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# Line 20 | Line 20
20  
21   \begin{document}
22  
23 < \title{Ice-{\it i}: a simulation-predicted ice polymorph which is more
24 < stable than Ice $I_h$ for point-charge and point-dipole water models}
23 > \title{Free Energy Analysis of Simulated Ice Polymorphs Using Simple
24 > Dipolar and Charge Based Water Models}
25  
26   \author{Christopher J. Fennell and J. Daniel Gezelter \\
27   Department of Chemistry and Biochemistry\\ University of Notre Dame\\
# Line 84 | Line 84 | constant pressure and temperature conditions. Crystall
84   crystalline water polymorphs in the low pressure regime.  This work is
85   unique in that one of the crystal lattices was arrived at through
86   crystallization of a computationally efficient water model under
87 < constant pressure and temperature conditions. Crystallization events
87 > constant pressure and temperature conditions.  Crystallization events
88   are interesting in and of themselves;\cite{Matsumoto02,Yamada02}
89   however, the crystal structure obtained in this case is different from
90   any previously observed ice polymorphs in experiment or
91   simulation.\cite{Fennell04} We have named this structure Ice-{\it i}
92   to indicate its origin in computational simulation. The unit cell
93   (Fig. \ref{iceiCell}A) consists of eight water molecules that stack in
94 < rows of interlocking water tetramers. Proton ordering can be
94 > rows of interlocking water tetramers.  This crystal structure has a
95 > limited resemblence to a recent two-dimensional ice tessellation
96 > simulated on a silica surface.\cite{Yang04} Proton ordering can be
97   accomplished by orienting two of the molecules so that both of their
98   donated hydrogen bonds are internal to their tetramer
99 < (Fig. \ref{protOrder}). As expected in an ice crystal constructed of
99 > (Fig. \ref{protOrder}).  As expected in an ice crystal constructed of
100   water tetramers, the hydrogen bonds are not as linear as those
101   observed in ice $I_h$, however the interlocking of these subunits
102 < appears to provide significant stabilization to the overall
103 < crystal. The arrangement of these tetramers results in surrounding
104 < open octagonal cavities that are typically greater than 6.3 \AA\ in
105 < diameter. This relatively open overall structure leads to crystals
102 > appears to provide significant stabilization to the overall crystal.
103 > The arrangement of these tetramers results in surrounding open
104 > octagonal cavities that are typically greater than 6.3 \AA\ in
105 > diameter.  This relatively open overall structure leads to crystals
106   that are 0.07 g/cm$^3$ less dense on average than ice $I_h$.
107  
108   \begin{figure}
# Line 116 | Line 118 | down the (001) crystal face. The rows of water tetrame
118   \begin{figure}
119   \includegraphics[width=\linewidth]{orderedIcei.eps}
120   \caption{Image of a proton ordered crystal of Ice-{\it i} looking
121 < down the (001) crystal face. The rows of water tetramers surrounded by
122 < octagonal pores leads to a crystal structure that is significantly
121 > down the (001) crystal face.  The rows of water tetramers surrounded
122 > by octagonal pores leads to a crystal structure that is significantly
123   less dense than ice $I_h$.}
124   \label{protOrder}
125   \end{figure}
# Line 128 | Line 130 | contributions to the overall free energy. To address t
130   see our previous work and related
131   articles).\cite{Fennell04,Liu96,Bratko85} Those results only
132   considered energetic stabilization and neglected entropic
133 < contributions to the overall free energy. To address this issue, we
133 > contributions to the overall free energy.  To address this issue, we
134   have calculated the absolute free energy of this crystal using
135   thermodynamic integration and compared to the free energies of cubic
136   and hexagonal ice $I$ (the experimental low density ice polymorphs)
# Line 139 | Line 141 | was used in calculations involving SPC/E, TIP4P, and T
141   common water models (TIP3P, TIP4P, TIP5P, and SPC/E) and a reaction
142   field parametrized single point dipole water model (SSD/RF). It should
143   be noted that a second version of Ice-{\it i} (Ice-{\it i}$^\prime$)
144 < was used in calculations involving SPC/E, TIP4P, and TIP5P. The unit
144 > was used in calculations involving SPC/E, TIP4P, and TIP5P.  The unit
145   cell of this crystal (Fig. \ref{iceiCell}B) is similar to the Ice-{\it
146   i} unit it is extended in the direction of the (001) face and
147   compressed along the other two faces.  There is typically a small
# Line 154 | Line 156 | propagated using the symplectic DLM integration method
156   Canonical ensemble (NVT) molecular dynamics calculations were
157   performed using the OOPSE molecular mechanics package.\cite{Meineke05}
158   All molecules were treated as rigid bodies, with orientational motion
159 < propagated using the symplectic DLM integration method. Details about
159 > propagated using the symplectic DLM integration method.  Details about
160   the implementation of this technique can be found in a recent
161   publication.\cite{Dullweber1997}
162  
# Line 167 | Line 169 | generate phase diagrams. All simulations were carried
169   SSD/E water models.\cite{Baez95a} Liquid state free energies at 300
170   and 400 K for all of these water models were also determined using
171   this same technique in order to determine melting points and to
172 < generate phase diagrams. All simulations were carried out at densities
173 < which correspond to a pressure of approximately 1 atm at their
174 < respective temperatures.
