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POSSIBILITIES OF FORMATION OF BRIGHT EBIC CONTRASTS DUE TO CRYSTAL DEFECTS IN SILICON

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HAL Id: jpa-00229668

https://hal.archives-ouvertes.fr/jpa-00229668

Submitted on 1 Jan 1989

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POSSIBILITIES OF FORMATION OF BRIGHT EBIC CONTRASTS DUE TO CRYSTAL DEFECTS IN

SILICON

H. Blumtritt, M. Kittler, W. Seifert

To cite this version:

H. Blumtritt, M. Kittler, W. Seifert. POSSIBILITIES OF FORMATION OF BRIGHT EBIC CON-

TRASTS DUE TO CRYSTAL DEFECTS IN SILICON. Journal de Physique Colloques, 1989, 50

(C6), pp.C6-183-C6-183. �10.1051/jphyscol:1989637�. �jpa-00229668�

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R E W E DE PHYSIQUE

APPLIQUEE

Colloque C6, Supplbment au n06, Tome 24, Juin 1989

POSSIBILITIES OF FORMATION OF BRIGHT EBIC CONTRASTS DUE TO CRYSTAL DEFECTS IN SILICON

H. BLUMTRITT, M. KITTLER' and W. SEIFERT"

Academy of Sciences of the D.R.G., Institute of Solid State Physics and Electron Microscopy, DDR-4020 Halle, D.R.G.

" ~ c a d e m y of Sciences of the D.R.GI, Institute of Semiconductor Physics, DDR-1200 Frankfurt, D.R.G.

Besides the usual, well understood dark recombination contrasts, also bright EBIC contrasts can be found at extended crystal defects in silicon. Often they appear as bright haloes around dark contrasts, but sole bright contrats are observed, too.

Different mechanisms may lead to the formation of such phenomena, thus rendering clear identification of the contrast origin difficult some- times

.

The poeter disouseea the possible origin of bright-contrast phenomena, except phenomena caused by microplasmas and surface structure. The following effects are illustrated by examples:

-

doping inhomogeneities

-

contrast due to increased width of the junction space-charge region

contrast due to plasma screening

-

lifetime enhancement within getter zones

-

charge collection by defect-own space-charge regions - repulsion of minority carriers by charged defects

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other, injection-dependent effects.

Up to now there are no models available to describe these contrast phenomena in a quantitative manner.

Article published online by EDP Sciences and available at http://dx.doi.org/10.1051/jphyscol:1989637

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