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# Line 69 | Line 69 | of Notre Dame, Notre Dame, IN 46556}
69   \begin{abstract}
70    We have tested the real-space shifted potential (SP),
71    gradient-shifted force (GSF), and Taylor-shifted force (TSF) methods
72 <  for multipoles that were developed in the first paper in this series
73 <  against the multipolar Ewald sum as a reference method. The tests
74 <  were carried out in a variety of condensed-phase environments which
75 <  were designed to test all levels of the multipole-multipole
76 <  interactions.  Comparisons of the energy differences between
77 <  configurations, molecular forces, and torques were used to analyze
78 <  how well the real-space models perform relative to the more
79 <  computationally expensive Ewald treatment.  We have also investigated the
80 <  energy conservation properties of the new methods in molecular
81 <  dynamics simulations using all of these methods. The SP method shows
82 <  excellent agreement with configurational energy differences, forces,
83 <  and torques, and would be suitable for use in Monte Carlo
84 <  calculations.  Of the two new shifted-force methods, the GSF
85 <  approach shows the best agreement with Ewald-derived energies,
86 <  forces, and torques and exhibits energy conservation properties that
87 <  make it an excellent choice for efficiently computing electrostatic
88 <  interactions in molecular dynamics simulations.
72 >  for multipole interactions that were developed in the first paper in
73 >  this series, using the multipolar Ewald sum as a reference
74 >  method. The tests were carried out in a variety of condensed-phase
75 >  environments which were designed to test all levels of the
76 >  multipole-multipole interactions.  Comparisons of the energy
77 >  differences between configurations, molecular forces, and torques
78 >  were used to analyze how well the real-space models perform relative
79 >  to the more computationally expensive Ewald treatment.  We have also
80 >  investigated the energy conservation properties of the new methods
81 >  in molecular dynamics simulations. The SP method shows excellent
82 >  agreement with configurational energy differences, forces, and
83 >  torques, and would be suitable for use in Monte Carlo calculations.
84 >  Of the two new shifted-force methods, the GSF approach shows the
85 >  best agreement with Ewald-derived energies, forces, and torques and
86 >  exhibits energy conservation properties that make it an excellent
87 >  choice for efficient computation of electrostatic interactions in
88 >  molecular dynamics simulations.