172 > generate phase diagrams.  All simulations were carried out at
173 > densities which correspond to a pressure of approximately 1 atm at
174 > their respective temperatures.
175  
176   Thermodynamic integration involves a sequence of simulations during
177   which the system of interest is converted into a reference system for
178 < which the free energy is known analytically. This transformation path
178 > which the free energy is known analytically.  This transformation path
179   is then integrated in order to determine the free energy difference
180   between the two states:
181   \begin{equation}
# Line 181 | Line 183 | transformation parameter that scales the overall
183   )}{\partial\lambda}\right\rangle_\lambda d\lambda,
184   \end{equation}
185   where $V$ is the interaction potential and $\lambda$ is the
186 < transformation parameter that scales the overall
187 < potential. Simulations are distributed strategically along this path
188 < in order to sufficiently sample the regions of greatest change in the
189 < potential. Typical integrations in this study consisted of $\sim$25
190 < simulations ranging from 300 ps (for the unaltered system) to 75 ps
191 < (near the reference state) in length.
186 > transformation parameter that scales the overall potential.
187 > Simulations are distributed strategically along this path in order to
188 > sufficiently sample the regions of greatest change in the potential.
189 > Typical integrations in this study consisted of $\sim$25 simulations
190 > ranging from 300 ps (for the unaltered system) to 75 ps (near the
191 > reference state) in length.
192  
193   For the thermodynamic integration of molecular crystals, the Einstein
194 < crystal was chosen as the reference system. In an Einstein crystal,
194 > crystal was chosen as the reference system.  In an Einstein crystal,
195   the molecules are restrained at their ideal lattice locations and
196   orientations. Using harmonic restraints, as applied by B\`{a}ez and
197   Clancy, the total potential for this reference crystal
# Line 201 | Line 203 | respectively.  It is clear from Fig. \ref{waterSpring}
203   where $K_\mathrm{v}$, $K_\mathrm{\theta}$, and $K_\mathrm{\omega}$ are
204   the spring constants restraining translational motion and deflection
205   of and rotation around the principle axis of the molecule
206 < respectively.  It is clear from Fig. \ref{waterSpring} that the values
207 < of $\theta$ range from $0$ to $\pi$, while $\omega$ ranges from
208 < $-\pi$ to $\pi$.  The partition function for a molecular crystal
206 > respectively.  These spring constants are typically calculated from
207 > the mean-square displacements of water molecules in an unrestrained
208 > ice crystal at 200 K.  For these studies, $K_\mathrm{r} = 4.29$ kcal
209 > mol$^{-1}$, $K_\theta\ = 13.88$ kcal mol$^{-1}$, and $K_\omega\ =
210 > 17.75$ kcal mol$^{-1}$.  It is clear from Fig. \ref{waterSpring} that
211 > the values of $\theta$ range from $0$ to $\pi$, while $\omega$ ranges
212 > from $-\pi$ to $\pi$.  The partition function for a molecular crystal
213   restrained in this fashion can be evaluated analytically, and the
214   Helmholtz Free Energy ({\it A}) is given by
215   \begin{eqnarray}
# Line 225 | Line 231 | body-frame {\it z}-axis. $K_\theta$ and $K_\omega$ are
231   \caption{Possible orientational motions for a restrained molecule.
