922 + other's cutoff. Though there are no significant benefits or drawbacks
923 + observed in $\Delta E$ and vector magnitude results when doing this,
924 + there is a measurable improvement in the vector angle results.  Table
925 + \ref{tab:groupAngle} shows the angular variance values obtained using
926 + group based cutoffs and a switching function alongside the results
927 + seen in figure \ref{fig:frcTrqAng}.  The {\sc sp} shows much narrower
928 + angular distributions for both the force and torque vectors when using
929 + an $\alpha$ of 0.2 \AA$^{-1}$ or less, while {\sc sf} shows
930 + improvements in the undamped and lightly damped cases.  Thus, by
931 + calculating the electrostatic interactions in terms of molecular pairs
932 + rather than atomic pairs, the direction of the force and torque
933 + vectors can be determined more accurately.
934 +
935   \begin{table}[htbp]
936     \centering
937 <   \caption{Variance ($\sigma^2$) of the force (top set) and torque (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$^2$.}  
937 >   \caption{Variance ($\sigma^2$) of the force (top set) and torque
938 > (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$^2$.}      
939     \begin{tabular}{@{} ccrrrrrrrr @{}}
940        \\
941        \toprule
# Line 671 | Line 966 | investigated further in the accompanying supporting in
966     \label{tab:groupAngle}
967   \end{table}
968  
674 Although not discussed previously, group based cutoffs can be applied
675 to both the Shifted-Potential and Shifted-Force methods.  Use off a
676 switching function corrects for the discontinuities that arise when
677 atoms of a group exit the cutoff before the group's center of mass.
678 Though there are no significant benefit or drawbacks observed in
679 $\Delta E$ and vector magnitude results when doing this, there is a
680 measurable improvement in the vector angle results.  Table
681 \ref{tab:groupAngle} shows the angular variance values obtained using
682 group based cutoffs and a switching function alongside the standard
683 results seen in figure \ref{fig:frcTrqAng} for comparison purposes.
684 The Shifted-Potential shows much narrower angular distributions for
685 both the force and torque vectors when using an $\alpha$ of 0.2
686 \AA$^{-1}$ or less, while Shifted-Force shows improvements in the
687 undamped and lightly damped cases.  Thus, by calculating the
688 electrostatic interactions in terms of molecular pairs rather than
689 atomic pairs, the direction of the force and torque vectors are
690 determined more accurately.
691
969   One additional trend to recognize in table \ref{tab:groupAngle} is
970 < that the $\sigma^2$ values for both Shifted-Potential and
971 < Shifted-Force converge as $\alpha$ increases, something that is easier
972 < to see when using group based cutoffs.  Looking back on figures
973 < \ref{fig:delE}, \ref{fig:frcMag}, and \ref{fig:trqMag}, show this
974 < behavior clearly at large $\alpha$ and cutoff values.  The reason for
975 < this is that the complimentary error function inserted into the
976 < potential weakens the electrostatic interaction as $\alpha$ increases.
977 < Thus, at larger values of $\alpha$, both the summation method types
978 < progress toward non-interacting functions, so care is required in
979 < choosing large damping functions lest one generate an undesirable loss
980 < in the pair interaction.  Kast \textit{et al.}  developed a method for
981 < choosing appropriate $\alpha$ values for these types of electrostatic
982 < summation methods by fitting to $g(r)$ data, and their methods
983 < indicate optimal values of 0.34, 0.25, and 0.16 \AA$^{-1}$ for cutoff
984 < values of 9, 12, and 15 \AA\ respectively.\cite{Kast03} These appear
985 < to be reasonable choices to obtain proper MC behavior
986 < (Fig. \ref{fig:delE}); however, based on these findings, choices this
987 < high would introduce error in the molecular torques, particularly for
988 < the shorter cutoffs.  Based on the above findings, empirical damping
712 < up to 0.2 \AA$^{-1}$ proves to be beneficial, but damping is arguably
713 < unnecessary when using the Shifted-Force method.
