Orbital magnetization in semiconductors
This paper theoretically investigates the orbital magnetization of electron-doped (n-type) semiconductor het-erostructures and of hole-doped (p-type) bulk semiconductors, which are respectively described by a two-dimensional electron/hole Hamiltonian with both the included Rashba spin-orbit coupling...
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Published in | Chinese physics B Vol. 18; no. 12; pp. 5431 - 5436 |
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Main Author | |
Format | Journal Article |
Language | English |
Published |
IOP Publishing
01.12.2009
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Subjects | |
Online Access | Get full text |
ISSN | 1674-1056 2058-3834 |
DOI | 10.1088/1674-1056/18/12/050 |
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Summary: | This paper theoretically investigates the orbital magnetization of electron-doped (n-type) semiconductor het-erostructures and of hole-doped (p-type) bulk semiconductors, which are respectively described by a two-dimensional electron/hole Hamiltonian with both the included Rashba spin-orbit coupling and Zeeman splitting terms. It is the Zeeman splitting, rather than the Rashba spin-orbit coupling, that destroys the time-reversal symmetry of the semiconductor systems and results in nontrivial orbital magnetization. The results show that the magnitude of the orbital magnetization per hole and the Hall conductance in the p-type bulk semiconductors are about 10^-2-10^-1 effective Bohr magneton and 10^-1-1 e^2/h, respectively. However, the orbital magnetization per electron and the Hall conductance in the n-type semiconductor heterostructures are too small to be easily observed in experiment. |
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Bibliography: | TN4 O572 11-5639/O4 orbital magnetization, Zeeman splitting, Berry phase effect, semiconductor ObjectType-Article-2 SourceType-Scholarly Journals-1 ObjectType-Feature-1 content type line 23 ObjectType-Article-1 ObjectType-Feature-2 |
ISSN: | 1674-1056 2058-3834 |
DOI: | 10.1088/1674-1056/18/12/050 |