232   $\theta$ angles correspond to displacement from the body-frame {\it
233   z}-axis, while $\omega$ angles correspond to rotation about the
234 < body-frame {\it z}-axis. $K_\theta$ and $K_\omega$ are spring
234 > body-frame {\it z}-axis.  $K_\theta$ and $K_\omega$ are spring
235   constants for the harmonic springs restraining motion in the $\theta$
236   and $\omega$ directions.}
237   \label{waterSpring}
# Line 245 | Line 251 | cubic switching between 100\% and 85\% of the cutoff v
251   methods.\cite{Baez95b}
252  
253   Charge, dipole, and Lennard-Jones interactions were modified by a
254 < cubic switching between 100\% and 85\% of the cutoff value (9 \AA
255 < ). By applying this function, these interactions are smoothly
256 < truncated, thereby avoiding the poor energy conservation which results
257 < from harsher truncation schemes. The effect of a long-range correction
258 < was also investigated on select model systems in a variety of
259 < manners. For the SSD/RF model, a reaction field with a fixed
260 < dielectric constant of 80 was applied in all
261 < simulations.\cite{Onsager36} For a series of the least computationally
262 < expensive models (SSD/E, SSD/RF, and TIP3P), simulations were
263 < performed with longer cutoffs of 12 and 15 \AA\ to compare with the 9
264 < \AA\ cutoff results. Finally, the effects of utilizing an Ewald
265 < summation were estimated for TIP3P and SPC/E by performing single
266 < configuration calculations with Particle-Mesh Ewald (PME) in the
267 < TINKER molecular mechanics software package.\cite{Tinker} The
268 < calculated energy difference in the presence and absence of PME was
269 < applied to the previous results in order to predict changes to the
264 < free energy landscape.
254 > cubic switching between 100\% and 85\% of the cutoff value (9 \AA).
255 > By applying this function, these interactions are smoothly truncated,
256 > thereby avoiding the poor energy conservation which results from
257 > harsher truncation schemes.  The effect of a long-range correction was
258 > also investigated on select model systems in a variety of manners.
259 > For the SSD/RF model, a reaction field with a fixed dielectric
260 > constant of 80 was applied in all simulations.\cite{Onsager36} For a
261 > series of the least computationally expensive models (SSD/E, SSD/RF,
262 > and TIP3P), simulations were performed with longer cutoffs of 12 and
263 > 15 \AA\ to compare with the 9 \AA\ cutoff results.  Finally, the
264 > effects of utilizing an Ewald summation were estimated for TIP3P and
265 > SPC/E by performing single configuration calculations with
266 > Particle-Mesh Ewald (PME) in the TINKER molecular mechanics software
267 > package.\cite{Tinker} The calculated energy difference in the presence
268 > and absence of PME was applied to the previous results in order to
269 > predict changes to the free energy landscape.
270  
271   \section{Results and discussion}
272  
# Line 273 | Line 278 | as proton disordered or antiferroelectric variants of
278   model at ambient conditions (Table \ref{freeEnergy}).\cite{Baez95b}
279   Ice XI, the experimentally-observed proton-ordered variant of ice
280   $I_h$, was investigated initially, but was found to be not as stable
281 < as proton disordered or antiferroelectric variants of ice $I_h$. The
281 > as proton disordered or antiferroelectric variants of ice $I_h$.  The
282   proton ordered variant of ice $I_h$ used here is a simple
283   antiferroelectric version that we devised, and it has an 8 molecule
284   unit cell similar to other predicted antiferroelectric $I_h$
285   crystals.\cite{Davidson84} The crystals contained 648 or 1728
286   molecules for ice B, 1024 or 1280 molecules for ice $I_h$, 1000
287 < molecules for ice $I_c$, or 1024 molecules for Ice-{\it i}. The larger
288 < crystal sizes were necessary for simulations involving larger cutoff
289 < values.
287 > molecules for ice $I_c$, or 1024 molecules for Ice-{\it i}.  The
288 > larger crystal sizes were necessary for simulations involving larger
289 > cutoff values.
