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# Line 8 | Line 8 | available, it is only natural to compare the models un
8   These models have been used to investigate important physical
9   phenomena like phase transitions and the hydrophobic
10   effect.\cite{Yamada02,Marrink94,Gallagher03} With the choice of models
11 < available, it is only natural to compare the models under interesting
11 > available, it is only natural to compare them under interesting
12   thermodynamic conditions in an attempt to clarify the limitations of
13 < each of the models.\cite{Jorgensen83,Jorgensen98b,Baez94,Mahoney01}
14 < Two important property to quantify are the Gibbs and Helmholtz free
15 < energies, particularly for the solid forms of water, as these predict
16 < the thermodynamic stability of the various phases. Water has a
13 > each.\cite{Jorgensen83,Jorgensen98b,Baez94,Mahoney01} Two important
14 > property to quantify are the Gibbs and Helmholtz free energies,
15 > particularly for the solid forms of water, as these predict the
16 > thermodynamic stability of the various phases. Water has a
17   particularly rich phase diagram and takes on a number of different and
18   stable crystalline structures as the temperature and pressure are
19   varied. This complexity makes it a challenging task to investigate the
# Line 34 | Line 34 | pressure of 1 atm. After melting from ice I$_\textrm{h
34  
35   While performing a series of melting simulations on an early iteration
36   of SSD/E, we observed several recrystallization events at a constant
37 < pressure of 1 atm. After melting from ice I$_\textrm{h}$ at 235K, two
38 < of five systems recrystallized near 245K. Crystallization events are
37 > pressure of 1 atm. After melting from ice I$_\textrm{h}$ at 235~K, two
38 > of five systems recrystallized near 245~K. Crystallization events are
39   interesting in and of themselves;\cite{Matsumoto02,Yamada02} however,
40   the crystal structure extracted from these systems is different from
41   any previously observed ice polymorphs in experiment or
# Line 51 | Line 51 | are typically greater than 6.3\AA\ in diameter (see fi
51   I$_\textrm{h}$; however, the interlocking of these subunits appears to
52   provide significant stabilization to the overall crystal. The
53   arrangement of these tetramers results in open octagonal cavities that
54 < are typically greater than 6.3\AA\ in diameter (see figure
54 > are typically greater than 6.3~\AA\ in diameter (see figure
55   \ref{fig:protOrder}). This open structure leads to crystals that are
56 < typically 0.07 g/cm$^3$ less dense than ice I$_\textrm{h}$.
56 > typically 0.07~g/cm$^3$ less dense than ice I$_\textrm{h}$.
57  
58   \begin{figure}
59   \includegraphics[width=\linewidth]{./figures/unitCell.pdf}
# Line 85 | Line 85 | structure observed by B\`{a}ez and Clancy in free ener
85   thermodynamic integration and compared to the free energies of ice
86   I$_\textrm{c}$ and ice I$_\textrm{h}$ (the common low-density ice
87   polymorphs) and ice B (a higher density, but very stable crystal
88 < structure observed by B\`{a}ez and Clancy in free energy studies of
88 > structure observed by B\'{a}ez and Clancy in free energy studies of
89   SPC/E).\cite{Baez95b} This work includes results for the water model
90   from which Ice-{\it i} was crystallized (SSD/E) in addition to several
91   common water models (TIP3P, TIP4P, TIP5P, and SPC/E) and a reaction
