Please use this identifier to cite or link to this item: https://doi.org/10.1103/PhysRevB.80.235404
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dc.titleOptical rotation of heavy hole spins by non-Abelian geometrical means
dc.contributor.authorSun, H.
dc.contributor.authorFeng, X.-L.
dc.contributor.authorWu, C.
dc.contributor.authorLiu, J.-M.
dc.contributor.authorGong, S.
dc.contributor.authorOh, C.H.
dc.date.accessioned2014-10-16T09:35:27Z
dc.date.available2014-10-16T09:35:27Z
dc.date.issued2009-12-03
dc.identifier.citationSun, H., Feng, X.-L., Wu, C., Liu, J.-M., Gong, S., Oh, C.H. (2009-12-03). Optical rotation of heavy hole spins by non-Abelian geometrical means. Physical Review B - Condensed Matter and Materials Physics 80 (23) : -. ScholarBank@NUS Repository. https://doi.org/10.1103/PhysRevB.80.235404
dc.identifier.issn10980121
dc.identifier.urihttp://scholarbank.nus.edu.sg/handle/10635/97453
dc.description.abstractA non-Abelian geometric method is proposed for rotating of heavy hole spins in a singly positive charged quantum dot in Voigt geometry. The key ingredient is the delay-dependent non-Abelian geometric phase, which is produced by the nonadiabatic transition between the two degenerate dark states. We demonstrate, by controlling the pump, the Stokes and the driving fields, that the rotations about y and z axes with arbitrary angles can be realized with high fidelity. Fast initialization and heavy hole-spin-state readout are also possible. © 2009 The American Physical Society.
dc.description.urihttp://libproxy1.nus.edu.sg/login?url=http://dx.doi.org/10.1103/PhysRevB.80.235404
dc.sourceScopus
dc.typeArticle
dc.contributor.departmentPHYSICS
dc.description.doi10.1103/PhysRevB.80.235404
dc.description.sourcetitlePhysical Review B - Condensed Matter and Materials Physics
dc.description.volume80
dc.description.issue23
dc.description.page-
dc.description.codenPRBMD
dc.identifier.isiut000273228800100
Appears in Collections:Staff Publications

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