970 > that the $\sigma^2$ values for both {\sc sp} and {\sc sf} converge as
971 > $\alpha$ increases, something that is easier to see when using group
972 > based cutoffs.  The reason for this is that the complimentary error
973 > function inserted into the potential weakens the electrostatic
974 > interaction as $\alpha$ increases.  Thus, at larger values of
975 > $\alpha$, both summation methods progress toward non-interacting
976 > functions, so care is required in choosing large damping functions
977 > lest one generate an undesirable loss in the pair interaction.  Kast
978 > \textit{et al.}  developed a method for choosing appropriate $\alpha$
979 > values for these types of electrostatic summation methods by fitting
980 > to $g(r)$ data, and their methods indicate optimal values of 0.34,
981 > 0.25, and 0.16 \AA$^{-1}$ for cutoff values of 9, 12, and 15 \AA\
982 > respectively.\cite{Kast03} These appear to be reasonable choices to
983 > obtain proper MC behavior (Fig. \ref{fig:delE}); however, based on
984 > these findings, choices this high would introduce error in the
985 > molecular torques, particularly for the shorter cutoffs.  Based on the
986 > above findings, empirical damping up to 0.2 \AA$^{-1}$ proves to be
987 > beneficial, but damping may be unnecessary when using the {\sc sf}
988 > method.
989  
990 + \subsection{Short-Time Dynamics: Velocity Autocorrelation Functions of NaCl Crystals}
991 +
992 + Zahn {\it et al.} investigated the structure and dynamics of water
993 + using eqs. (\ref{eq:ZahnPot}) and
994 + (\ref{eq:WolfForces}).\cite{Zahn02,Kast03} Their results indicated
995 + that a method similar (but not identical with) the damped {\sc sf}
996 + method resulted in properties very similar to those obtained when
997 + using the Ewald summation.  The properties they studied (pair
998 + distribution functions, diffusion constants, and velocity and
999 + orientational correlation functions) may not be particularly sensitive
1000 + to the long-range and collective behavior that governs the
1001 + low-frequency behavior in crystalline systems.
1002 +
1003 + We are using two separate measures to probe the effects of these
1004 + alternative electrostatic methods on the dynamics in crystalline
1005 + materials.  For short- and intermediate-time dynamics, we are
1006 + computing the velocity autocorrelation function, and for long-time
1007 + and large length-scale collective motions, we are looking at the
1008 + low-frequency portion of the power spectrum.
1009 +
1010 + \begin{figure}
1011 + \centering
1012 + \includegraphics[width = \linewidth]{./vCorrPlot.pdf}
1013 + \caption{Velocity auto-correlation functions of NaCl crystals at
1014 + 1000 K using SPME, {\sc sf} ($\alpha$ = 0.0, 0.1, \& 0.2), and {\sc
1015 + sp} ($\alpha$ = 0.2). The inset is a magnification of the area around
1016 + the first minimum.  The times to first collision are nearly identical,
1017 + but differences can be seen in the peaks and troughs, where the
1018 + undamped and weakly damped methods are stiffer than the moderately
1019 + damped and SPME methods.}
1020 + \label{fig:vCorrPlot}
1021 + \end{figure}
1022 +
1023 + The short-time decays through the first collision are nearly identical
1024 + in figure \ref{fig:vCorrPlot}, but the peaks and troughs of the
1025 + functions show how the methods differ.  The undamped {\sc sf} method
1026 + has deeper troughs (see inset in Fig. \ref{fig:vCorrPlot}) and higher
1027 + peaks than any of the other methods.  As the damping function is
1028 + increased, these peaks are smoothed out, and approach the SPME
1029 + curve. The damping acts as a distance dependent Gaussian screening of
1030 + the point charges for the pairwise summation methods; thus, the
1031 + collisions are more elastic in the undamped {\sc sf} potential, and the
1032 + stiffness of the potential is diminished as the electrostatic
1033 + interactions are softened by the damping function.  With $\alpha$
1034 + values of 0.2 \AA$^{-1}$, the {\sc sf} and {\sc sp} functions are
1035 + nearly identical and track the SPME features quite well.  This is not
1036 + too surprising in that the differences between the {\sc sf} and {\sc
1037 + sp} potentials are mitigated with increased damping.  However, this
1038 + appears to indicate that once damping is utilized, the form of the
1039 + potential seems to play a lesser role in the crystal dynamics.
1040 +
1041   \subsection{Collective Motion: Power Spectra of NaCl Crystals}
1042  
1043 < In the previous studies using a Shifted-Force variant of the damped
1044 < Wolf coulomb potential, the structure and dynamics of water were
1045 < investigated rather extensively.\cite{Zahn02,Kast03} Their results
1046 < indicated that the damped Shifted-Force method results in properties
1047 < very similar to those obtained when using the Ewald summation.
1048 < Considering the statistical results shown above, the good performance
1049 < of this method is not that surprising.  Rather than consider the same
724 < systems and simply recapitulate their results, we decided to look at
725 < the solid state dynamical behavior obtained using the best performing
726 < summation methods from the above results.
