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DUFF Energy Functions

The total potential energy function in DUFF is

$\displaystyle V = \sum^{N}_{I=1} V^{I}_{\text{Internal}} + \sum^{N-1}_{I=1} \sum_{J>I} V^{IJ}_{\text{Cross}},$ (3.7)

where $ V^{I}_{\text{Internal}}$ is the internal potential of molecule $ I$ :

$\displaystyle V^{I}_{\text{Internal}} = \sum_{\theta_{ijk} \in I} V_{\text{bend...
...le}} (\mathbf{r}_{ij},\boldsymbol{\Omega}_{i},\boldsymbol{\Omega}_{j}) \biggr].$ (3.8)

Here $ V_{\text{bend}}$ is the bend potential for all 1, 3 bonded pairs within the molecule $ I$ , and $ V_{\text{torsion}}$ is the torsion potential for all 1, 4 bonded pairs. The pairwise portions of the non-bonded interactions are excluded for atom pairs that are involved in the smae bond, bend, or torsion. All other atom pairs within a molecule are subject to the LJ pair potential.

The bend potential of a molecule is represented by the following function:

$\displaystyle V_{\text{bend}}(\theta_{ijk}) = k_{\theta}( \theta_{ijk} - \theta_0 )^2,$ (3.9)

where $ \theta_{ijk}$ is the angle defined by atoms $ i$ , $ j$ , and $ k$ (see Fig. 3.1), $ \theta_0$ is the equilibrium bond angle, and $ k_{\theta}$ is the force constant which determines the strength of the harmonic bend. The parameters for $ k_{\theta}$ and $ \theta_0$ are borrowed from those in TraPPE.[18]

The torsion potential and parameters are also borrowed from TraPPE. It is of the form:

$\displaystyle V_{\text{torsion}}(\phi) = c_1[1 + \cos \phi] + c_2[1 + \cos(2\phi)] + c_3[1 + \cos(3\phi)],$ (3.10)

where:

$\displaystyle \cos\phi = (\hat{\mathbf{r}}_{ij} \times \hat{\mathbf{r}}_{jk}) \cdot (\hat{\mathbf{r}}_{jk} \times \hat{\mathbf{r}}_{kl}).$ (3.11)

Here, $ \hat{\mathbf{r}}_{\alpha\beta}$ are the set of unit bond vectors between atoms $ i$ , $ j$ , $ k$ , and $ l$ . For computational efficiency, the torsion potential has been recast after the method of CHARMM,[1] in which the angle series is converted to a power series of the form:

$\displaystyle V_{\text{torsion}}(\phi) = k_3 \cos^3 \phi + k_2 \cos^2 \phi + k_1 \cos \phi + k_0,$ (3.12)

where:

$\displaystyle k_0$ $\displaystyle = c_1 + c_3,$    
$\displaystyle k_1$ $\displaystyle = c_1 - 3c_3,$    
$\displaystyle k_2$ $\displaystyle = 2 c_2,$    
$\displaystyle k_3$ $\displaystyle = 4c_3.$    

By recasting the potential as a power series, repeated trigonometric evaluations are avoided during the calculation of the potential energy.

The cross potential between molecules $ I$ and $ J$ , $ V^{IJ}_{\text{Cross}}$ , is as follows:

$\displaystyle V^{IJ}_{\text{Cross}} = \sum_{i \in I} \sum_{j \in J} \biggl[ V_{...
...ky}} (\mathbf{r}_{ij},\boldsymbol{\Omega}_{i},\boldsymbol{\Omega}_{j}) \biggr],$ (3.13)

where $ V_{\text{LJ}}$ is the Lennard Jones potential, $ V_{\text{dipole}}$ is the dipole dipole potential, and $ V_{\text{sticky}}$ is the sticky potential defined by the SSD model (Sec. 3.2.2). Note that not all atom types include all interactions.

The dipole-dipole potential has the following form:

$\displaystyle V_{\text{dipole}}(\mathbf{r}_{ij},\boldsymbol{\Omega}_{i}, \bolds...
...l_comment_mark>25 (\boldsymbol{\hat{u}}_j \cdot \hat{\mathbf{r}}_{ij}) \biggr].$ (3.14)

Here $ \mathbf{r}_{ij}$ is the vector starting at atom $ i$ pointing towards $ j$ , and $ \boldsymbol{\Omega}_i$ and $ \boldsymbol{\Omega}_j$ are the orientational degrees of freedom for atoms $ i$ and $ j$ respectively. The magnitude of the dipole moment of atom $ i$ is $ \vert\mu_i\vert$ , $ \boldsymbol{\hat{u}}_i$ is the standard unit orientation vector of $ \boldsymbol{\Omega}_i$ , and $ \boldsymbol{\hat{r}}_{ij}$ is the unit vector pointing along $ \mathbf{r}_{ij}$ ( $ \boldsymbol{\hat{r}}_{ij}=\mathbf{r}_{ij}/\vert\mathbf{r}_{ij}\vert$ ).


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Next: The DUFF Water Models: Up: Dipolar Unified-Atom Force Field Previous: Dipolar Unified-Atom Force Field   Contents
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Updated on January 16, 2006