290  
291   \begin{table*}
292   \begin{minipage}{\linewidth}
293   \begin{center}
294  
295   \caption{Calculated free energies for several ice polymorphs with a
296 < variety of common water models. All calculations used a cutoff radius
297 < of 9 \AA\ and were performed at 200 K and $\sim$1 atm. Units are
298 < kcal/mol. Calculated error of the final digits is in parentheses.}
296 > variety of common water models.  All calculations used a cutoff radius
297 > of 9 \AA\ and were performed at 200 K and $\sim$1 atm.  Units are
298 > kcal/mol.  Calculated error of the final digits is in parentheses.}
299  
300   \begin{tabular}{lcccc}
301   \hline
# Line 310 | Line 315 | models studied. With the calculated free energy at the
315  
316   The free energy values computed for the studied polymorphs indicate
317   that Ice-{\it i} is the most stable state for all of the common water
318 < models studied. With the calculated free energy at these state points,
319 < the Gibbs-Helmholtz equation was used to project to other state points
320 < and to build phase diagrams.  Figures
321 < \ref{tp3phasedia} and \ref{ssdrfphasedia} are example diagrams built
322 < from the free energy results. All other models have similar structure,
323 < although the crossing points between the phases move to slightly
324 < different temperatures and pressures. It is interesting to note that
325 < ice $I$ does not exist in either cubic or hexagonal form in any of the
326 < phase diagrams for any of the models. For purposes of this study, ice
327 < B is representative of the dense ice polymorphs. A recent study by
328 < Sanz {\it et al.} goes into detail on the phase diagrams for SPC/E and
318 > models studied.  With the calculated free energy at these state
319 > points, the Gibbs-Helmholtz equation was used to project to other
320 > state points and to build phase diagrams.  Figures \ref{tp3phasedia}
321 > and \ref{ssdrfphasedia} are example diagrams built from the free
322 > energy results.  All other models have similar structure, although the
323 > crossing points between the phases move to slightly different
324 > temperatures and pressures.  It is interesting to note that ice $I$
325 > does not exist in either cubic or hexagonal form in any of the phase
326 > diagrams for any of the models.  For purposes of this study, ice B is
327 > representative of the dense ice polymorphs.  A recent study by Sanz
328 > {\it et al.} goes into detail on the phase diagrams for SPC/E and
329   TIP4P at higher pressures than those studied here.\cite{Sanz04}
330  
331   \begin{figure}
332   \includegraphics[width=\linewidth]{tp3PhaseDia.eps}
333   \caption{Phase diagram for the TIP3P water model in the low pressure
334 < regime. The displayed $T_m$ and $T_b$ values are good predictions of
334 > regime.  The displayed $T_m$ and $T_b$ values are good predictions of
335   the experimental values; however, the solid phases shown are not the
336 < experimentally observed forms. Both cubic and hexagonal ice $I$ are
336 > experimentally observed forms.  Both cubic and hexagonal ice $I$ are
337   higher in energy and don't appear in the phase diagram.}
338   \label{tp3phasedia}
339   \end{figure}
# Line 336 | Line 341 | regime. Calculations producing these results were done
341   \begin{figure}
342   \includegraphics[width=\linewidth]{ssdrfPhaseDia.eps}
343   \caption{Phase diagram for the SSD/RF water model in the low pressure
344 < regime. Calculations producing these results were done under an
345 < applied reaction field. It is interesting to note that this
344 > regime.  Calculations producing these results were done under an
345 > applied reaction field.  It is interesting to note that this
346   computationally efficient model (over 3 times more efficient than
347   TIP3P) exhibits phase behavior similar to the less computationally
348   conservative charge based models.}
# Line 350 | Line 355 | experiment. The $T_m$ and $T_s$ values from simulation
355  
356   \caption{Melting ($T_m$), boiling ($T_b$), and sublimation ($T_s$)
357   temperatures at 1 atm for several common water models compared with
358 < experiment. The $T_m$ and $T_s$ values from simulation correspond to a
359 < transition between Ice-{\it i} (or Ice-{\it i}$^\prime$) and the
358 > experiment.  The $T_m$ and $T_s$ values from simulation correspond to
359 > a transition between Ice-{\it i} (or Ice-{\it i}$^\prime$) and the
360   liquid or gas state.}
361  
362   \begin{tabular}{lccccccc}
# Line 368 | Line 373 | calculated from this work. Surprisingly, most of these
373   \end{table*}
374  
375   Table \ref{meltandboil} lists the melting and boiling temperatures
376 < calculated from this work. Surprisingly, most of these models have
377 < melting points that compare quite favorably with experiment. The
376 > calculated from this work.  Surprisingly, most of these models have
377 > melting points that compare quite favorably with experiment.  The
378   unfortunate aspect of this result is that this phase change occurs
379   between Ice-{\it i} and the liquid state rather than ice $I_h$ and the
380 < liquid state. These results are actually not contrary to previous
381 < studies in the literature. Earlier free energy studies of ice $I$