# Line 105 | Line 105 | isobaric-isothermal ({\it NPT}) simulations performed
105   performed using the OOPSE molecular mechanics package.\cite{Meineke05}
106   The densities chosen for the simulations were taken from
107   isobaric-isothermal ({\it NPT}) simulations performed at 1 atm and
108 < 200K. Each model (and each crystal structure) was allowed to relax for
109 < 300ps in the {\it NPT} ensemble before averaging the density to obtain
108 > 200~K. Each model (and each crystal structure) was allowed to relax for
109 > 300~ps in the {\it NPT} ensemble before averaging the density to obtain
110   the volumes for the {\it NVT} simulations.All molecules were treated
111   as rigid bodies, with orientational motion propagated using the
112   symplectic DLM integration method described in section
# Line 159 | Line 159 | ice crystal at 200 K.  For these studies, $K_\mathrm{v
159   of and rotation around the principle axis of the molecule
160   respectively.  These spring constants are typically calculated from
161   the mean-square displacements of water molecules in an unrestrained
162 < ice crystal at 200 K.  For these studies, $K_\mathrm{v} = 4.29$ kcal
163 < mol$^{-1}$ \AA$^{-2}$, $K_\theta\ = 13.88$ kcal mol$^{-1}$ rad$^{-2}$,
164 < and $K_\omega\ = 17.75$ kcal mol$^{-1}$ rad$^{-2}$.  It is clear from
165 < Fig. \ref{fig:waterSpring} that the values of $\theta$ range from $0$ to
166 < $\pi$, while $\omega$ ranges from $-\pi$ to $\pi$.  The partition
162 > ice crystal at 200~K.  For these studies, $K_\mathrm{v} =
163 > 4.29$~kcal~mol$^{-1}$~\AA$^{-2}$, $K_\theta\ =
164 > 13.88$~kcal~mol$^{-1}$~rad$^{-2}$, and $K_\omega\ =
165 > 17.75$~kcal~mol$^{-1}$~rad$^{-2}$.  It is clear from
166 > Fig. \ref{fig:waterSpring} that the values of $\theta$ range from $0$
167 > to $\pi$, while $\omega$ ranges from $-\pi$ to $\pi$.  The partition
168   function for a molecular crystal restrained in this fashion can be
169   evaluated analytically, and the Helmholtz Free Energy ({\it A}) is
170   given by
# Line 184 | Line 185 | Einstein crystal reference stat is somewhat arbitrary.
185   \end{equation}
186   where $2\pi\nu = (K_\mathrm{v}/m)^{1/2}$, and $E_m$ is the minimum
187   potential energy of the ideal crystal.\cite{Baez95a} The choice of an
188 < Einstein crystal reference stat is somewhat arbitrary. Any ideal
188 > Einstein crystal reference state is somewhat arbitrary. Any ideal
189   system for which the partition function is known exactly could be used
190   as a reference point as long as the system does not undergo a phase
191   transition during the integration path between the real and ideal
192   systems.  Nada and van der Eerden have shown that the use of different
193 < force constants in the Einstein crystal doesn not affect the total
193 > force constants in the Einstein crystal does not affect the total
194   free energy, and Gao {\it et al.} have shown that free energies
195   computed with the Debye crystal reference state differ from the
196 < Einstein crystal by only a few tenths of a kJ
197 < mol$^{-1}$.\cite{Nada03,Gao00} These free energy differences can lead
198 < to some uncertainty in the computed melting point of the solids.
196 > Einstein crystal by only a few tenths of a
197 > kJ~mol$^{-1}$.\cite{Nada03,Gao00} These free energy differences can
198 > lead to some uncertainty in the computed melting point of the solids.
