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More results and discussion

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1 %\documentclass[prb,aps,twocolumn,tabularx]{revtex4}
2 \documentclass[preprint,aps,endfloats]{revtex4}
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20
21 \begin{document}
22
23 \title{A Free Energy Study of Low Temperature and Anomolous Ice}
24
25 \author{Christopher J. Fennell and J. Daniel Gezelter{\thefootnote}
26 \footnote[1]{Corresponding author. \ Electronic mail: gezelter@nd.edu}}
27
28 \address{Department of Chemistry and Biochemistry\\ University of Notre Dame\\
29 Notre Dame, Indiana 46556}
30
31 \date{\today}
32
33 %\maketitle
34 %\doublespacing
35
36 \begin{abstract}
37 \end{abstract}
38
39 \maketitle
40
41 \newpage
42
43 %\narrowtext
44
45 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
46 % BODY OF TEXT
47 %%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%%
48
49 \section{Introduction}
50
51 \section{Methods}
52
53 Canonical ensemble (NVT) molecular dynamics calculations were
54 performed using the OOPSE (Object-Oriented Parallel Simulation Engine)
55 molecular mechanics package. All molecules were treated as rigid
56 bodies, with orientational motion propogated using the symplectic DLM
57 integration method. Details about the implementation of these
58 techniques can be found in a recent publication.\cite{Meineke05}
59
60 Thermodynamic integration was utilized to calculate the free energy of
61 several ice crystals at 200 K using the TIP3P, TIP4P, TIP5P, SPC/E,
62 SSD/RF, and SSD/E water models. Liquid state free energies at 300 and
63 400 K for all of these water models were also determined using this
64 same technique, in order to determine melting points and generate
65 phase diagrams. All simulations were carried out at densities
66 resulting in a pressure of approximately 1 atm at their respective
67 temperatures.
68
69 For the thermodynamic integration of molecular crystals, the Einstein
70 Crystal is chosen as the reference state that the system is converted
71 to over the course of the simulation. In an Einstein Crystal, the
72 molecules are harmonically restrained at their ideal lattice locations
73 and orientations. The partition function for a molecular crystal
74 restrained in this fashion has been evaluated, and the Helmholtz Free
75 Energy ({\it A}) is given by
76 \begin{eqnarray}
77 A = E_m\ -\ kT\ln \left (\frac{kT}{h\nu}\right )^3&-&kT\ln \left
78 [\pi^\frac{1}{2}\left (\frac{8\pi^2I_\mathrm{A}kT}{h^2}\right
79 )^\frac{1}{2}\left (\frac{8\pi^2I_\mathrm{B}kT}{h^2}\right
80 )^\frac{1}{2}\left (\frac{8\pi^2I_\mathrm{C}kT}{h^2}\right
81 )^\frac{1}{2}\right ] \nonumber \\ &-& kT\ln \left [\frac{kT}{2(\pi
82 K_\omega K_\theta)^{\frac{1}{2}}}\exp\left
83 (-\frac{kT}{2K_\theta}\right)\int_0^{\left (\frac{kT}{2K_\theta}\right
84 )^\frac{1}{2}}\exp(t^2)\mathrm{d}t\right ],
85 \label{ecFreeEnergy}
86 \end{eqnarray}
87 where $2\pi\nu = (K_\mathrm{v}/m)^{1/2}$.\cite{Baez95a} In equation
88 \ref{ecFreeEnergy}, $K_\mathrm{v}$, $K_\mathrm{\theta}$, and
89 $K_\mathrm{\omega}$ are the spring constants restraining translational
90 motion and deflection of and rotation around the principle axis of the
91 molecule respectively (Fig. \ref{waterSpring}), and $E_m$ is the
92 minimum potential energy of the ideal crystal. In the case of
93 molecular liquids, the ideal vapor is chosen as the target reference
94 state.
95 \begin{figure}
96 \includegraphics[scale=1.0]{rotSpring.eps}
97 \caption{Possible orientational motions for a restrained molecule.