89   \end{abstract}
90  
91   %\pacs{Valid PACS appear here}% PACS, the Physics and Astronomy
# Line 97 | Line 97 | most expensive aspects of molecular simulations, which
97  
98   \section{\label{sec:intro}Introduction}
99   Computing the interactions between electrostatic sites is one of the
100 < most expensive aspects of molecular simulations, which is why there
101 < have been significant efforts to develop practical, efficient and
102 < convergent methods for handling these interactions. Ewald's method is
103 < perhaps the best known and most accurate method for evaluating
104 < energies, forces, and torques in explicitly-periodic simulation
105 < cells. In this approach, the conditionally convergent electrostatic
106 < energy is converted into two absolutely convergent contributions, one
107 < which is carried out in real space with a cutoff radius, and one in
108 < reciprocal space.\cite{Clarke:1986eu,Woodcock75}
100 > most expensive aspects of molecular simulations. There have been
101 > significant efforts to develop practical, efficient and convergent
102 > methods for handling these interactions. Ewald's method is perhaps the
103 > best known and most accurate method for evaluating energies, forces,
104 > and torques in explicitly-periodic simulation cells. In this approach,
105 > the conditionally convergent electrostatic energy is converted into
106 > two absolutely convergent contributions, one which is carried out in
107 > real space with a cutoff radius, and one in reciprocal
108 > space. BETTER CITATIONS\cite{Clarke:1986eu,Woodcock75}
109  
110   When carried out as originally formulated, the reciprocal-space
111   portion of the Ewald sum exhibits relatively poor computational
# Line 116 | Line 116 | Because of the artificial periodicity required for the
116   the computational cost from $O(N^2)$ down to $O(N \log
117   N)$.\cite{Takada93,Gunsteren94,Gunsteren95,Darden:1993pd,Essmann:1995pb}.
118  
119 < Because of the artificial periodicity required for the Ewald sum, the
120 < method may require modification to compute interactions for
119 > Because of the artificial periodicity required for the Ewald sum,
120   interfacial molecular systems such as membranes and liquid-vapor
121 < interfaces.\cite{Parry:1975if,Parry:1976fq,Clarke77,Perram79,Rhee:1989kl}
122 < To simulate interfacial systems, Parry's extension of the 3D Ewald sum
123 < is appropriate for slab geometries.\cite{Parry:1975if} The inherent
124 < periodicity in the Ewald method can also be problematic for molecular
125 < interfaces.\cite{Fennell:2006lq} Modified Ewald methods that were
126 < developed to handle two-dimensional (2D) electrostatic interactions in
127 < interfacial systems have not seen similar particle-mesh
129 < treatments,\cite{Parry:1975if, Parry:1976fq, Clarke77,
121 > interfaces require modifications to the
122 > method.\cite{Parry:1975if,Parry:1976fq,Clarke77,Perram79,Rhee:1989kl}
123 > Parry's extension of the three dimensional Ewald sum is appropriate
124 > for slab geometries.\cite{Parry:1975if} Modified Ewald methods that
125 > were developed to handle two-dimensional (2D) electrostatic
126 > interactions in interfacial systems have not seen similar
127 > particle-mesh treatments,\cite{Parry:1975if, Parry:1976fq, Clarke77,
128    Perram79,Rhee:1989kl,Spohr:1997sf,Yeh:1999oq} and still scale poorly
129 < with system size.
129 > with system size. The inherent periodicity in the Ewald’s method can
130 > also be problematic for interfacial molecular
131 > systems.\cite{Fennell:2006lq}
132  
133   \subsection{Real-space methods}
134   Wolf \textit{et al.}\cite{Wolf:1999dn} proposed a real space $O(N)$
135   method for calculating electrostatic interactions between point
136 < charges. They argued that the effective Coulomb interaction in
137 < condensed phase systems is actually short ranged.\cite{Wolf92,Wolf95}
138 < For an ordered lattice (e.g., when computing the Madelung constant of
139 < an ionic solid), the material can be considered as a set of ions
140 < interacting with neutral dipolar or quadrupolar ``molecules'' giving
141 < an effective distance dependence for the electrostatic interactions of
142 < $r^{-5}$ (see figure \ref{fig:schematic}).  For this reason, careful
143 < application of Wolf's method can obtain accurate estimates of Madelung
144 < constants using relatively short cutoff radii.  Recently, Fukuda used
145 < neutralization of the higher order moments for calculation of the
146 < electrostatic interactions in point charge
136 > charges. They argued that the effective Coulomb interaction in most
137 > condensed phase systems is effectively short
138 > ranged.\cite{Wolf92,Wolf95} For an ordered lattice (e.g., when
139 > computing the Madelung constant of an ionic solid), the material can
140 > be considered as a set of ions interacting with neutral dipolar or
141 > quadrupolar ``molecules'' giving an effective distance dependence for
142 > the electrostatic interactions of $r^{-5}$ (see figure
143 > \ref{fig:schematic}). If one views the \ce{NaCl} crystal as a simple
144 > cubic (SC) structure with an octupolar \ce{(NaCl)4} basis, the
145 > electrostatic energy per ion converges more rapidly to the Madelung
146 > energy than the dipolar approximation.\cite{Wolf92} To find the
147 > correct Madelung constant, Lacman suggested that the NaCl structure
148 > could be constructed in a way that the finite crystal terminates with
149 > complete \ce{(NaCl)4} molecules.\cite{Lacman65} The central ion sees
150 > what is effectively a set of octupoles at large distances. These facts
151 > suggest that the Madelung constants are relatively short ranged for
152 > perfect ionic crystals.\cite{Wolf:1999dn} For this reason, careful
153 > application of Wolf's method are able to obtain accurate estimates of
154 > Madelung constants using relatively short cutoff radii.
155 >
156 > Direct truncation of interactions at a cutoff radius creates numerical
157 > errors.  Wolf \textit{et al.}  argued that truncation errors are due
158 > to net charge remaining inside the cutoff sphere.\cite{Wolf:1999dn} To
159 > neutralize this charge they proposed placing an image charge on the
160 > surface of the cutoff sphere for every real charge inside the cutoff.