199   \begin{figure}
200   \centering
201   \includegraphics[width=3.5in]{./figures/rotSpring.pdf}
# Line 230 | Line 231 | performed with longer cutoffs of 10.5, 12, 13.5, and 1
231   dielectric constant of 80 was applied in all
232   simulations.\cite{Onsager36} For a series of the least computationally
233   expensive models (SSD/E, SSD/RF, TIP3P, and SPC/E), simulations were
234 < performed with longer cutoffs of 10.5, 12, 13.5, and 15\AA\ to
235 < compare with the 9\AA\ cutoff results.  Finally, the effects of using
234 > performed with longer cutoffs of 10.5, 12, 13.5, and 15~\AA\ to
235 > compare with the 9~\AA\ cutoff results.  Finally, the effects of using
236   the Ewald summation were estimated for TIP3P and SPC/E by performing
237   single configuration Particle-Mesh Ewald (PME) calculations for each
238   of the ice polymorphs.\cite{Ponder87} The calculated energy difference
# Line 278 | Line 279 | TIP3P & -11.41(2) & -11.23(3) & -11.82(3) & -12.30(3)
279   \cmidrule(l){7-8}
280   & \multicolumn{5}{c}{(kcal mol$^{-1}$)} & \multicolumn{2}{c}{(K)}\\
281   \midrule
281 TIP3P & -11.41(2) & -11.23(3) & -11.82(3) & -12.30(3) & - & 269(7) & 357(4)\\
282 TIP4P & -11.84(3) & -12.04(2) & -12.08(3) & - & -12.33(3) & 262(6) & 354(4)\\
282   TIP5P & -11.85(3) & -11.86(2) & -11.96(2) & - & -12.29(2) & 266(7) & 337(4)\\
283 + TIP4P & -11.84(3) & -12.04(2) & -12.08(3) & - & -12.33(3) & 262(6) & 354(4)\\
284 + TIP3P & -11.41(2) & -11.23(3) & -11.82(3) & -12.30(3) & - & 269(7) & 357(4)\\
285   SPC/E & -12.87(2) & -13.05(2) & -13.26(3) & - & -13.55(2) & 299(6) & 396(4)\\
286   SSD/E & -11.27(2) & -11.19(4) & -12.09(2) & -12.54(2) & - & *355(4) & -\\
287   SSD/RF & -11.96(2) & -11.60(2) & -12.53(3) & -12.79(2) & - & 278(7) & 382(4)\\
# Line 312 | Line 313 | We note that all of the crystals investigated in this
313   \label{fig:ssdrfPhaseDia}
314   \end{figure}
315  
316 < We note that all of the crystals investigated in this study ar ideal
316 > We note that all of the crystals investigated in this study are ideal
317   proton-ordered antiferroelectric structures. All of the structures
318   obey the Bernal-Fowler rules and should be able to form stable
319   proton-{\it disordered} crystals which have the traditional
320 < $k_\textrm{B}$ln(3/2) residual entropy at 0K.\cite{Bernal33,Pauling35}
320 > $k_\textrm{B}$ln(3/2) residual entropy at 0~K.\cite{Bernal33,Pauling35}
321   Simulations of proton-disordered structures are relatively unstable
322   with all but the most expensive water models.\cite{Nada03} Our
323   simulations have therefore been performed with the ordered
# Line 327 | Line 328 | favorably with the experimental value of 273 K.  The u
328   of the disordered structures.\cite{Sanz04}
329  
330   Most of the water models have melting points that compare quite
331 < favorably with the experimental value of 273 K.  The unfortunate
331 > favorably with the experimental value of 273~K.  The unfortunate
332   aspect of this result is that this phase change occurs between
333   Ice-{\it i} and the liquid state rather than ice I$_h$ and the liquid
334   state.  These results do not contradict other studies.  Studies of ice
335 < I$_h$ using TIP4P predict a $T_m$ ranging from 191 to 238 K
335 > I$_h$ using TIP4P predict a $T_m$ ranging from 191 to 238~K
336   (differences being attributed to choice of interaction truncation and
337   different ordered and disordered molecular
338   arrangements).\cite{Nada03,Vlot99,Gao00,Sanz04} If the presence of ice
339 < B and Ice-{\it i} were omitted, a $T_\textrm{m}$ value around 200 K
339 > B and Ice-{\it i} were omitted, a $T_\textrm{m}$ value around 200~K
340   would be predicted from this work.  However, the $T_\textrm{m}$ from
341 < Ice-{\it i} is calculated to be 262 K, indicating that these
341 > Ice-{\it i} is calculated to be 262~K, indicating that these
342   simulation based structures ought to be included in studies probing
343   phase transitions with this model.  Also of interest in these results
344   is that SSD/E does not exhibit a melting point at 1 atm but does
345 < sublime at 355 K.  This is due to the significant stability of
345 > sublime at 355~K.  This is due to the significant stability of
346   Ice-{\it i} over all other polymorphs for this particular model under
347   these conditions.  While troubling, this behavior resulted in the
348   spontaneous crystallization of Ice-{\it i} which led us to investigate
349   this structure.  These observations provide a warning that simulations
350 < of SSD/E as a ``liquid'' near 300 K are actually metastable and run
350 > of SSD/E as a ``liquid'' near 300~K are actually metastable and run
351   the risk of spontaneous crystallization.  However, when a longer
352   cutoff radius is used, SSD/E prefers the liquid state under standard
353   temperature and pressure.