382 < using TIP4P predict a $T_m$ ranging from 214 to 238 K (differences
383 < being attributed to choice of interaction truncation and different
379 < ordered and disordered molecular
380 > liquid state.  These results are actually not contrary to other
381 > studies.  Studies of ice $I_h$ using TIP4P predict a $T_m$ ranging
382 > from 214 to 238 K (differences being attributed to choice of
383 > interaction truncation and different ordered and disordered molecular
384   arrangements).\cite{Vlot99,Gao00,Sanz04} If the presence of ice B and
385   Ice-{\it i} were omitted, a $T_m$ value around 210 K would be
386 < predicted from this work. However, the $T_m$ from Ice-{\it i} is
387 < calculated at 265 K, significantly higher in temperature than the
388 < previous studies. Also of interest in these results is that SSD/E does
389 < not exhibit a melting point at 1 atm, but it shows a sublimation point
390 < at 355 K. This is due to the significant stability of Ice-{\it i} over
391 < all other polymorphs for this particular model under these
392 < conditions. While troubling, this behavior resulted in spontaneous
386 > predicted from this work.  However, the $T_m$ from Ice-{\it i} is
387 > calculated to be 265 K, indicating that these simulation based
388 > structures ought to be included in studies probing phase transitions
389 > with this model.  Also of interest in these results is that SSD/E does
390 > not exhibit a melting point at 1 atm, but it shows a sublimation point
391 > at 355 K.  This is due to the significant stability of Ice-{\it i}
392 > over all other polymorphs for this particular model under these
393 > conditions.  While troubling, this behavior resulted in spontaneous
394   crystallization of Ice-{\it i} and led us to investigate this
395 < structure. These observations provide a warning that simulations of
395 > structure.  These observations provide a warning that simulations of
396   SSD/E as a ``liquid'' near 300 K are actually metastable and run the
397 < risk of spontaneous crystallization. However, this risk lessens when
397 > risk of spontaneous crystallization.  However, this risk lessens when
398   applying a longer cutoff.
399  
400   \begin{figure}
401   \includegraphics[width=\linewidth]{cutoffChange.eps}
402 < \caption{Free energy as a function of cutoff radius for (A) SSD/E, (B)
403 < TIP3P, and (C) SSD/RF with a reaction field. Both SSD/E and TIP3P show
404 < significant cutoff radius dependence of the free energy and appear to
405 < converge when moving to cutoffs greater than 12 \AA. Use of a reaction
406 < field with SSD/RF results in free energies that exhibit minimal cutoff
407 < radius dependence.}
402 > \caption{Free energy as a function of cutoff radius for SSD/E, TIP3P,
403 > SPC/E, SSD/RF with a reaction field, and the TIP3P and SPC/E models
404 > with an added Ewald correction term.  Calculations performed without a
405 > long-range correction show noticable free energy dependence on the
406 > cutoff radius and show some degree of converge at large cutoff radii.
407 > Inclusion of a long-range correction reduces the cutoff radius
408 > dependence of the free energy for all the models.  Data for ice I$_c$
409 > with TIP3P using both 12 and 13.5 \AA\ cutoffs were omitted because
410 > the crystal was prone to distortion and melting at 200 K.  Ice-{\it
411 > i}$^\prime$ is the form of Ice-{\it i} used in the SPC/E simulations.}
412   \label{incCutoff}
413   \end{figure}
414  
415   Increasing the cutoff radius in simulations of the more
416   computationally efficient water models was done in order to evaluate
417   the trend in free energy values when moving to systems that do not
418 < involve potential truncation. As seen in Fig. \ref{incCutoff}, the
419 < free energy of all the ice polymorphs for the SSD/E and TIP3P models
420 < show a substantial dependence on cutoff radius. In general, there is a
421 < narrowing of the free energy differences while moving to greater
422 < cutoff radii.  As the free energies for the polymorphs converge, the
423 < stability advantage that Ice-{\it i} exhibits is reduced; however, it
424 < remains the most stable polymorph for both of these models over the
425 < depicted range for both models. This narrowing trend is not
426 < significant in the case of SSD/RF, indicating that the free energies
427 < calculated with a reaction field present provide, at minimal
428 < computational cost, a more accurate picture of the free energy
429 < landscape in the absence of potential truncation.  Interestingly,
430 < increasing the cutoff radius a mere 1.5 \AA\ with the SSD/E model
431 < destabilizes the Ice-{\it i} polymorph enough that the liquid state is
432 < preferred under standard simulation conditions (298 K and 1
433 < atm). Thus, it is recommended that simulations using this model choose
434 < interaction truncation radii greater than 9 \AA. Considering this
435 < stabilization provided by smaller cutoffs, it is not surprising that
436 < crystallization into Ice-{\it i} was observed with SSD/E.  The choice
437 < of a 9 \AA\ cutoff in the previous simulations gives the Ice-{\it i}
429 < polymorph a greater than 1 kcal/mol lower free energy than the ice
430 < $I_\textrm{h}$ starting configurations.