98 $\theta$ angles correspond to displacement from the body-frame {\it
99 z}-axis, while $\omega$ angles correspond to rotation about the
100 body-frame {\it z}-axis. $K_\theta$ and $K_\omega$ are spring
101 constants for the harmonic springs restraining motion in the $\theta$
102 and $\omega$ directions.}
103 \label{waterSpring}
104 \end{figure}
105
106 Charge, dipole, and Lennard-Jones interactions were modified by a
107 cubic switching between 100\% and 85\% of the cutoff value (9 \AA ). By
108 applying this function, these interactions are smoothly truncated,
109 thereby avoiding poor energy conserving dynamics resulting from
110 harsher truncation schemes. The effect of a long-range correction was
111 also investigated on select model systems in a variety of manners. For
112 the SSD/RF model, a reaction field with a fixed dielectric constant of
113 80 was applied in all simulations.\cite{Onsager36} For a series of the
114 least computationally expensive models (SSD/E, SSD/RF, and TIP3P),
115 simulations were performed with longer cutoffs of 12 and 15 \AA\ to
116 compare with the 9 \AA\ cutoff results. Finally, results from the use
117 of an Ewald summation were estimated for TIP3P and SPC/E by performing
118 calculations with Particle-Mesh Ewald (PME) in the TINKER molecular
119 mechanics software package. TINKER was chosen because it can also
120 propogate the motion of rigid-bodies, and provides the most direct
121 comparison to the results from OOPSE. The calculated energy difference
122 in the presence and absence of PME was applied to the previous results
123 in order to predict changes in the free energy landscape.
124
125 \section{Results and discussion}
126
127 The free energy of proton ordered Ice-{\it i} was calculated and
128 compared with the free energies of proton ordered variants of the
129 experimentally observed low-density ice polymorphs, $I_h$ and $I_c$,
130 as well as the higher density ice B, observed by B\`{a}ez and Clancy
131 and thought to be the minimum free energy structure for the SPC/E
132 model at ambient conditions (Table \ref{freeEnergy}).\cite{Baez95b}
133 Ice XI, the experimentally observed proton ordered variant of ice
134 $I_h$, was investigated initially, but it was found not to be as
135 stable as antiferroelectric variants of proton ordered or even proton
136 disordered ice$I_h$.\cite{Davidson84} The proton ordered variant of
137 ice $I_h$ used here is a simple antiferroelectric version that has an
138 8 molecule unit cell. The crystals contained 648 or 1728 molecules for
139 ice B, 1024 or 1280 molecules for ice $I_h$, 1000 molecules for ice
140 $I_c$, or 1024 molecules for Ice-{\it i}. The larger crystal sizes
141 were necessary for simulations involving larger cutoff values.
142
143 \begin{table*}
144 \begin{minipage}{\linewidth}
145 \renewcommand{\thefootnote}{\thempfootnote}
146 \begin{center}
147 \caption{Calculated free energies for several ice polymorphs with a
148 variety of common water models. All calculations used a cutoff radius
149 of 9 \AA\ and were performed at 200 K and $\sim$1 atm. Units are
150 kcal/mol. *Ice $I_c$ is unstable at 200 K using SSD/RF.}
151 \begin{tabular}{ l c c c c }
152 \hline \\[-7mm]
153 \ \quad \ Water Model\ \ & \ \quad \ \ \ \ $I_h$ \ \ & \ \quad \ \ \ \ $I_c$ \ \ & \ \quad \ \ \ \ B \ \ & \ \quad \ \ \ Ice-{\it i} \ \quad \ \\
154 \hline \\[-3mm]
155 \ \quad \ TIP3P & \ \quad \ -11.41 & \ \quad \ -11.23 & \ \quad \ -11.82 & \quad -12.30\\
156 \ \quad \ TIP4P & \ \quad \ -11.84 & \ \quad \ -12.04 & \ \quad \ -12.08 & \quad -12.33\\
157 \ \quad \ TIP5P & \ \quad \ -11.85 & \ \quad \ -11.86 & \ \quad \ -11.96 & \quad -12.29\\
158 \ \quad \ SPC/E & \ \quad \ -12.67 & \ \quad \ -12.96 & \ \quad \ -13.25 & \quad -13.55\\
159 \ \quad \ SSD/E & \ \quad \ -11.27 & \ \quad \ -11.19 & \ \quad \ -12.09 & \quad -12.54\\
160 \ \quad \ SSD/RF & \ \quad \ -11.51 & \ \quad \ NA* & \ \quad \ -12.08 & \quad -12.29\\
161 \end{tabular}
162 \label{freeEnergy}
163 \end{center}
164 \end{minipage}
165 \end{table*}
166
167 The free energy values computed for the studied polymorphs indicate
168 that Ice-{\it i} is the most stable state for all of the common water
169 models studied. With the free energy at these state points, the