354  
355 < \section{Effects of Potential Trucation}
355 > \section{Effects of Potential Truncation}
356  
357   \begin{figure}
358   \includegraphics[width=\linewidth]{./figures/cutoffChange.pdf}
359   \caption{Free energy as a function of cutoff radius for SSD/E, TIP3P,
360   SPC/E, SSD/RF with a reaction field, and the TIP3P and SPC/E models
361   with an added Ewald correction term.  Error for the larger cutoff
362 < points is equivalent to that observed at 9.0\AA\ (see Table
362 > points is equivalent to that observed at 9.0~\AA\ (see Table
363   \ref{tab:freeEnergy}). Data for ice I$_\textrm{c}$ with TIP3P using
364 < both 12 and 13.5\AA\ cutoffs were omitted because the crystal was
365 < prone to distortion and melting at 200K.  Ice-$i^\prime$ is the
364 > both 12 and 13.5~\AA\ cutoffs were omitted because the crystal was
365 > prone to distortion and melting at 200~K.  Ice-$i^\prime$ is the
366   form of Ice-{\it i} used in the SPC/E simulations.}
367   \label{fig:incCutoff}
368   \end{figure}
369  
370   For the more computationally efficient water models, we have also
371 < investigated the effect of potential trunctaion on the computed free
371 > investigated the effect of potential truncation on the computed free
372   energies as a function of the cutoff radius.  As seen in
373   Fig. \ref{fig:incCutoff}, the free energies of the ice polymorphs with
374   water models lacking a long-range correction show significant cutoff
# Line 382 | Line 383 | Although TIP3P was paramaterized for use without the E
383   field cavity in this model, so small cutoff radii mimic bulk
384   calculations quite well under SSD/RF.
385  
386 < Although TIP3P was paramaterized for use without the Ewald summation,
386 > Although TIP3P was parametrized for use without the Ewald summation,
387   we have estimated the effect of this method for computing long-range
388   electrostatics for both TIP3P and SPC/E.  This was accomplished by
389   calculating the potential energy of identical crystals both with and
# Line 402 | Line 403 | influence the polymorph expressed upon crystallization
403  
404   \section{Expanded Results Using Damped Shifted Force Electrostatics}
405  
406 + In chapter \ref{chap:electrostatics}, we discussed in detail a
407 + pairwise method for handling electrostatics (shifted force, {\sc sf})
408 + that can be used as a simple and efficient replacement for the Ewald
409 + summation. Answering the question of the free energies of these ice
410 + polymorphs with varying water models would be an interesting
411 + application of this technique. To this end, we set up thermodynamic
412 + integrations of all of the previously discussed ice polymorphs using
413 + the {\sc sf} technique with a cutoff radius of 12~\AA\ and an $\alpha$
414 + of 0.2125~\AA . These calculations were performed on TIP5P-E and
415 + TIP4P-Ew (variants of the root models optimized for the Ewald
416 + summation) as well as SPC/E, SSD/RF, and TRED (see section
417 + \ref{sec:tredWater}).
