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dc.creatorSinitsyn, NA
dc.creatorHankiewicz, EM
dc.creatorTeizer, Winfried
dc.creatorSinova, Jairo.
dc.date.accessioned2012-09-19T20:05:35Z
dc.date.available2012-09-19T20:05:35Z
dc.date.issued2004
dc.identifier.citationNA Sinitsyn, EM Hankiewicz, Winfried Teizer and Jairo Sinova. Phys.Rev.B 70 081312 2004."Copyright (2004) by the American Physical Society."en
dc.identifier.urihttp://dx.doi.org/10.1103/PhysRevB.70.081312
dc.identifier.urihttps://hdl.handle.net/1969.1/146802
dc.descriptionJournals published by the American Physical Society can be found at http://journals.aps.org/en
dc.description.abstractWe investigate the spin-current linear response conductivity tensor to an electric field in a paramagnetic two-dimensional electron gas with both Rashba and Dresselhaus spin-orbit coupling in the weak scattering regime within the Born approximation. In the usual sample parameters, and for cross-sectional size smaller than the spin-coherence length, the spin-Hall conductivity depends only on the sign of the difference in magnitude of the Rashba and Dresselhaus coupling except within a narrow window where both coupling strengths are equal. We also find that a spin current is generated in the direction of the driving field for a non-zero Dresselhaus term. Possible experimental setups for its detection, taking into account the finite mobility and typical parameters of current samples, are discussed.en
dc.language.isoen
dc.publisherAmerican Physical Society
dc.rightsThis work is archived in the Texas A&M Digital Repository with the express permission of the rights holder (commonly but not always the publisher). A copy of the permission document is on file with the Texas A&M University Libraries.en
dc.subjectROOM-TEMPERATUREen
dc.subjectTUNNEL-JUNCTIONSen
dc.subjectSEMICONDUCTORSen
dc.subjectMAGNETORESISTANCEen
dc.subjectINJECTIONen
dc.subjectLAYERSen
dc.subjectPhysicsen
dc.titleSpin Hall and spin-diagonal conductivity in the presence of Rashba and Dresselhaus spin-orbit couplingen
dc.typeArticleen
local.departmentPhysics and Astronomyen


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