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2   %\documentclass[prb,aps,twocolumn,tabularx]{revtex4}
3   \documentclass[preprint,aps,endfloats]{revtex4}
4   %\documentclass[11pt]{article}
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21  
22   \begin{document}
23  
24 < \title{A Free Energy Study of Low Temperature and Anomolous Ice}
24 > \title{A Free Energy Study of Low Temperature and Anomalous Ice}
25  
26   \author{Christopher J. Fennell and J. Daniel Gezelter{\thefootnote}
27   \footnote[1]{Corresponding author. \ Electronic mail: gezelter@nd.edu}}
# Line 34 | Line 35 | Notre Dame, Indiana 46556}
35   %\doublespacing
36  
37   \begin{abstract}
38 + The free energies of several ice polymorphs in the low pressure regime
39 + were calculated using thermodynamic integration of systems consisting
40 + of a variety of common water models. Ice-{\it i}, a recent
41 + computationally observed solid structure, was determined to be the
42 + stable state with the lowest free energy for all the water models
43 + investigated. Phase diagrams were generated, and melting and boiling
44 + points for all the models were determined and show relatively good
45 + agreement with experiment, although the solid phase is different
46 + between simulation and experiment. In addition, potential truncation
47 + was shown to have an effect on the calculated free energies, and may
48 + result in altered free energy landscapes.
49   \end{abstract}
50  
51   \maketitle
# Line 48 | Line 60 | Notre Dame, Indiana 46556}
60  
61   \section{Introduction}
62  
63 + Molecular dynamics has developed into a valuable tool for studying the
64 + phase behavior of systems ranging from small or simple
65 + molecules\cite{smallStuff} to complex biological
66 + species.\cite{bigStuff} Many techniques have been developed in order
67 + to investigate the thermodynamic properites of model substances,
68 + providing both qualitative and quantitative comparisons between
69 + simulations and experiment.\cite{thermMethods} Investigation of these
70 + properties leads to the development of new and more accurate models,
71 + leading to better understanding and depiction of physical processes
72 + and intricate molecular systems.
73 +
74 + Water has proven to be a challenging substance to depict in
75 + simulations, and has resulted in a variety of models that attempt to
76 + describe its behavior under a varying simulation
77 + conditions.\cite{lotsOfWaterPapers} Many of these models have been
78 + used to investigate important physical phenomena like phase
79 + transitions and the hydrophobic effect.\cite{evenMorePapers} With the
80 + advent of numerous differing models, it is only natural that attention
81 + is placed on the properties of the models themselves in an attempt to
82 + clarify their benefits and limitations when applied to a system of
83 + interest.\cite{modelProps} One important but challenging property to
84 + quantify is the free energy, particularly of the solid forms of
85 + water. Difficulty in these types of studies typically arises from the
86 + assortment of possible crystalline polymorphs that water that water
87 + adopts over a wide range of pressures and temperatures. There are
88 + currently 13 recognized forms of ice, and it is a challenging task to
89 + investigate the entire free energy landscape.\cite{Sanz04} Ideally,
90 + research is focused on the phases having the lowest free energy,
91 + because these phases will dictate the true transition temperatures and
92 + pressures for their respective model.
93 +
94 + In this paper, standard reference state methods were applied to the
95 + study of crystalline water polymorphs in the low pressure regime. This
96 + work is unique in the fact that one of the crystal lattices was
97 + arrived at through crystallization of a computationally efficient
98 + water model under constant pressure and temperature
99 + conditions. Crystallization events are interesting in and of
100 + themselves\cite{nucleationStudies}; however, the crystal structure
101 + obtained in this case was different from any previously observed ice
102 + polymorphs, in experiment or simulation.\cite{Fennell04} This crystal
103 + was termed Ice-{\it i} in homage to its origin in computational
104 + simulation. The unit cell (Fig. \ref{iceiCell}A) consists of eight
105 + water molecules that stack in rows of interlocking water
106 + tetramers. Proton ordering can be accomplished by orienting two of the
107 + waters so that both of their donated hydrogen bonds are internal to
108 + their tetramer (Fig. \ref{protOrder}). As expected in an ice crystal
109 + constructed of water tetramers, the hydrogen bonds are not as linear
110 + as those observed in ice $I_h$, however the interlocking of these
111 + subunits appears to provide significant stabilization to the overall
112 + crystal. The arrangement of these tetramers results in surrounding
113 + open octagonal cavities that are typically greater than 6.3 \AA\ in
114 + diameter. This relatively open overall structure leads to crystals
115 + that are 0.07 g/cm$^3$ less dense on average than ice $I_h$.