170 temperature and pressure dependence of the free energy was used to
171 project to other state points and build phase diagrams. Figures
172 \ref{tp3phasedia} and \ref{ssdrfphasedia} are example diagrams built
173 from the free energy results. All other models have similar structure,
174 only the crossing points between these phases exist at different
175 temperatures and pressures. It is interesting to note that ice $I$
176 does not exist in either cubic or hexagonal form in any of the phase
177 diagrams for any of the models. For purposes of this study, ice B is
178 representative of the dense ice polymorphs. A recent study by Sanz
179 {\it et al.} goes into detail on the phase diagrams for SPC/E and
180 TIP4P in the high pressure regime.\cite{Sanz04}
181 \begin{figure}
182 \includegraphics[width=\linewidth]{tp3PhaseDia.eps}
183 \caption{Phase diagram for the TIP3P water model in the low pressure
184 regime. The displayed $T_m$ and $T_b$ values are good predictions of
185 the experimental values; however, the solid phases shown are not the
186 experimentally observed forms. Both cubic and hexagonal ice $I$ are
187 higher in energy and don't appear in the phase diagram.}
188 \label{tp3phasedia}
189 \end{figure}
190 \begin{figure}
191 \includegraphics[width=\linewidth]{ssdrfPhaseDia.eps}
192 \caption{Phase diagram for the SSD/RF water model in the low pressure
193 regime. Calculations producing these results were done under an
194 applied reaction field. It is interesting to note that this
195 computationally efficient model (over 3 times more efficient than
196 TIP3P) exhibits phase behavior similar to the less computationally
197 conservative charge based models.}
198 \label{ssdrfphasedia}
199 \end{figure}
200
201 \begin{table*}
202 \begin{minipage}{\linewidth}
203 \renewcommand{\thefootnote}{\thempfootnote}
204 \begin{center}
205 \caption{Melting ($T_m$), boiling ($T_b$), and sublimation ($T_s$)
206 temperatures of several common water models compared with experiment.}
207 \begin{tabular}{ l c c c c c c c }
208 \hline \\[-7mm]
209 \ \ Equilibria Point\ \ & \ \ \ \ \ TIP3P \ \ & \ \ \ \ \ TIP4P \ \ & \ \quad \ \ \ \ TIP5P \ \ & \ \ \ \ \ SPC/E \ \ & \ \ \ \ \ SSD/E \ \ & \ \ \ \ \ SSD/RF \ \ & \ \ \ \ \ Exp. \ \ \\
210 \hline \\[-3mm]
211 \ \ $T_m$ (K) & \ \ 269 & \ \ 265 & \ \ 271 & 297 & \ \ - & \ \ 278 & \ \ 273\\
212 \ \ $T_b$ (K) & \ \ 357 & \ \ 354 & \ \ 337 & 396 & \ \ - & \ \ 349 & \ \ 373\\
213 \ \ $T_s$ (K) & \ \ - & \ \ - & \ \ - & - & \ \ 355 & \ \ - & \ \ -\\
214 \end{tabular}
215 \label{meltandboil}
216 \end{center}
217 \end{minipage}
218 \end{table*}
219
220 Table \ref{meltandboil} lists the melting and boiling temperatures
221 calculated from this work. Surprisingly, most of these models have
222 melting points that compare quite favorably with experiment. The
223 unfortunate aspect of this result is that this phase change occurs
224 between Ice-{\it i} and the liquid state rather than ice $I_h$ and the
225 liquid state. These results are actually not contrary to previous
226 studies in the literature. Earlier free energy studies of ice $I$
227 using TIP4P predict a $T_m$ ranging from 214 to 238 K (differences
228 being attributed to choice of interaction truncation and different
229 ordered and disordered molecular arrangements). If the presence of ice
230 B and Ice-{\it i} were omitted, a $T_m$ value around 210 K would be
231 predicted from this work. However, the $T_m$ from Ice-{\it i} is
232 calculated at 265 K, significantly higher in temperature than the
233 previous studies. Also of interest in these results is that SSD/E does
234 not exhibit a melting point at 1 atm, but it shows a sublimation point
235 at 355 K. This is due to the significant stability of Ice-{\it i} over
236 all other polymorphs for this particular model under these
237 conditions. While troubling, this behavior turned out to be
238 advantagious in that it facilitated the spontaneous crystallization of
239 Ice-{\it i}. These observations provide a warning that simulations of
240 SSD/E as a ``liquid'' near 300 K are actually metastable and run the
241 risk of spontaneous crystallization. However, this risk changes when
242 applying a longer cutoff.
