Statistics of Coulomb Blockade Peak Spacings

Statistics of Coulomb Blockade Peak Spacings
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库仑封锁峰间距统计

DOI:
10.1103/physrevlett.80.4522
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发表时间:
1997
影响因子:
8.6
通讯作者:
A. Gossard
A. Gossard
中科院分区:
物理与天体物理1区
文献类型:
--
作者:
S. Patel;S. M. Cronenwett;Duncan R. Stewart;A. Huibers;Charles Marcus;C. I. Duruöz;James S. Harris;K. Campman;A. Gossard

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本文报道了GaAs量子点中未破缺(磁场$B\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}}0$)和破缺(磁场$B\ensuremath{\ne}0$)时间反转对称性的大集合的库仑阻断峰间距分布。这两个分布都是对称的,大致为高斯分布,宽度为平均间距的2%,尾部为宽的非高斯分布。在$B\phantom{\rule{0ex}{0ex} = $ phantom{\rule{0ex}{0ex}}0$时,分布系统地更宽,其倍数为$\ensuremath{\sim}1.2\ifmmode\pm\else\textpm\fi{}0.1$。在空间分布中没有发现奇偶间距相关或双峰结构,表明不存在自旋简并。峰间距和峰高之间没有观察到相关关系。
Distributions of Coulomb blockade peak spacings are reported for large ensembles of both unbroken (magnetic field $B\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}0$) and broken ( $B\ensuremath{\ne}0$) time-reversal symmetry in GaAs quantum dots. Both distributions are symmetric and roughly Gaussian with a width of $\ensuremath{\sim}2%\char21{}6%$ of the average spacing, with broad, non-Gaussian tails. The distribution is systematically wider at $B\phantom{\rule{0ex}{0ex}}=\phantom{\rule{0ex}{0ex}}0$ by a factor of $\ensuremath{\sim}1.2\ifmmode\pm\else\textpm\fi{}0.1$. No even-odd spacing correlations or bimodal structure in the spacing distribution is found, suggesting an absence of spin degeneracy. There is no observed correlation between peak spacing and peak height.