161 > These charges are present for the evaluation of both the pair
162 > interaction energy and the force, although the force expression
163 > maintained a discontinuity at the cutoff sphere.  In the original Wolf
164 > formulation, the total energy for the charge and image were not equal
165 > to the integral of their force expression, and as a result, the total
166 > energy would not be conserved in molecular dynamics (MD)
167 > simulations.\cite{Zahn:2002hc} Zahn \textit{et al.}, and Fennel and
168 > Gezelter later proposed shifted force variants of the Wolf method with
169 > commensurate force and energy expressions that do not exhibit this
170 > problem.\cite{Fennell:2006lq} Related real-space methods were also
171 > proposed by Chen \textit{et
172 >  al.}\cite{Chen:2004du,Chen:2006ii,Denesyuk:2008ez,Rodgers:2006nw}
173 > and by Wu and Brooks.\cite{Wu:044107} Recently, Fukuda has used
174 > neutralization of the higher order moments for the calculation of the
175 > electrostatic interaction of the point charge
176   systems.\cite{Fukuda:2013sf}
177  
178   \begin{figure}
# Line 163 | Line 192 | The direct truncation of interactions at a cutoff radi
192    \label{fig:schematic}
193   \end{figure}
194  
195 < The direct truncation of interactions at a cutoff radius creates
196 < truncation defects. Wolf \textit{et al.}  argued that
197 < truncation errors are due to net charge remaining inside the cutoff
198 < sphere.\cite{Wolf:1999dn} To neutralize this charge they proposed
199 < placing an image charge on the surface of the cutoff sphere for every
200 < real charge inside the cutoff.  These charges are present for the
201 < evaluation of both the pair interaction energy and the force, although
202 < the force expression maintained a discontinuity at the cutoff sphere.
203 < In the original Wolf formulation, the total energy for the charge and
204 < image were not equal to the integral of their force expression, and as
176 < a result, the total energy would not be conserved in molecular
177 < dynamics (MD) simulations.\cite{Zahn:2002hc} Zahn \textit{et al.} and
178 < Fennel and Gezelter later proposed shifted force variants of the Wolf
179 < method with commensurate force and energy expressions that do not
180 < exhibit this problem.\cite{Fennell:2006lq}   Related real-space
181 < methods were also proposed by Chen \textit{et
182 <  al.}\cite{Chen:2004du,Chen:2006ii,Denesyuk:2008ez,Rodgers:2006nw}
183 < and by Wu and Brooks.\cite{Wu:044107}
184 <
185 < Considering the interaction of one central ion in an ionic crystal
186 < with a portion of the crystal at some distance, the effective Columbic
187 < potential is found to decrease as $r^{-5}$. If one views the \ce{NaCl}
188 < crystal as a simple cubic (SC) structure with an octupolar
189 < \ce{(NaCl)4} basis, the electrostatic energy per ion converges more
190 < rapidly to the Madelung energy than the dipolar
191 < approximation.\cite{Wolf92} To find the correct Madelung constant,
192 < Lacman suggested that the NaCl structure could be constructed in a way
193 < that the finite crystal terminates with complete \ce{(NaCl)4}
194 < molecules.\cite{Lacman65} The central ion sees what is effectively a
195 < set of octupoles at large distances. These facts suggest that the
196 < Madelung constants are relatively short ranged for perfect ionic
197 < crystals.\cite{Wolf:1999dn}
198 <
199 < One can make a similar argument for crystals of point multipoles. The
200 < Luttinger and Tisza treatment of energy constants for dipolar lattices
201 < utilizes 24 basis vectors that contain dipoles at the eight corners of
202 < a unit cube.  Only three of these basis vectors, $X_1, Y_1,
203 < \mathrm{~and~} Z_1,$ retain net dipole moments, while the rest have
204 < zero net dipole and retain contributions only from higher order
205 < multipoles.  The effective interaction between a dipole at the center
195 > One can make a similar effective range argument for crystals of point
196 > \textit{multipoles}. The Luttinger and Tisza treatment of energy
197 > constants for dipolar lattices utilizes 24 basis vectors that contain
198 > dipoles at the eight corners of a unit cube.  Only three of these
199 > basis vectors, $X_1, Y_1, \mathrm{~and~} Z_1,$ retain net dipole
200 > moments, while the rest have zero net dipole and retain contributions
201 > only from higher order multipoles.  The lowest energy crystalline
202 > structures are built out of basis vectors that have only residual
203 > quadrupolar moments (e.g. the $Z_5$ array). In these low energy
204 > structures, the effective interaction between a dipole at the center
205   of a crystal and a group of eight dipoles farther away is
206   significantly shorter ranged than the $r^{-3}$ that one would expect
207   for raw dipole-dipole interactions.  Only in crystals which retain a
# Line 259 | Line 258 | The damping function used in our research has been dis
258   densities.\cite{Shi:2013ij,Kannam:2012rr,Acevedo13,Space12,English08,Lawrence13,Vergne13}
259  
260   \subsection{The damping function}
261 < The damping function used in our research has been discussed in detail
262 < in the first paper of this series.\cite{PaperI} The radial kernel
263 < $1/r$ for the interactions between point charges can be replaced by
264 < the complementary error function $\mathrm{erfc}(\alpha r)/r$ to
265 < accelerate the rate of convergence, where $\alpha$ is a damping
266 < parameter with units of inverse distance.  Altering the value of
267 < $\alpha$ is equivalent to changing the width of Gaussian charge
268 < distributions that replace each point charge -- Gaussian overlap
269 < integrals yield complementary error functions when truncated at a
270 < finite distance.
