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interactions:coulomb

Electrostatics can be enabled with the *coulomb* option. A charge $q$, which has to be given
in the potential file, is assigned to each atom type. The coulomb interaction of a set of $N$ ions
is calculated as
$$E_\text{total}^\text{Coul} = \frac{1}{2} \sum_{i\neq j} E(r_{ij}) \qquad \text{with} \qquad
E(r_{ij}) \sim \frac{q_{i}q_{j}}{r_{ij}}.$$

There are three modifications required for a proper numerical calculation.

$$E_\text{total}^\text{Coul} = \frac{1}{2} \sum_{\substack{i\neq j\\r_{ij} \leq r_\text{cut}}} E(r_{ij})$$

Because electrostatics are long ranged, a cutoff radius $r_{\text{cut}}$ is introduced to achieve convergency.

$$E (r_{ij}) \longrightarrow E (r_{ij}) - E (r_{\text{cut}}) - (r_{ij} - \left.r_{\text{cut}})\frac{dE}{dr} \right|_{r_{\text{cut}}}$$

The shifted potential enery and it's gradient go to zero at the cutoff sphere. This is equivalent to the idea of putting mirror charges on the sphere which screen the total net charge within the sphere.

$$E (r_{ij}) \longrightarrow E (r_{ij}) \text{erfc}(\kappa r_{ij})$$

This damping is an approximation, which yields faster convergency in real space.

This approach is the Wolf summation method^{1)}.
The Coulomb potential can be combined with any analytic (short-range) pair potential. Morse-Stretch (ms) and Buckingham (buck) potentials are adapted to use with Wolf-Summation for dipoles by assuring zero gradient at the cutoff. Coulomb potentials can be combined with EAM or angular-dependent potentials by using the force calculation routines built for this purpose.

Only one additional parameter can be given in the parameter file:

**dp_cut** - float - 10

cutoff-radius for electrostatic interactions, doesn't depend on other
pair-function-radii.

`coulomb`

has to be compiled with option`apot`

.`coulomb`

can be used with`stress`

,`fweight`

,`evo`

and can also be executed in parallel using option`mpi`

.`coulomb`

can optionally be combined with angular (`ang`

) or EAM (`eam`

) potentials. It cannot not be used together with any other force-field approaches (`pair`

,`adp`

, …). Note that pair potentials are available by default and must not be specifically added.

When using `coulomb`

interactions, the following parameters have to given in the potential file, labeled by the keyword elstat:

`ratio`

stoichiometric ratio is needed, because charges are optimized under the constraint of charge neutrality.`charge`

(ntypes-1) charges have to be given, the last one is calculated via ratio.`kappa`

damping parameter $\kappa$ of the Wolf summation, it is recommended to keep it constant

Example for the diatomic oxide SiO_{2}

#F 0 3 #C Si O #I 0 0 0 #E elstat ratio 1 2 charge_Si value min max kappa value min max

An entire potential file can be downloaded here: Examples

To describe a system with $N$ atom types you need $N(N+1)/2$ potentials.

$N$ | $N(N+1)/2$ |
---|---|

1 | 1 |

2 | 3 |

3 | 6 |

The potential table is assumed to be symmetric, i.e. the potential for the atom types 1-0 is the same as the potential 0-1.

The order of the pair potentials in the potential file for *N* atom types is:

$\Phi_{00}, \ldots, \Phi_{0N}, \Phi_{11}, \ldots, \Phi_{1N}, \ldots, \Phi_{NN}$

D. Wolf, P. Keblinski, S. R. Phillpot, and J. Eggenbrecht, J. Chem. Phys. **110**, 8254 (1999)

interactions/coulomb.txt · Last modified: 2018/03/19 16:29 by pbro

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