418 > involve potential truncation.  As seen in Fig. \ref{incCutoff}, the
419 > free energy of the ice polymorphs with water models lacking a
420 > long-range correction show a significant cutoff radius dependence.  In
421 > general, there is a narrowing of the free energy differences while
422 > moving to greater cutoff radii.  As the free energies for the
423 > polymorphs converge, the stability advantage that Ice-{\it i} exhibits
424 > is reduced.  Interestingly, increasing the cutoff radius a mere 1.5
425 > \AA\ with the SSD/E model destabilizes the Ice-{\it i} polymorph
426 > enough that the liquid state is preferred under standard simulation
427 > conditions (298 K and 1 atm).  Thus, it is recommended that
428 > simulations using this model choose interaction truncation radii
429 > greater than 9 \AA.  Considering the stabilization of Ice-{\it i} with
430 > smaller cutoffs, it is not surprising that crystallization was
431 > observed with SSD/E.  The choice of a 9 \AA\ cutoff in the previous
432 > simulations gives the Ice-{\it i} polymorph a greater than 1 kcal/mol
433 > lower free energy than the ice $I_\textrm{h}$ starting configurations.
434 > Additionally, it should be noted that ice $I_c$ is not stable with
435 > cutoff radii of 12 and 13.5 \AA\ using the TIP3P water model.  These
436 > simulations showed bulk distortions of the simulation cell that
437 > rapidly deteriorated crystal integrity.
438  
439 < To further study the changes resulting to the inclusion of a
440 < long-range interaction correction, the effect of an Ewald summation
441 < was estimated by applying the potential energy difference do to its
442 < inclusion in systems in the presence and absence of the correction.
443 < This was accomplished by calculation of the potential energy of
444 < identical crystals both with and without PME.  The free energies for
445 < the investigated polymorphs using the TIP3P and SPC/E water models are
446 < shown in Table \ref{pmeShift}.  The same trend pointed out through
447 < increase of cutoff radius is observed in these PME results. Ice-{\it
448 < i} is the preferred polymorph at ambient conditions for both the TIP3P
449 < and SPC/E water models; however, the narrowing of the free energy
450 < differences between the various solid forms with the SPC/E model is
451 < significant enough that it becomes less clear that it is the most
452 < stable polymorph.  The free energies of Ice-{\it i} and $I_\textrm{c}$
453 < overlap within error, while ice B and $I_\textrm{h}$ are just outside
454 < at t slightly higher free energy.  This indicates that with SPC/E,
455 < Ice-{\it i} might be metastable with all the studied polymorphs,
456 < particularly ice $I_\textrm{c}$. However, these results do not
457 < significantly alter the finding that the Ice-{\it i} polymorph is a
458 < stable crystal structure that should be considered when studying the
459 < phase behavior of water models.