243
244 Increasing the cutoff radius in simulations of the more
245 computationally efficient water models was done in order to evaluate
246 the trend in free energy values when moving to systems that do not
247 involve potential truncation. As seen in Fig. \ref{incCutoff}, the
248 free energy of all the ice polymorphs show a substantial dependence on
249 cutoff radius. In general, there is a narrowing of the free energy
250 differences while moving to greater cutoff radius. This trend is much
251 more subtle in the case of SSD/RF, indicating that the free energies
252 calculated with a reaction field present provide a more accurate
253 picture of the free energy landscape in the absence of potential
254 truncation.
255
256 To further study the changes resulting to the inclusion of a
257 long-range interaction correction, the effect of an Ewald summation
258 was estimated by applying the potential energy difference do to its
259 inclusion in systems in the presence and absence of the
260 correction. This was accomplished by calculation of the potential
261 energy of identical crystals with and without PME using TINKER. The
262 free energies for the investigated polymorphs using the TIP3P and
263 SPC/E water models are shown in Table \ref{pmeShift}. TIP4P and TIP5P
264 are not fully supported in TINKER, so the results for these models
265 could not be estimated. The same trend pointed out through increase of
266 cutoff radius is observed in these results. Ice-{\it i} is the
267 preferred polymorph at ambient conditions for both the TIP3P and SPC/E
268 water models; however, there is a narrowing of the free energy
269 differences between the various solid forms. In the case of SPC/E this
270 narrowing is significant enough that it becomes less clear cut that
271 Ice-{\it i} is the most stable polymorph, and is possibly metastable
272 with respect to ice B and possibly ice $I_c$. However, these results
273 do not significantly alter the finding that the Ice-{\it i} polymorph
274 is a stable crystal structure that should be considered when studying
275 the phase behavior of water models.
276
277 \begin{table*}
278 \begin{minipage}{\linewidth}
279 \renewcommand{\thefootnote}{\thempfootnote}
280 \begin{center}
281 \caption{The free energy of the studied ice polymorphs after applying the energy difference attributed to the inclusion of the PME long-range interaction correction. Units are kcal/mol.}
282 \begin{tabular}{ l c c c c }
283 \hline \\[-7mm]
284 \ \ Water Model \ \ & \ \ \ \ \ $I_h$ \ \ & \ \ \ \ \ $I_c$ \ \ & \ \quad \ \ \ \ B \ \ & \ \ \ \ \ Ice-{\it i} \ \ \\
285 \hline \\[-3mm]
286 \ \ TIP3P & \ \ -11.53 & \ \ -11.24 & \ \ -11.51 & \ \ -11.67\\
287 \ \ SPC/E & \ \ -12.77 & \ \ -12.92 & \ \ -12.96 & \ \ -13.02\\
288 \end{tabular}
289 \label{pmeShift}
290 \end{center}
291 \end{minipage}
292 \end{table*}
293
294 \section{Conclusions}
295
296 \section{Acknowledgments}
297 Support for this project was provided by the National Science
298 Foundation under grant CHE-0134881. Computation time was provided by
299 the Notre Dame Bunch-of-Boxes (B.o.B) computer cluster under NSF grant
300 DMR-0079647.
301
302 \newpage
303
304 \bibliographystyle{jcp}
305 \bibliography{iceiPaper}
306
307
308 \end{document}