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 inChinese physics B Vol. 18; no. 12; pp. 5431 - 5436
Main Author 方诚 王志刚 李树深 张平
Format Journal Article
LanguageEnglish
Published IOP Publishing 01.12.2009
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ISSN1674-1056
2058-3834
DOI10.1088/1674-1056/18/12/050

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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.
Bibliography:TN4
O572
11-5639/O4
orbital magnetization, Zeeman splitting, Berry phase effect, semiconductor
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ISSN:1674-1056
2058-3834
DOI:10.1088/1674-1056/18/12/050