116 + \begin{figure}
117 + \includegraphics[scale=1.0]{unitCell.eps}
118 + \caption{Unit cells for (A) Ice-{\it i} and (B) Ice-2{\it i}, the elongated variant of Ice-{\it i}.  For Ice-{\it i}, the $a$ to $c$ relation is given by $a = 2.1214c$, while for Ice-2{\it i}, $a = 1.7850c$.}
119 + \label{iceiCell}
120 + \end{figure}
121 + \begin{figure}
122 + \includegraphics[scale=1.0]{orderedIcei.eps}
123 + \caption{Image of a proton ordered crystal of Ice-{\it i} looking
124 + down the (001) crystal face. The rows of water tetramers surrounded by
125 + octagonal pores leads to a crystal structure that is significantly
126 + less dense than ice $I_h$.}
127 + \label{protOrder}
128 + \end{figure}
129 +
130 + Results in the previous study indicated that Ice-{\it i} is the
131 + minimum energy crystal structure for the single point water models
132 + being studied (for discussions on these single point dipole models,
133 + see the previous work and related
134 + articles\cite{Fennell04,Ichiye96,Bratko85}). Those results only
135 + consider energetic stabilization and neglect entropic contributions to
136 + the overall free energy. To address this issue, the absolute free
137 + energy of this crystal was calculated using thermodynamic integration
138 + and compared to the free energies of cubic and hexagonal ice $I$ (the
139 + experimental low density ice polymorphs) and ice B (a higher density,
140 + but very stable crystal structure observed by B\`{a}ez and Clancy in
141 + free energy studies of SPC/E).\cite{Baez95b} This work includes
142 + results for the water model from which Ice-{\it i} was crystallized
143 + (soft sticky dipole extended, SSD/E) in addition to several common
144 + water models (TIP3P, TIP4P, TIP5P, and SPC/E) and a reaction field
145 + parametrized single point dipole water model (soft sticky dipole
146 + reaction field, SSD/RF). In should be noted that a second version of
147 + Ice-{\it i} (Ice-2{\it i}) was used in calculations involving SPC/E,
148 + TIP4P, and TIP5P. The unit cell of this crystal (Fig. \ref{iceiCell}B)
149 + is similar to the Ice-{\it i} unit it is extended in the direction of
150 + the (001) face and compressed along the other two faces.
151 +
152   \section{Methods}
153  
154 + Canonical ensemble (NVT) molecular dynamics calculations were
155 + performed using the OOPSE (Object-Oriented Parallel Simulation Engine)
156 + molecular mechanics package. All molecules were treated as rigid
157 + bodies, with orientational motion propagated using the symplectic DLM
158 + integration method. Details about the implementation of these
159 + techniques can be found in a recent publication.\cite{Meineke05}
160 +
161 + Thermodynamic integration was utilized to calculate the free energy of
162 + several ice crystals at 200 K using the TIP3P, TIP4P, TIP5P, SPC/E,
163 + SSD/RF, and SSD/E water models. Liquid state free energies at 300 and
164 + 400 K for all of these water models were also determined using this
165 + same technique, in order to determine melting points and generate
166 + phase diagrams. All simulations were carried out at densities
167 + resulting in a pressure of approximately 1 atm at their respective
168 + temperatures.
169 +
170 + A single thermodynamic integration involves a sequence of simulations
171 + over which the system of interest is converted into a reference system
172 + for which the free energy is known. This transformation path is then
173 + integrated in order to determine the free energy difference between
174 + the two states:
175 + \begin{equation}
176 + \Delta A = \int_0^1\left\langle\frac{\partial V(\lambda
177 + )}{\partial\lambda}\right\rangle_\lambda d\lambda,
178 + \end{equation}
179 + where $V$ is the interaction potential and $\lambda$ is the
180 + transformation parameter that scales the overall
181 + potential. Simulations are distributed unevenly along this path in
182 + order to sufficiently sample the regions of greatest change in the
183 + potential. Typical integrations in this study consisted of $\sim$25
184 + simulations ranging from 300 ps (for the unaltered system) to 75 ps
185 + (near the reference state) in length.