1043 > The short time dynamics were extended to evaluate how the differences
1044 > between the methods affect the collective long-time motion.  The same
1045 > electrostatic summation methods were used as in the short time
1046 > velocity autocorrelation function evaluation, but the trajectories
1047 > were sampled over a much longer time. The power spectra of the
1048 > resulting velocity autocorrelation functions were calculated and are
1049 > displayed in figure \ref{fig:methodPS}.
1050  
1051   \begin{figure}
1052   \centering
1053   \includegraphics[width = \linewidth]{./spectraSquare.pdf}
1054 < \caption{Power spectra obtained from the velocity auto-correlation functions of NaCl crystals at 1000 K while using SPME, Shifted-Force ($\alpha$ = 0, 0.1, \& 0.2), and Shifted-Potential ($\alpha$ = 0.2).  Apodization of the correlation functions via a cubic switching function between 40 and 50 ps was used to clear up the spectral noise resulting from data truncation, and had no noticeable effect on peak location or magnitude.  The inset shows the frequency region below 100 cm$^{-1}$ to highlight where the spectra begin to differ.}
1054 > \caption{Power spectra obtained from the velocity auto-correlation
1055 > functions of NaCl crystals at 1000 K while using SPME, {\sc sf}
1056 > ($\alpha$ = 0, 0.1, \& 0.2), and {\sc sp} ($\alpha$ = 0.2).
1057 > Apodization of the correlation functions via a cubic switching
1058 > function between 40 and 50 ps was used to clear up the spectral noise
1059 > resulting from data truncation, and had no noticeable effect on peak
1060 > location or magnitude.  The inset shows the frequency region below 100
1061 > cm$^{-1}$ to highlight where the spectra begin to differ.}
1062   \label{fig:methodPS}
1063   \end{figure}
1064  
1065 < Figure \ref{fig:methodPS} shows the power spectra for the NaCl
1066 < crystals (from averaged Na and Cl ion velocity autocorrelation
1067 < functions) using the stated electrostatic summation methods.  While
1068 < high frequency peaks of all the spectra overlap, showing the same
1069 < general features, the low frequency region shows how the summation
1070 < methods differ.  Considering the low-frequency inset (expanded in the
1071 < upper frame of figure \ref{fig:dampInc}), at frequencies below 100
1072 < cm$^{-1}$, the correlated motions are blue-shifted when using undamped
1073 < or weakly damped Shifted-Force.  When using moderate damping ($\alpha
1074 < = 0.2$ \AA$^{-1}$) both the Shifted-Force and Shifted-Potential
1075 < methods give near identical correlated motion behavior as the Ewald
1076 < method (which has a damping value of 0.3119).  The damping acts as a
1077 < distance dependent Gaussian screening of the point charges for the
1078 < pairwise summation methods.  This weakening of the electrostatic
1079 < interaction with distance explains why the long-ranged correlated
750 < motions are at lower frequencies for the moderately damped methods
751 < than for undamped or weakly damped methods.  To see this effect more
752 < clearly, we show how damping strength affects a simple real-space
753 < electrostatic potential,
1065 > While high frequency peaks of the spectra in this figure overlap,
1066 > showing the same general features, the low frequency region shows how
1067 > the summation methods differ.  Considering the low-frequency inset
1068 > (expanded in the upper frame of figure \ref{fig:dampInc}), at
1069 > frequencies below 100 cm$^{-1}$, the correlated motions are
1070 > blue-shifted when using undamped or weakly damped {\sc sf}.  When
1071 > using moderate damping ($\alpha = 0.2$ \AA$^{-1}$) both the {\sc sf}
1072 > and {\sc sp} methods give near identical correlated motion behavior as
1073 > the Ewald method (which has a damping value of 0.3119).  This
1074 > weakening of the electrostatic interaction with increased damping
1075 > explains why the long-ranged correlated motions are at lower
1076 > frequencies for the moderately damped methods than for undamped or
1077 > weakly damped methods.  To see this effect more clearly, we show how
1078 > damping strength alone affects a simple real-space electrostatic
1079 > potential,
1080   \begin{equation}
1081 < V_\textrm{damped}=\sum^N_i\sum^N_{j\ne i}q_iq_j\left[\frac{\textrm{erfc}({\alpha r_{ij}})}{r_{ij}}\right]S(r),
1081 > V_\textrm{damped}=\sum^N_i\sum^N_{j\ne i}q_iq_j\left[\frac{\textrm{erfc}({\alpha r})}{r}\right]S(r),
1082   \end{equation}
1083   where $S(r)$ is a switching function that smoothly zeroes the
1084   potential at the cutoff radius.  Figure \ref{fig:dampInc} shows how
# Line 765 | Line 1091 | blue-shifted such that the lowest frequency peak resid
1091   shift to higher frequency in exponential fashion.  Though not shown,
1092   the spectrum for the simple undamped electrostatic potential is
1093   blue-shifted such that the lowest frequency peak resides near 325
1094 < cm$^{-1}$.  In light of these results, the undamped Shifted-Force
1095 < method producing low-lying motion peaks within 10 cm$^{-1}$ of SPME is
1096 < quite respectable; however, it appears as though moderate damping is
1097 < required for accurate reproduction of crystal dynamics.