439 > Adjacent to each of these model plots is a system with an applied or
440 > estimated long-range correction.  SSD/RF was parametrized for use with
441 > a reaction field, and the benefit provided by this computationally
442 > inexpensive correction is apparent.  Due to the relative independence
443 > of the resultant free energies, calculations performed with a small
444 > cutoff radius provide resultant properties similar to what one would
445 > expect for the bulk material.  In the cases of TIP3P and SPC/E, the
446 > effect of an Ewald summation was estimated by applying the potential
447 > energy difference do to its inclusion in systems in the presence and
448 > absence of the correction.  This was accomplished by calculation of
449 > the potential energy of identical crystals both with and without
450 > particle mesh Ewald (PME).  Similar behavior to that observed with
451 > reaction field is seen for both of these models.  The free energies
452 > show less dependence on cutoff radius and span a more narrowed range
453 > for the various polymorphs.  Like the dipolar water models, TIP3P
454 > displays a relatively constant preference for the Ice-{\it i}
455 > polymorph.  Crystal preference is much more difficult to determine for
456 > SPC/E.  Without a long-range correction, each of the polymorphs
457 > studied assumes the role of the preferred polymorph under different
458 > cutoff conditions.  The inclusion of the Ewald correction flattens and
459 > narrows the sequences of free energies so much that they often overlap
460 > within error (see Table \ref{spcecut}), indicating that other
461 > conditions, such as cell volume in microcanonical simulations, can
462 > influence the chosen polymorph upon crystallization.  All of these
463 > results support the finding that the Ice-{\it i} polymorph is a stable
464 > crystal structure that should be considered when studying the phase
465 > behavior of water models.
466  
467   \begin{table*}
468   \begin{minipage}{\linewidth}
469   \begin{center}
470  
471 < \caption{The free energy of the studied ice polymorphs after applying
472 < the energy difference attributed to the inclusion of the PME
473 < long-range interaction correction. Units are kcal/mol.}
471 > \caption{The free energy versus cutoff radius for the studied ice
472 > polymorphs using SPC/E after the inclusion of the PME long-range
473 > interaction correction. Units are kcal/mol.}
474  
475   \begin{tabular}{ccccc}
476   \hline
477 < Water Model &  $I_h$ & $I_c$ &  B & Ice-{\it i} \\
477 > Cutoff (\AA) & $I_h$ & $I_c$ & B & Ice-{\it i} \\
478   \hline
479 < TIP3P  & -11.53(2) & -11.24(3) & -11.51(3) & -11.67(3) \\
480 < SPC/E  & -12.97(2) & -13.00(2) & -12.96(3) & -13.02(2) \\
479 > 9.0   & -12.98(2) & -13.00(2) & -12.97(3) & -13.02(2) \\
480 > 10.5  & -13.13(3) & -13.09(4) & -13.17(3) & -13.11(2) \\
481 > 12.0  & -13.06(2) & -13.09(2) & -13.15(4) & -13.12(2) \\
482 > 13.5  & -13.02(2) & -13.02(2) & -13.08(2) & -13.07(2) \\
483 > 15.0  & -13.11(4) & -12.97(2) & -13.09(2) & -12.95(2) \\
484   \end{tabular}
485 < \label{pmeShift}
485 > \label{spcecut}
486   \end{center}
487   \end{minipage}
488   \end{table*}
# Line 476 | Line 492 | via thermodynamic integration. All the water models st
492   The free energy for proton ordered variants of hexagonal and cubic ice
493   $I$, ice B, and our recently discovered Ice-{\it i} structure were
494   calculated under standard conditions for several common water models
495 < via thermodynamic integration. All the water models studied show
495 > via thermodynamic integration.  All the water models studied show
496   Ice-{\it i} to be the minimum free energy crystal structure with a 9
497 < \AA\ switching function cutoff. Calculated melting and boiling points
497 > \AA\ switching function cutoff.  Calculated melting and boiling points
498   show surprisingly good agreement with the experimental values;
499 < however, the solid phase at 1 atm is Ice-{\it i}, not ice $I_h$. The
499 > however, the solid phase at 1 atm is Ice-{\it i}, not ice $I_h$.  The
500   effect of interaction truncation was investigated through variation of
501   the cutoff radius, use of a reaction field parameterized model, and
502 < estimation of the results in the presence of the Ewald
503 < summation. Interaction truncation has a significant effect on the
504 < computed free energy values, and may significantly alter the free
505 < energy landscape for the more complex multipoint water models. Despite
506 < these effects, these results show Ice-{\it i} to be an important ice
507 < polymorph that should be considered in simulation studies.
502 > estimation of the results in the presence of the Ewald summation.
503 > Interaction truncation has a significant effect on the computed free
504 > energy values, and may significantly alter the free energy landscape
505 > for the more complex multipoint water models.  Despite these effects,
506 > these results show Ice-{\it i} to be an important ice polymorph that
507 > should be considered in simulation studies.
508  
509   Due to this relative stability of Ice-{\it i} in all of the
510   investigated simulation conditions, the question arises as to possible

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