186 +
187 + For the thermodynamic integration of molecular crystals, the Einstein
188 + Crystal is chosen as the reference state that the system is converted
189 + to over the course of the simulation. In an Einstein Crystal, the
190 + molecules are harmonically restrained at their ideal lattice locations
191 + and orientations. The partition function for a molecular crystal
192 + restrained in this fashion has been evaluated, and the Helmholtz Free
193 + Energy ({\it A}) is given by
194 + \begin{eqnarray}
195 + A = E_m\ -\ kT\ln \left (\frac{kT}{h\nu}\right )^3&-&kT\ln \left
196 + [\pi^\frac{1}{2}\left (\frac{8\pi^2I_\mathrm{A}kT}{h^2}\right
197 + )^\frac{1}{2}\left (\frac{8\pi^2I_\mathrm{B}kT}{h^2}\right
198 + )^\frac{1}{2}\left (\frac{8\pi^2I_\mathrm{C}kT}{h^2}\right
199 + )^\frac{1}{2}\right ] \nonumber \\ &-& kT\ln \left [\frac{kT}{2(\pi
200 + K_\omega K_\theta)^{\frac{1}{2}}}\exp\left
201 + (-\frac{kT}{2K_\theta}\right)\int_0^{\left (\frac{kT}{2K_\theta}\right
202 + )^\frac{1}{2}}\exp(t^2)\mathrm{d}t\right ],
203 + \label{ecFreeEnergy}
204 + \end{eqnarray}
205 + where $2\pi\nu = (K_\mathrm{v}/m)^{1/2}$.\cite{Baez95a} In equation
206 + \ref{ecFreeEnergy}, $K_\mathrm{v}$, $K_\mathrm{\theta}$, and
207 + $K_\mathrm{\omega}$ are the spring constants restraining translational
208 + motion and deflection of and rotation around the principle axis of the
209 + molecule respectively (Fig. \ref{waterSpring}), and $E_m$ is the
210 + minimum potential energy of the ideal crystal. In the case of
211 + molecular liquids, the ideal vapor is chosen as the target reference
212 + state.
213 + \begin{figure}
214 + \includegraphics[scale=1.0]{rotSpring.eps}
215 + \caption{Possible orientational motions for a restrained molecule.
216 + $\theta$ angles correspond to displacement from the body-frame {\it
217 + z}-axis, while $\omega$ angles correspond to rotation about the
218 + body-frame {\it z}-axis. $K_\theta$ and $K_\omega$ are spring
219 + constants for the harmonic springs restraining motion in the $\theta$
220 + and $\omega$ directions.}
221 + \label{waterSpring}
222 + \end{figure}
223 +
224 + Charge, dipole, and Lennard-Jones interactions were modified by a
225 + cubic switching between 100\% and 85\% of the cutoff value (9 \AA ). By
226 + applying this function, these interactions are smoothly truncated,
227 + thereby avoiding poor energy conserving dynamics resulting from
228 + harsher truncation schemes. The effect of a long-range correction was
229 + also investigated on select model systems in a variety of manners. For
230 + the SSD/RF model, a reaction field with a fixed dielectric constant of
231 + 80 was applied in all simulations.\cite{Onsager36} For a series of the
232 + least computationally expensive models (SSD/E, SSD/RF, and TIP3P),
233 + simulations were performed with longer cutoffs of 12 and 15 \AA\ to
234 + compare with the 9 \AA\ cutoff results. Finally, results from the use
235 + of an Ewald summation were estimated for TIP3P and SPC/E by performing
236 + calculations with Particle-Mesh Ewald (PME) in the TINKER molecular
237 + mechanics software package. TINKER was chosen because it can also
238 + propagate the motion of rigid-bodies, and provides the most direct
239 + comparison to the results from OOPSE. The calculated energy difference
240 + in the presence and absence of PME was applied to the previous results
241 + in order to predict changes in the free energy landscape.
242 +
243   \section{Results and discussion}
244 +
245 + The free energy of proton ordered Ice-{\it i} was calculated and
246 + compared with the free energies of proton ordered variants of the
247 + experimentally observed low-density ice polymorphs, $I_h$ and $I_c$,
248 + as well as the higher density ice B, observed by B\`{a}ez and Clancy
249 + and thought to be the minimum free energy structure for the SPC/E
250 + model at ambient conditions (Table \ref{freeEnergy}).\cite{Baez95b}
251 + Ice XI, the experimentally observed proton ordered variant of ice
252 + $I_h$, was investigated initially, but it was found not to be as
253 + stable as antiferroelectric variants of proton ordered or even proton
254 + disordered ice$I_h$.\cite{Davidson84} The proton ordered variant of
255 + ice $I_h$ used here is a simple antiferroelectric version that has an
256 + 8 molecule unit cell. The crystals contained 648 or 1728 molecules for
257 + ice B, 1024 or 1280 molecules for ice $I_h$, 1000 molecules for ice
258 + $I_c$, or 1024 molecules for Ice-{\it i}. The larger crystal sizes
259 + were necessary for simulations involving larger cutoff values.
