Issue |
Eur. Phys. J. AP
Volume 20, Number 1, October 2002
|
|
---|---|---|
Page(s) | 41 - 53 | |
Section | Surfaces, Interfaces and Films | |
DOI | https://doi.org/10.1051/epjap:2002074 | |
Published online | 01 October 2002 |
https://doi.org/10.1051/epjap:2002074
Interpretation method for mirror experiments based on a Monte Carlo charge implantation model
1
LPIO (EA 3254), Faculté des Sciences de Nantes, 2 rue de la Houssinière, 44322 Nantes
Cedex 03, France
2
CEA, Le Ripault, BP 16, 37260 Monts, France
Corresponding author: raphael.renoud@physique.univ-nantes.fr
Received:
3
June
2002
Accepted:
31
July
2002
Published online:
1
October
2002
The scanning electron microscope mirror (SEMM) method is considered as a suitable approach for the characterisation of the charge trapping ability of insulators. However, the interpretation of the experimental results is far from being obvious. The aim of this paper is to give some new insights in this problem. Our description of the mirror plots is conventionally based on a multipole analysis of the charge distribution and on the radius of curvature approximation. This approach indicates that the trend of the plots is mainly controlled by the quadrupole contribution. This clearly illustrates the non- uniqueness of the interpretation since different trapped charge distributions, but with nearly equal quadrupole terms, can produce rather similar mirror plots. To make the problem unambiguous, a semi-ellipsoidal shell model is used to account for the implanted space charge. Within this model, we propose a simple method to get the mean density of trapped charge ρ0. Our Monte Carlo simulations of the charge implantation phase show that ρ0 can strongly differ from the density of traps NT. The reasons for these deviations are discussed for a significant set of values of NT and of the primary energy Ep.
PACS: 77.22.Jp – Dielectric breakdown and space-charge effects / 72.20.Jv – Charge carriers: generation, recombination, lifetime, and trapping / 79.20.Hx – Electron impact: secondary emission
© EDP Sciences, 2002
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