261 > The damping function has been discussed in detail in the first paper
262 > of this series.\cite{PaperI} The $1/r$ Coulombic kernel for the
263 > interactions between point charges can be replaced by the
264 > complementary error function $\mathrm{erfc}(\alpha r)/r$ to accelerate
265 > convergence, where $\alpha$ is a damping parameter with units of
266 > inverse distance.  Altering the value of $\alpha$ is equivalent to
267 > changing the width of Gaussian charge distributions that replace each
268 > point charge, as Coulomb integrals with Gaussian charge distributions
269 > produce complementary error functions when truncated at a finite
270 > distance.
271  
272 < By using suitable value of damping alpha ($\alpha \sim 0.2$) for a
273 < cutoff radius ($r_{­c}=9 A$), Fennel and Gezelter produced very good
274 < agreement with SPME for the interaction energies, forces and torques
275 < for charge-charge interactions.\cite{Fennell:2006lq}
272 > With moderate damping coefficients, $\alpha \sim 0.2$, the DSF method
273 > produced very good agreement with SPME for interaction energies,
274 > forces and torques for charge-charge
275 > interactions.\cite{Fennell:2006lq}
276  
277   \subsection{Point multipoles in molecular modeling}
278   Coarse-graining approaches which treat entire molecular subsystems as
279   a single rigid body are now widely used. A common feature of many
280   coarse-graining approaches is simplification of the electrostatic
281   interactions between bodies so that fewer site-site interactions are
282 < required to compute configurational energies.  Many coarse-grained
283 < molecular structures would normally consist of equal positive and
285 < negative charges, and rather than use multiple site-site interactions,
286 < the interaction between higher order multipoles can also be used to
287 < evaluate a single molecule-molecule
288 < interaction.\cite{Ren06,Essex10,Essex11}
282 > required to compute configurational
283 > energies.\cite{Ren06,Essex10,Essex11}
284  
285   Because electrons in a molecule are not localized at specific points,
286 < the assignment of partial charges to atomic centers is a relatively
287 < rough approximation.  Atomic sites can also be assigned point
288 < multipoles and polarizabilities to increase the accuracy of the
289 < molecular model.  Recently, water has been modeled with point
290 < multipoles up to octupolar order using the soft sticky
296 < dipole-quadrupole-octupole (SSDQO)
286 > the assignment of partial charges to atomic centers is always an
287 > approximation.  Atomic sites can also be assigned point multipoles and
288 > polarizabilities to increase the accuracy of the molecular model.
289 > Recently, water has been modeled with point multipoles up to octupolar
290 > order using the soft sticky dipole-quadrupole-octupole (SSDQO)
291   model.\cite{Ichiye10_1,Ichiye10_2,Ichiye10_3} Atom-centered point
292   multipoles up to quadrupolar order have also been coupled with point
293   polarizabilities in the high-quality AMOEBA and iAMOEBA water
294 < models.\cite{Ren:2003uq,Ren:2004kx,Ponder:2010vl,Wang:2013fk} But
295 < using point multipole with the real space truncation without
296 < accounting for multipolar neutrality will create energy conservation
303 < issues in molecular dynamics (MD) simulations.
294 > models.\cite{Ren:2003uq,Ren:2004kx,Ponder:2010vl,Wang:2013fk} However,
295 > truncating point multipoles without smoothing the forces and torques
296 > will create energy conservation issues in molecular dynamics simulations.
297  
298   In this paper we test a set of real-space methods that were developed
299   for point multipolar interactions.  These methods extend the damped

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