260  
261 + \begin{table*}
262 + \begin{minipage}{\linewidth}
263 + \renewcommand{\thefootnote}{\thempfootnote}
264 + \begin{center}
265 + \caption{Calculated free energies for several ice polymorphs with a
266 + variety of common water models. All calculations used a cutoff radius
267 + of 9 \AA\ and were performed at 200 K and $\sim$1 atm. Units are
268 + kcal/mol. *Ice $I_c$ is unstable at 200 K using SSD/RF.}
269 + \begin{tabular}{ l  c  c  c  c }
270 + \hline \\[-7mm]
271 + \ \quad \ Water Model\ \ & \ \quad \ \ \ \ $I_h$ \ \ & \ \quad \ \ \ \ $I_c$ \ \  & \ \quad \ \ \ \ B \ \  & \ \quad \ \ \ Ice-{\it i} \ \quad \ \\
272 + \hline \\[-3mm]
273 + \ \quad \ TIP3P  & \ \quad \ -11.41 & \ \quad \ -11.23 & \ \quad \ -11.82 & \quad -12.30\\
274 + \ \quad \ TIP4P  & \ \quad \ -11.84 & \ \quad \ -12.04 & \ \quad \ -12.08 & \quad -12.33\\
275 + \ \quad \ TIP5P  & \ \quad \ -11.85 & \ \quad \ -11.86 & \ \quad \ -11.96 & \quad -12.29\\
276 + \ \quad \ SPC/E  & \ \quad \ -12.67 & \ \quad \ -12.96 & \ \quad \ -13.25 & \quad -13.55\\
277 + \ \quad \ SSD/E  & \ \quad \ -11.27 & \ \quad \ -11.19 & \ \quad \ -12.09 & \quad -12.54\\
278 + \ \quad \ SSD/RF & \ \quad \ -11.51 & \ \quad \ NA* & \ \quad \ -12.08 & \quad -12.29\\
279 + \end{tabular}
280 + \label{freeEnergy}
281 + \end{center}
282 + \end{minipage}
283 + \end{table*}
284 +
285 + The free energy values computed for the studied polymorphs indicate
286 + that Ice-{\it i} is the most stable state for all of the common water
287 + models studied. With the free energy at these state points, the
288 + temperature and pressure dependence of the free energy was used to
289 + project to other state points and build phase diagrams. Figures
290 + \ref{tp3phasedia} and \ref{ssdrfphasedia} are example diagrams built
291 + from the free energy results. All other models have similar structure,
292 + only the crossing points between these phases exist at different
293 + temperatures and pressures. It is interesting to note that ice $I$
294 + does not exist in either cubic or hexagonal form in any of the phase
295 + diagrams for any of the models. For purposes of this study, ice B is
296 + representative of the dense ice polymorphs. A recent study by Sanz
297 + {\it et al.} goes into detail on the phase diagrams for SPC/E and
298 + TIP4P in the high pressure regime.\cite{Sanz04}
299 + \begin{figure}
300 + \includegraphics[width=\linewidth]{tp3PhaseDia.eps}
301 + \caption{Phase diagram for the TIP3P water model in the low pressure
302 + regime. The displayed $T_m$ and $T_b$ values are good predictions of
303 + the experimental values; however, the solid phases shown are not the
304 + experimentally observed forms. Both cubic and hexagonal ice $I$ are
305 + higher in energy and don't appear in the phase diagram.}
306 + \label{tp3phasedia}
307 + \end{figure}
308 + \begin{figure}
309 + \includegraphics[width=\linewidth]{ssdrfPhaseDia.eps}
310 + \caption{Phase diagram for the SSD/RF water model in the low pressure
311 + regime. Calculations producing these results were done under an
312 + applied reaction field. It is interesting to note that this
313 + computationally efficient model (over 3 times more efficient than
314 + TIP3P) exhibits phase behavior similar to the less computationally
315 + conservative charge based models.}
316 + \label{ssdrfphasedia}
317 + \end{figure}
318 +
319 + \begin{table*}
320 + \begin{minipage}{\linewidth}
321 + \renewcommand{\thefootnote}{\thempfootnote}
322 + \begin{center}
323 + \caption{Melting ($T_m$), boiling ($T_b$), and sublimation ($T_s$)
324 + temperatures of several common water models compared with experiment.}
325 + \begin{tabular}{ l  c  c  c  c  c  c  c }
326 + \hline \\[-7mm]
