Mahadevan, Priya ; Zunger, Alex (2003) Ferromagnetism in Mn-doped GaAs due to substitutional-interstitial complexes Physical Review B: Condensed Matter and Materials Physics, 68 (7). Article ID 075202. ISSN 2469-9950
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Official URL: http://journals.aps.org/prb/abstract/10.1103/PhysR...
Related URL: http://dx.doi.org/10.1103/PhysRevB.68.075202
Abstract
While most calculations on the properties of the ferromagnetic semiconductor GaAs:Mn have focused on isolated Mn substituting the Ga site (MnGa), we investigate here whether alternate lattice sites are favored and what the magnetic consequences of this might be. Under As-rich (Ga-poor) conditions prevalent at growth, we find that the formation energies are lower for MnGa over interstitial Mn (Mni). As the Fermi energy is shifted towards the valence band maximum via external p doping, the formation energy of Mni is reduced relative to MnGa. Furthermore, under epitaxial growth conditions, the solubility of both substitutional and interstitial Mn are strongly enhanced over what is possible under bulk growth conditions. The high concentration of Mn attained under epitaxial growth of p-type material opens the possibility of Mn atoms forming small clusters. We consider various types of clusters, including the Coulomb-stabilized clusters involving two MnGa and one Mni. While isolated Mni are hole killers (donors), and therefore destroy ferromagnetism, complexes such as (MnGa− Mni− MnGa) are found to be more stable than complexes involving MnGa− MnGa− MnGa. The former complexes exhibit partial or total quenching of holes, yet Mni in these complexes provide a channel for a ferromagnetic arrangement of the spins on the two MnGa within the complex. This suggests that ferromagnetism in Mn-doped GaAs arises both from holes due to isolated MnGa as well as from strongly Coulomb stabilized MnGa− Mni− MnGa clusters.
Item Type: | Article |
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Source: | Copyright of this article belongs to American Physical Society. |
ID Code: | 102969 |
Deposited On: | 02 Feb 2018 03:55 |
Last Modified: | 02 Feb 2018 03:55 |
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