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$Robin-Rolland^{[1]}$ type simulations for APT trajectories.
Consider a perfect conductor isolated in space brought to electric potential $V_{a}$, as shown above.
$V_{p}$ be the electrostatic potential at point P on the surface. Coloumb's law makes it possible to write this potential from the distribution of charges in space
(on the surface in this case):
When the point P is displaced infinitesimally displace along the unit surface normal $\vec{n_{P}}$, the variation in the potential $V_{P}$ is given by
$$\frac{\partial{V_{P}}}{\partial{n_{P}}} = \frac{1}{4\pi\varepsilon_{o}}\iint_{S^\prime}\frac{\partial(1/|\vec{u}|)}{\partial{n_{P}}}\sigma(P^{\prime}),dS^\prime$$
Combining the above two equations gives:
$$\sigma(P) = \frac{1}{2\pi} \iint_{S^\prime}\frac{\vec{n_{P}}\cdot\vec{u}}{|\vec{u}|^3}\sigma(P^{\prime}),dS^\prime - (1)$$
The above integral equation called Robin's equation, connects the surface density of charges at a point on the surface to the distribution of the charge density on the rest of the surface of the conductor. It is possible to solve iteratively by introducing a series of functions $f_{n}$ defined by:
For a point M infinitesimally close to point i, but inside the conductor. The field generated is given by the right-hand side of the above equation pointing outward, whereas the field induced by the atom i points inward, thereby canceling each other out.
Now a sequence of charges is introdued $q_{i,n}$ on atom i, as follows:
$$\frac{q_{i,n+1}}{s_{at}} = \frac{1}{2\pi} \sum_{k=1,k\neq i}^{N} q_{k,n}\frac{\vec{n_i}\cdot\vec{r_{i,k}}}{|\vec{r_{i,k}}|^3}$$
where $q_{i,0}$ being an arbitary real positive number.
the unit vector for $i^{th}$ atom depends on the theoretical P nearest neighbors:
[1] Rolland, N., Vurpillot, F., Duguay, S., & Blavette, D. (2015). A Meshless Algorithm to Model Field Evaporation in Atom Probe Tomography. Microscopy and Microanalysis, 21(6). https://doi.org/10.1017/S1431927615015184