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High-field ODMR investigation of the EL2 defect in semi-insulating GaAs

The microscopic structure of the EL2 defect in semi-insulating GaAs has remained controversial. It is generally agreed that EL2 is an As antisite-related defect, but whether it is an isolated AsGa defect or an AsGa-related pair defect, has not been unambiguously decided. In a previous investigation...

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Bibliographic Details
Published in:Physica. B, Condensed matter Condensed matter, 2003-12, Vol.340-342, p.353-357
Main Authors: Tkach, I., Krambrock, K., Overhof, H., Spaeth, J.-M.
Format: Article
Language:English
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Summary:The microscopic structure of the EL2 defect in semi-insulating GaAs has remained controversial. It is generally agreed that EL2 is an As antisite-related defect, but whether it is an isolated AsGa defect or an AsGa-related pair defect, has not been unambiguously decided. In a previous investigation with electron nuclear double resonance (ENDOR) detected via the magnetic circular dichroism (MCD) of the near infrared absorption of EL2+ (MCDA-ENDOR) at 24GHz (K-band) the local symmetry could not be determined conclusively due to complicated multiple ENDOR line splittings caused by strong effects of pseudo-dipolar couplings. We report on an MCDA-ENDOR investigation at 95GHz (W-band) where the undesired 75As ENDOR line splittings due to pseudo-dipolar coupling were suppressed. The surprising result is that the angular dependence of the nearest 75As shell shows almost Td symmetry. A small non-equivalence of the nearest neighbours is hidden in an unresolved ENDOR line width for B0||[001] and can be a most 1.5% of the superhyperfine (shf) constants. The lines of a further 75As shell, interpreted as the fifth shell, are split into at least two subshells indicating a pair defect in spite of the almost equivalence of the nearest neighbours. It is discussed whether EL2 is an AsGa+–VGa3− pair defect following recent theoretical calculations showing that this pair defect has the observed properties of the shf interactions.
ISSN:0921-4526
1873-2135
DOI:10.1016/j.physb.2003.09.072