2008
DOI: 10.1103/physrevb.78.079901
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Erratum: Zero-field spin splitting and spin lifetime inn-InSbIn1xAlxSb

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Cited by 16 publications
(38 citation statements)
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“…The smaller value of α = 0.1 eVÅ is closer to the values obtained by experiment and theory. 16,17 The simulated curves T f oc reproduce well the salient features of the experimental data, namely, the focusing peak and the non-monotonic background resistance. These focusing peaks have a FWHM of ∼33 mT, whereas the splitting of the peaks are only 1, 5 and 13 mT, respectively.…”
Section: Modelsupporting
confidence: 55%
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“…The smaller value of α = 0.1 eVÅ is closer to the values obtained by experiment and theory. 16,17 The simulated curves T f oc reproduce well the salient features of the experimental data, namely, the focusing peak and the non-monotonic background resistance. These focusing peaks have a FWHM of ∼33 mT, whereas the splitting of the peaks are only 1, 5 and 13 mT, respectively.…”
Section: Modelsupporting
confidence: 55%
“…Eq. 4 includes both Zeeman and Rashba terms but excludes Dresselhaus terms for simplicity (as is appropriate for a highly asymmetric InSb QW 16,17 ). The spin S is evolved using the cross product,…”
Section: Modelmentioning
confidence: 99%
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“…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. In support of this concept, Akabori et al 19 recently reported experimental results indicating that BIA was dominant in a similar narrow gap InGaSb/AlInSb QW sample.…”
Section: Introductionmentioning
confidence: 74%
“…12,13 Despite T 2 spin lifetimes of the order of a ps 14,15 arising from spin precessional frequencies in the THz range, these observations are possible since Fermi velocities (v F ) in these materials can be of the order of a 10 6 ms −1 . Counterintuitively, the fact that these materials exhibit long spin coherence lengths limits the ability to scale down device dimensions as the distance required to precess the electron spin can be measured in micrometres.…”
mentioning
confidence: 99%