418  
419 + \begin{table}
420 + \centering
421 + \caption{HELMHOLTZ FREE ENERGIES OF ICE POLYMORPHS USING THE DAMPED
422 + SHIFTED FORCE CORRECTION}
423 + \begin{tabular}{ lccccc }
424 + \toprule
425 + \toprule
426 + Model & I$_\textrm{h}$ & I$_\textrm{c}$ & B & Ice-$i$ & Ice-$i^\prime$ \\
427 + \cmidrule(lr){2-6}
428 + & \multicolumn{5}{c}{(kcal mol$^{-1}$)} \\
429 + \midrule
430 + TIP5P-E & -10.76(4) & -10.72(4) & & - & -10.68(4) \\
431 + TIP4P-Ew & & -11.77(3) & & - & -11.60(3) \\
432 + SPC/E & -12.98(3) & -11.60(3) & & - & -12.93(3) \\
433 + SSD/RF & -11.81(4) & -11.65(3) & & -12.41(4) & - \\
434 + TRED & -12.58(3) & -12.44(3) & & -13.09(4) & - \\
435 + \end{tabular}
436 + \label{tab:dampedFreeEnergy}
437 + \end{table}
438 +
439 +
440   \section{Conclusions}
441  
442   In this work, thermodynamic integration was used to determine the
443   absolute free energies of several ice polymorphs.  The new polymorph,
444   Ice-{\it i} was observed to be the stable crystalline state for {\it
445 < all} the water models when using a 9.0\AA\ cutoff.  However, the free
445 > all} the water models when using a 9.0~\AA\ cutoff.  However, the free
446   energy partially depends on simulation conditions (particularly on the
447   choice of long range correction method). Regardless, Ice-{\it i} was
448 < still observered to be a stable polymorph for all of the studied water
448 > still observed to be a stable polymorph for all of the studied water
449   models.
450  
451   So what is the preferred solid polymorph for simulated water?  As
# Line 447 | Line 481 | I$_\textrm{h}$ and I$_\textrm{c}$ plots) at 77K, and t
481   results, we have calculated the oxygen-oxygen pair correlation
482   function, $g_\textrm{OO}(r)$, and the structure factor, $S(\vec{q})$
483   for the two Ice-{\it i} variants (along with example ice
484 < I$_\textrm{h}$ and I$_\textrm{c}$ plots) at 77K, and they are shown in
484 > I$_\textrm{h}$ and I$_\textrm{c}$ plots) at 77~K, and they are shown in
485   figures \ref{fig:gofr} and \ref{fig:sofq} respectively.  It is
486   interesting to note that the structure factors for Ice-$i^\prime$ and
487   Ice-I$_c$ are quite similar.  The primary differences are small peaks
488 < at 1.125, 2.29, and 2.53\AA$^{-1}$, so particular attention to these
488 > at 1.125, 2.29, and 2.53~\AA$^{-1}$, so particular attention to these
489   regions would be needed to identify the new $i^\prime$ variant from
490   the I$_\textrm{c}$ polymorph.
491  
# Line 460 | Line 494 | model at 77 K.}
494   \includegraphics[width=\linewidth]{./figures/iceGofr.pdf}
495   \caption{Radial distribution functions of Ice-{\it i} and ice
496   I$_\textrm{c}$ calculated from from simulations of the SSD/RF water
497 < model at 77 K.}
497 > model at 77~K.}
498   \label{fig:gofr}
499   \end{figure}
500  
501   \begin{figure}
502   \includegraphics[width=\linewidth]{./figures/sofq.pdf}
503   \caption{Predicted structure factors for Ice-{\it i} and ice
504 < I$_\textrm{c}$ at 77 K.  The raw structure factors have been
505 < convoluted with a gaussian instrument function (0.075 \AA$^{-1}$
506 < width) to compensate for the trunction effects in our finite size
504 > I$_\textrm{c}$ at 77~K.  The raw structure factors have been
505 > convoluted with a gaussian instrument function (0.075~\AA$^{-1}$
506 > width) to compensate for the truncation effects in our finite size
507   simulations. The labeled peaks compared favorably with ``spurious''
508   peaks observed in experimental studies of amorphous solid
509   water.\cite{Bizid87}}

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