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Revision 759 by chrisfen, Wed Sep 10 22:42:57 2003 UTC vs.
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# Line 146 | Line 146 | water.\cite{Ichiye96} In the original molecular dynami
146   simulations using this model, Ichiye \emph{et al.} reported a
147   calculation speed up of up to an order of magnitude over other
148   comparable models while maintaining the structural behavior of
149 < water.\cite{Ichiye96} In the original molecular dynamics studies of
150 < SSD, it was shown that it actually improves upon the prediction of
151 < water's dynamical properties 3 and 4-point models.\cite{Ichiye99} This
149 > water.\cite{Ichiye96} In the original molecular dynamics studies, it
150 > was shown that SSD improves on the prediction of many of water's
151 > dynamical properties over TIP3P and SPC/E.\cite{Ichiye99} This
152   attractive combination of speed and accurate depiction of solvent
153   properties makes SSD a model of interest for the simulation of large
154   scale biological systems, such as membrane phase behavior, a specific
# Line 205 | Line 205 | SSD more compatible with a reaction field.
205   to the use of reaction field, simulations were also performed without
206   a surrounding dielectric and suggestions are proposed on how to make
207   SSD more compatible with a reaction field.
208 <
208 >
209   Simulations were performed in both the isobaric-isothermal and
210   microcanonical ensembles. The constant pressure simulations were
211   implemented using an integral thermostat and barostat as outlined by
212 < Hoover.\cite{Hoover85,Hoover86} For the constant pressure
213 < simulations, the \emph{Q} parameter for the was set to 5.0 amu
214 < \(\cdot\)\AA\(^{2}\), and the relaxation time (\(\tau\))\ was set at
215 < 100 ps.
212 > Hoover.\cite{Hoover85,Hoover86} All particles were treated as
213 > non-linear rigid bodies. Vibrational constraints are not necessary in
214 > simulations of SSD, because there are no explicit hydrogen atoms, and
215 > thus no molecular vibrational modes need to be considered.
216  
217   Integration of the equations of motion was carried out using the
218   symplectic splitting method proposed by Dullweber \emph{et
# Line 220 | Line 220 | requirement that is actually quite sensitive to errors
220   deals with poor energy conservation of rigid body systems using
221   quaternions. While quaternions work well for orientational motion in
222   alternate ensembles, the microcanonical ensemble has a constant energy
223 < requirement that is actually quite sensitive to errors in the
224 < equations of motion. The original implementation of this code utilized
225 < quaternions for rotational motion propagation; however, a detailed
226 < investigation showed that they resulted in a steady drift in the total
227 < energy, something that has been observed by others.\cite{Laird97}
223 > requirement that is quite sensitive to errors in the equations of
224 > motion. The original implementation of this code utilized quaternions
225 > for rotational motion propagation; however, a detailed investigation
226 > showed that they resulted in a steady drift in the total energy,
227 > something that has been observed by others.\cite{Laird97}
228  
229   The key difference in the integration method proposed by Dullweber
230   \emph{et al.} is that the entire rotation matrix is propagated from
# Line 244 | Line 244 | simpler arithmetic quaternion propagation. On average,
244   method, the orientational propagation involves a sequence of matrix
245   evaluations to update the rotation matrix.\cite{Dullweber1997} These
246   matrix rotations end up being more costly computationally than the
247 < simpler arithmetic quaternion propagation. On average, a 1000 SSD
248 < particle simulation shows a 7\% increase in computation time using the
249 < symplectic step method in place of quaternions. This cost is more than
250 < justified when comparing the energy conservation of the two methods as
251 < illustrated in figure \ref{timestep}.
247 > simpler arithmetic quaternion propagation. With the same time step, a
248 > 1000 SSD particle simulation shows an average 7\% increase in
249 > computation time using the symplectic step method in place of
250 > quaternions. This cost is more than justified when comparing the
251 > energy conservation of the two methods as illustrated in figure
252 > \ref{timestep}.
253  
254   \begin{figure}
255   \includegraphics[width=61mm, angle=-90]{timeStep.epsi}
# Line 316 | Line 317 | volume fluctuations dampened out in all but the very c
317   increment was decreased from 25 K to 10 and then 5 K. The above
318   equilibration and production times were sufficient in that the system
319   volume fluctuations dampened out in all but the very cold simulations
320 < (below 225 K). In order to further improve statistics, five separate
321 < simulation progressions were performed, and the averaged results from
322 < the $I_h$ melting simulations are shown in figure \ref{dense1}.
322 <
323 < \begin{figure}
324 < \includegraphics[width=65mm, angle=-90]{1hdense.epsi}
325 < \caption{Average density of SSD water at increasing temperatures
326 < starting from ice $I_h$ lattice.}
327 < \label{dense1}
328 < \end{figure}
320 > (below 225 K). In order to further improve statistics, an ensemble
321 > average was accumulated from five separate simulation progressions,
322 > each starting from a different ice crystal.
323  
324   \subsection{Density Behavior}
325   In the initial average density versus temperature plot, the density
# Line 902 | Line 896 | The authors would like to thank the National Science F
896   simulations of biochemical systems.
897  
898   \section{Acknowledgments}
899 < The authors would like to thank the National Science Foundation for
900 < funding under grant CHE-0134881. Computation time was provided by the
901 < Notre Dame Bunch-of-Boxes (B.o.B) computer cluster under NSF grant DMR
902 < 00 79647.
899 > Support for this project was provided by the National Science
900 > Foundation under grant CHE-0134881. Computation time was provided by
901 > the Notre Dame Bunch-of-Boxes (B.o.B) computer cluster under NSF grant
902 > DMR 00 79647.
903  
904   \bibliographystyle{jcp}
905  

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