327 + \ \ Equilibria Point\ \ & \ \ \ \ \ TIP3P \ \ & \ \ \ \ \ TIP4P \ \ & \ \quad \ \ \ \ TIP5P \ \ & \ \ \ \ \ SPC/E \ \ & \ \ \ \ \ SSD/E \ \ & \ \ \ \ \ SSD/RF \ \ & \ \ \ \ \ Exp. \ \ \\
328 + \hline \\[-3mm]
329 + \ \ $T_m$ (K)  & \ \ 269 & \ \ 265 & \ \ 271 &  297 & \ \ - & \ \ 278 & \ \ 273\\
330 + \ \ $T_b$ (K)  & \ \ 357 & \ \ 354 & \ \ 337 &  396 & \ \ - & \ \ 349 & \ \ 373\\
331 + \ \ $T_s$ (K)  & \ \ - & \ \ - & \ \ - &  - & \ \ 355 & \ \ - & \ \ -\\
332 + \end{tabular}
333 + \label{meltandboil}
334 + \end{center}
335 + \end{minipage}
336 + \end{table*}
337 +
338 + Table \ref{meltandboil} lists the melting and boiling temperatures
339 + calculated from this work. Surprisingly, most of these models have
340 + melting points that compare quite favorably with experiment. The
341 + unfortunate aspect of this result is that this phase change occurs
342 + between Ice-{\it i} and the liquid state rather than ice $I_h$ and the
343 + liquid state. These results are actually not contrary to previous
344 + studies in the literature. Earlier free energy studies of ice $I$
345 + using TIP4P predict a $T_m$ ranging from 214 to 238 K (differences
346 + being attributed to choice of interaction truncation and different
347 + ordered and disordered molecular arrangements). If the presence of ice
348 + B and Ice-{\it i} were omitted, a $T_m$ value around 210 K would be
349 + predicted from this work. However, the $T_m$ from Ice-{\it i} is
350 + calculated at 265 K, significantly higher in temperature than the
351 + previous studies. Also of interest in these results is that SSD/E does
352 + not exhibit a melting point at 1 atm, but it shows a sublimation point
353 + at 355 K. This is due to the significant stability of Ice-{\it i} over
354 + all other polymorphs for this particular model under these
355 + conditions. While troubling, this behavior turned out to be
356 + advantageous in that it facilitated the spontaneous crystallization of
357 + Ice-{\it i}. These observations provide a warning that simulations of
358 + SSD/E as a ``liquid'' near 300 K are actually metastable and run the
359 + risk of spontaneous crystallization. However, this risk changes when
360 + applying a longer cutoff.
361 +
362 + \begin{figure}
363 + \includegraphics[width=\linewidth]{cutoffChange.eps}
364 + \caption{Free energy as a function of cutoff radius for (A) SSD/E, (B)
365 + TIP3P, and (C) SSD/RF. Data points omitted include SSD/E: $I_c$ 12
366 + \AA\, TIP3P: $I_c$ 12 \AA\ and B 12 \AA\, and SSD/RF: $I_c$ 9
367 + \AA\. These crystals are unstable at 200 K and rapidly convert into a
368 + liquid. The connecting lines are qualitative visual aid.}
369 + \label{incCutoff}
370 + \end{figure}
371 +
372 + Increasing the cutoff radius in simulations of the more
373 + computationally efficient water models was done in order to evaluate
374 + the trend in free energy values when moving to systems that do not
375 + involve potential truncation. As seen in Fig. \ref{incCutoff}, the
376 + free energy of all the ice polymorphs show a substantial dependence on
377 + cutoff radius. In general, there is a narrowing of the free energy
378 + differences while moving to greater cutoff radius. Interestingly, by
379 + increasing the cutoff radius, the free energy gap was narrowed enough
380 + in the SSD/E model that the liquid state is preferred under standard
381 + simulation conditions (298 K and 1 atm). Thus, it is recommended that
382 + simulations using this model choose interaction truncation radii
383 + greater than 9 \AA\. This narrowing trend is much more subtle in the
384 + case of SSD/RF, indicating that the free energies calculated with a
385 + reaction field present provide a more accurate picture of the free
386 + energy landscape in the absence of potential truncation.
