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Revision 710 by mmeineke, Fri Aug 22 19:37:54 2003 UTC vs.
Revision 716 by mmeineke, Sun Aug 24 04:00:44 2003 UTC

# Line 1 | Line 1
1  
2 < \documentclass[prb,aps,twocolumn]{revtex4}
2 > \section{\label{sec:DUFF}The DUFF Force Field}
3  
4 < \usepackage{amsmath}
5 < \usepackage{berkeley}
6 < \usepackage{graphicx}
7 < \usepackage{tabularx}
4 > The DUFF (\underline{D}ipolar \underline{U}nified-atom
5 > \underline{F}orce \underline{F}ield) force field was developed to
6 > simulate lipid bilayer formation and equilibrium dynamics. We needed a
7 > model capable of forming bilaers, while still being sufficiently
8 > computationally efficient allowing simulations of large systems
9 > (\~100's of phospholipids, \~1000's of waters) for long times (\~10's
10 > of nanoseconds).
11  
12 < \begin{document}
12 > With this goal in mind, we decided to eliminate all charged
13 > interactions within the force field. Charge distributions were
14 > replaced with dipolar entities, and charge neutral distributions were
15 > reduced to Lennard-Jones interaction sites. This simplification cuts
16 > the length scale of long range interactions from $\frac{1}{r}$ to
17 > $\frac{1}{r^3}$ (Eq.~\ref{eq:dipole} vs.~ Eq.~\ref{eq:coloumb}),
18 > allowing us to avoid the computationally expensive Ewald-Sum. Instead,
19 > we can use neighbor-lists and cutoff radii for the dipolar
20 > interactions.
21  
22 < \section{The DUFF Energy Function}
23 < \label{sec:energyFunctionals}
22 > \begin{align}
23 > V^{\text{dipole}}_{ij}(\mathbf{r}_{ij},\boldsymbol{\Omega}_{i},
24 >        \boldsymbol{\Omega}_{j}) &=
25 >        \frac{1}{4\pi\epsilon_{0}} \biggl[
26 >        \frac{\boldsymbol{\mu}_{i} \cdot \boldsymbol{\mu}_{j}}{r^{3}_{ij}}
27 >        -
28 >        \frac{3(\boldsymbol{\mu}_i \cdot \mathbf{r}_{ij}) %
29 >                (\boldsymbol{\mu}_j \cdot \mathbf{r}_{ij}) }
30 >                {r^{5}_{ij}} \biggr]\label{eq:dipole} \\
31 > V^{\text{ch}}_{ij}(\mathbf{r}_{ij}) &= \frac{q_{i}q_{j}}%
32 >        {4\pi\epsilon_{0} r_{ij}} \label{eq:coloumb}
33 > \end{align}
34  
35 + Applying this standard to the lipid model, we decided to represent the
36 + lipid model as a point dipole interaction site. Lipid head groups are
37 + typically zwitterionic in nature, with sometimes full integer charges
38 + seperated by only 5 to 6~$\mbox{\AA}$. By placing a dipole of
39 + 20.6~Debye at the head groups center of mass, our model mimics the
40 + dipole of DMPC.\cite{Cevc87} Then, to account for the steric henderanc
41 + of the head group, a Lennard-Jones interaction site is also oacted at
42 + the psuedoatom's center of mass. The model is illustrated in
43 + Fig.~\ref{fig:lipidModel}.
44  
45 + \begin{figure}
46 + \includegraphics[angle=-90,width=\linewidth]{lipidModel.epsi}
47 + \caption{A representation of the lipid model. $\phi$ is the torsion angle, $\theta$ %
48 + is the bend angle, $\mu$ is the dipole moment of the head group, and n is the chain length.}
49 + \label{fig:lipidModel}
50 + \end{figure}
51  
52 < The main energy function in OOPSE is DUFF (the Dipolar
53 < Unified-atom Force Field). DUFF is a collection of parameters taken
54 < from Seipmann \emph{et al.}\cite{Siepmann1998} and Ichiye \emph{et
52 > Turning to the tail chains of the phospholipids, we needed a set of
53 > scalable parameters to model the alkyl groups as Lennard-Jones
54 > interaction sites. For this, we used the TraPPE force field of
55 > Siepmann \emph{et al}.\cite{Siepmann1998} The force field is a
56 > unified-atom representation of n-alkanes. It is parametrized against
57 > phase equilibria using Gibbs Monte Carlo simulation techniques. One of
58 > the advantages of TraPPE is that is generalizes the types of atoms in
59 > an alkyl chain to keep the number of pseudoatoms to a minimum.
60 > %( $ \mbox{CH_3} $ %-$\mathbf{\mbox{CH_2}}$-$\mbox{CH_3}$ is the same as
61 >
62 > Another advantage of using TraPPE is the constraining of all bonds to
63 > be of fixed length. Typically, bond vibrations are the motions in a
64 > molecular dynamic simulation. This neccesitates a small time step
65 > between force evaluations be used to ensure adequate sampling of the
66 > bond potential. Failure to do so will result in loss of energy
67 > conservation within the microcanonical ensemble. By constraining this
68 > degree of freedom, time steps larger than were previously allowable
69 > are able to be used when integrating the equations of motion.
70 >
71 > The main energy function in OOPSE is DUFF (the Dipolar Unified-atom
72 > Force Field). DUFF is a collection of parameters taken from Seipmann
73 > and Ichiye \emph{et
74   al.}\cite{liu96:new_model} The total energy of interaction is given by
75   Eq.~\ref{eq:totalPotential}:
76   \begin{equation}
# Line 58 | Line 113 | V_{\text{LJ}} = \text{internal + external}
113   \end{equation}
114  
115  
61
62 \bibliography{oopse}
63
64 \end{document}

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