1094 > cm$^{-1}$.  In light of these results, the undamped {\sc sf} method
1095 > producing low-lying motion peaks within 10 cm$^{-1}$ of SPME is quite
1096 > respectable and shows that the shifted force procedure accounts for
1097 > most of the effect afforded through use of the Ewald summation.
1098 > However, it appears as though moderate damping is required for
1099 > accurate reproduction of crystal dynamics.
1100   \begin{figure}
1101   \centering
1102   \includegraphics[width = \linewidth]{./comboSquare.pdf}
1103 < \caption{Upper: Zoomed inset from figure \ref{fig:methodPS}.  As the damping value for the Shifted-Force potential increases, the low-frequency peaks red-shift.  Lower: Low-frequency correlated motions for NaCl crystals at 1000 K when using SPME and a simple damped Coulombic sum with damping coefficients ($\alpha$) ranging from 0.15 to 0.3 \AA$^{-1}$.  As $\alpha$ increases, the peaks are red-shifted toward and eventually beyond the values given by SPME.  The larger $\alpha$ values weaken the real-space electrostatics, explaining this shift towards less strongly correlated motions in the crystal.}
1103 > \caption{Regions of spectra showing the low-frequency correlated
1104 > motions for NaCl crystals at 1000 K using various electrostatic
1105 > summation methods.  The upper plot is a zoomed inset from figure
1106 > \ref{fig:methodPS}.  As the damping value for the {\sc sf} potential
1107 > increases, the low-frequency peaks red-shift.  The lower plot is of
1108 > spectra when using SPME and a simple damped Coulombic sum with damping
1109 > coefficients ($\alpha$) ranging from 0.15 to 0.3 \AA$^{-1}$.  As
1110 > $\alpha$ increases, the peaks are red-shifted toward and eventually
1111 > beyond the values given by SPME.  The larger $\alpha$ values weaken
1112 > the real-space electrostatics, explaining this shift towards less
1113 > strongly correlated motions in the crystal.}
1114   \label{fig:dampInc}
1115   \end{figure}
1116  
# Line 783 | Line 1121 | Wolf \textit{et al.}\cite{Wolf99,Zahn02} In particular
1121   electrostatic summation techniques than the Ewald summation, chiefly
1122   methods derived from the damped Coulombic sum originally proposed by
1123   Wolf \textit{et al.}\cite{Wolf99,Zahn02} In particular, the
1124 < Shifted-Force method, reformulated above as equation \ref{eq:SFPot},
1124 > {\sc sf} method, reformulated above as eq. (\ref{eq:DSFPot}),
1125   shows a remarkable ability to reproduce the energetic and dynamic
1126   characteristics exhibited by simulations employing lattice summation
1127   techniques.  The cumulative energy difference results showed the
1128 < undamped Shifted-Force and moderately damped Shifted-Potential methods
1128 > undamped {\sc sf} and moderately damped {\sc sp} methods
1129   produced results nearly identical to SPME.  Similarly for the dynamic
1130 < features, the undamped or moderately damped Shifted-Force and
1131 < moderately damped Shifted-Potential methods produce force and torque
1130 > features, the undamped or moderately damped {\sc sf} and
1131 > moderately damped {\sc sp} methods produce force and torque
1132   vector magnitude and directions very similar to the expected values.
1133   These results translate into long-time dynamic behavior equivalent to
1134   that produced in simulations using SPME.
# Line 812 | Line 1150 | today, the Ewald summation may no longer be required t
1150   standard by which these simple pairwise sums are judged.  However,
1151   these results do suggest that in the typical simulations performed
1152   today, the Ewald summation may no longer be required to obtain the
1153 < level of accuracy most researcher have come to expect
1153 > level of accuracy most researchers have come to expect
1154  
1155   \section{Acknowledgments}
1156   \newpage

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