387 +
388 + To further study the changes resulting to the inclusion of a
389 + long-range interaction correction, the effect of an Ewald summation
390 + was estimated by applying the potential energy difference do to its
391 + inclusion in systems in the presence and absence of the
392 + correction. This was accomplished by calculation of the potential
393 + energy of identical crystals with and without PME using TINKER. The
394 + free energies for the investigated polymorphs using the TIP3P and
395 + SPC/E water models are shown in Table \ref{pmeShift}. TIP4P and TIP5P
396 + are not fully supported in TINKER, so the results for these models
397 + could not be estimated. The same trend pointed out through increase of
398 + cutoff radius is observed in these PME results. Ice-{\it i} is the
399 + preferred polymorph at ambient conditions for both the TIP3P and SPC/E
400 + water models; however, there is a narrowing of the free energy
401 + differences between the various solid forms. In the case of SPC/E this
402 + narrowing is significant enough that it becomes less clear cut that
403 + Ice-{\it i} is the most stable polymorph, and is possibly metastable
404 + with respect to ice B and possibly ice $I_c$. However, these results
405 + do not significantly alter the finding that the Ice-{\it i} polymorph
406 + is a stable crystal structure that should be considered when studying
407 + the phase behavior of water models.
408 +
409 + \begin{table*}
410 + \begin{minipage}{\linewidth}
411 + \renewcommand{\thefootnote}{\thempfootnote}
412 + \begin{center}
413 + \caption{The free energy of the studied ice polymorphs after applying
414 + the energy difference attributed to the inclusion of the PME
415 + long-range interaction correction. Units are kcal/mol.}
416 + \begin{tabular}{ l  c  c  c  c }
417 + \hline \\[-7mm]
418 + \ \ Water Model \ \ & \ \ \ \ \ $I_h$ \ \ & \ \ \ \ \ $I_c$ \ \ & \ \quad \ \ \ \ B \ \ & \ \ \ \ \ Ice-{\it i} \ \ \\
419 + \hline \\[-3mm]
420 + \ \ TIP3P  & \ \ -11.53 & \ \ -11.24 & \ \ -11.51 & \ \ -11.67\\
421 + \ \ SPC/E  & \ \ -12.77 & \ \ -12.92 & \ \ -12.96 & \ \ -13.02\\
422 + \end{tabular}
423 + \label{pmeShift}
424 + \end{center}
425 + \end{minipage}
426 + \end{table*}
427 +
428   \section{Conclusions}
429  
430 + The free energy for proton ordered variants of hexagonal and cubic ice
431 + $I$, ice B, and recently discovered Ice-{\it i} where calculated under
432 + standard conditions for several common water models via thermodynamic
433 + integration. All the water models studied show Ice-{\it i} to be the
434 + minimum free energy crystal structure in the with a 9 \AA\ switching
435 + function cutoff. Calculated melting and boiling points show
436 + surprisingly good agreement with the experimental values; however, the
437 + solid phase at 1 atm is Ice-{\it i}, not ice $I_h$. The effect of
438 + interaction truncation was investigated through variation of the
439 + cutoff radius, use of a reaction field parameterized model, and
440 + estimation of the results in the presence of the Ewald summation
441 + correction. Interaction truncation has a significant effect on the
442 + computed free energy values, and may significantly alter the free
443 + energy landscape for the more complex multipoint water models. Despite
444 + these effects, these results show Ice-{\it i} to be an important ice
445 + polymorph that should be considered in simulation studies.
446 +
447 + Due to this relative stability of Ice-{\it i} in all manner of
448 + investigated simulation examples, the question arises as to possible
449 + experimental observation of this polymorph. The rather extensive past
450 + and current experimental investigation of water in the low pressure
451 + regime leads the authors to be hesitant in ascribing relevance outside
452 + of computational models, hence the descriptive name presented. That
453 + being said, there are certain experimental conditions that would
454 + provide the most ideal situation for possible observation. These
455 + include the negative pressure or stretched solid regime, small
456 + clusters in vacuum deposition environments, and in clathrate
457 + structures involving small non-polar molecules.
458 +
459   \section{Acknowledgments}
460   Support for this project was provided by the National Science
461   Foundation under grant CHE-0134881. Computation time was provided by
462 < the Notre Dame Bunch-of-Boxes (B.o.B) computer cluster under NSF grant
463 < DMR-0079647.
462 > the Notre Dame High Performance Computing Cluster and the Notre Dame
463 > Bunch-of-Boxes (B.o.B) computer cluster (NSF grant DMR-0079647).
464  
465   \newpage
466  

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