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dc.contributor.authorZhao, Hui
dc.contributor.authorMower, Matt
dc.contributor.authorVignale, G.
dc.date.accessioned2011-04-06T19:27:53Z
dc.date.available2011-04-06T19:27:53Z
dc.date.issued2009-03
dc.identifier.citationHui Zhao, M. Mower, and G. Vignale, Ambipolar spin diffusion and D'yakonov-Perel' spin relaxation in GaAs quantum wells. Physical Review B 79, 115321 (2009). http://link.aps.org/doi/10.1103/PhysRevB.79.115321
dc.identifier.urihttp://hdl.handle.net/1808/7356
dc.descriptionPermissions were not obtained for sharing the full text of this article. Full text available from the American Physical Society and from arXiv. See links in this record.
dc.description.abstractWe report theoretical and experimental studies of ambipolar spin diffusion in a semiconductor. A circularly polarized laser pulse is used to excite spin-polarized carriers in a GaAs multiple quantum-well sample at 80 K. Diffusion of electron and spin densities is simultaneously measured using a spatially and temporally resolved pump-probe technique. Two regimes of diffusion for spin-polarized electrons are observed. Initially, the rate of spin diffusion is similar to that of density diffusion and is controlled by the ambipolar diffusion coefficient. At later times, the spin diffusion slows down considerably relative to the density diffusion and appears to be controlled by a nonconstant (decreasing) spin-diffusion coefficient. We suggest that the long-time behavior of the spin density can be understood in terms of an inhomogeneous spin-relaxation rate, which grows with decreasing density. The behavior of the spin-relaxation rate is consistent with a model of D'yakonov-Perel' relaxation limited by the Coulomb scattering between carriers.
dc.publisherAmerican Physical Society
dc.relation.hasversionhttp://arxiv.org/abs/0903.4931v1
dc.subjectMesoscale and Nanoscale Physics
dc.subjectMaterials Science
dc.titleAmbipolar spin diffusion and D'yakonov-Perel' spin relaxation in GaAs quantum wells
dc.typeOther
kusw.kuauthorZhao, Hui
kusw.kudepartmentPhysics and Astronomy
kusw.oastatuspublisherdenied
dc.identifier.doi10.1103/PhysRevB.79.115321
kusw.oapolicyThis item does not meet KU Open Access policy criteria. Publisher denied.
dc.rights.accessrightsopenAccess


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