DOI: 10.1007/978-1-4020-8425-6_9
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Measurement of the Dresselhaus and Rashba Spin-Orbit Coupling Via Weak Anti-Localization in InSb Quantum Wells

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Cited by 7 publications
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“…25 Our k ⃗ • p⃗ calculation for this QW width predicts α = 0.2 eVÅ, which is lower than the α = 0.8 eVÅ estimated from extracted parameters, suggesting there are contributions from Dresselhaus SOC terms in Sb compounds. 26 We also note that a Schrodinger-Poisson calculation for our 20 nm QW showed one electronic sub-band is occupied.…”
mentioning
confidence: 59%
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“…25 Our k ⃗ • p⃗ calculation for this QW width predicts α = 0.2 eVÅ, which is lower than the α = 0.8 eVÅ estimated from extracted parameters, suggesting there are contributions from Dresselhaus SOC terms in Sb compounds. 26 We also note that a Schrodinger-Poisson calculation for our 20 nm QW showed one electronic sub-band is occupied.…”
mentioning
confidence: 59%
“…If this splitting were all due to the linear Rashba SOC term, we would obtain its parameter as , where Δ n = | n + – n – |, assuming a band mass of m * = 0.011 m e at 50% composition . Our k⃗ · p⃗ calculation for this QW width predicts α = 0.2 eVÅ, which is lower than the α = 0.8 eVÅ estimated from extracted parameters, suggesting there are contributions from Dresselhaus SOC terms in Sb compounds . We also note that a Schrödinger-Poisson calculation for our 20 nm QW showed one electronic sub-band is occupied.…”
mentioning
confidence: 74%
“…5 Measurements on n-InSb/ InAlSb 2DESs which are remotely doped from only one side of the well have determined 0.07 Շ ͉␣͉ Շ 0.14 eV Å. 38,39 In the sections below the AL data will be analyzed to obtain the magnitude of ␣ in the heterostructure shown in Fig. 1.…”
Section: Methodsmentioning
confidence: 99%
“…Dedigama et al recently reported the first observations of WAL in a ͑low mobility͒ InSb QW supporting the presence of large SO coupling. 16 In an alternative approach, Khodaparast et al 17 extrapolated a spin splitting to zero field in an asymmetric 30 nm InSb/InAlSb QW from electron-spinresonance measurements. Assuming the Rashba interaction to be dominant, ␣ R was determined to be as high as 1.3 ϫ 10 −11 eV m. This is larger than recent theoretical calculations in InSb/InAlSb QWs estimating ␣ R to be in the range of 2-7ϫ 10 −12 eV m. 18 In this work it was also demonstrated that the bulk inversion asymmetry ͑BIA͒ contribution to spin splitting can be of significant and comparable value to that of the Rashba depending on the specific details of the heterostructure.…”
Section: Introductionmentioning
confidence: 99%