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Volumn 75, Issue 3, 2007, Pages

Rashba and Dresselhaus spin splittings in semiconductor quantum wells measured by spin photocurrents

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EID: 33846345357     PISSN: 10980121     EISSN: 1550235X     Source Type: Journal    
DOI: 10.1103/PhysRevB.75.035327     Document Type: Article
Times cited : (173)

References (40)
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    • We note that strictly speaking under oblique incidence the photocurrent is caused by a superposition of the CPGE and the SGE and the total current j= jCPGE + jSGE (Refs.). The individual contributions can be separated in time-resolved experiments only. However, estimations show that for the photocurrent formation due to Drude absorption usually jCPGE > jSGE which allows to neglect the SGE contribution (Refs.). Even if the SGE dominates the RD ratio can be determined from measurements under oblique incidence. In this case Eqs. 3 4 5 6 7 should be used taking into account that for optical spin orientation S e.
    • We note that strictly speaking under oblique incidence the photocurrent is caused by a superposition of the CPGE and the SGE and the total current j= jCPGE + jSGE (Refs.). The individual contributions can be separated in time-resolved experiments only. However, estimations show that for the photocurrent formation due to Drude absorption usually jCPGE > jSGE which allows to neglect the SGE contribution (Refs.). Even if the SGE dominates the RD ratio can be determined from measurements under oblique incidence. In this case Eqs. 3 4 5 6 7 should be used taking into account that for optical spin orientation S e.
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    • The measurements should be carried out at low magnetic field strengths so that ωL τs <1 and, thus, the Hanle denominator in S can be neglected. For higher magnetic fields the Hanle denominator must be taken into account.
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* 이 정보는 Elsevier사의 SCOPUS DB에서 KISTI가 분석하여 추출한 것입니다.