NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Identification of the Ga interstitial in Al(x)Ga(1-x)As by optically detected magnetic resonanceA new optically detected magnetic resonance spectrum in Al(x)Ga(1-x)As is reported and assigned to native Ga interstitials. Luminescence-quenching signals were observed over the energy region from 0.75 to 1.1 eV. The optically detected magnetic resonance is nearly isotropic, with spin-Hamiltonian parameters g = 2.025 + or - 0.006, central hyperfine splitting A(Ga-69) = 0.050 + or - 0.001/cm, and A(Ga-71) = 0.064 + or - 0.001/cm for H near the 001 line. The strong hyperfine coupling denotes an electronic state of A1 symmetry, which current theories predict for the Ga interstitial but not the Ga antisite. The slight anisotropy probably indicates that the Ga(i) is paired with a second, unknown defect.
Document ID
19870037797
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Kennedy, T. A.
(U.S. Navy, Naval Research Laboratory, Washington DC, United States)
Spencer, M. G.
(Howard University Washington, DC, United States)
Date Acquired
August 13, 2013
Publication Date
November 24, 1986
Publication Information
Publication: Physical Review Letters
Volume: 57
ISSN: 0031-9007
Subject Category
Solid-State Physics
Accession Number
87A25071
Funding Number(s)
CONTRACT_GRANT: NAG5-246
CONTRACT_GRANT: NSF ECS-84-51522
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available