Local current distribution and hot spots in the integer quantum Hall regime
Yonatan Dubi,1 Yigal Meir,1,2 and Yshai Avishai1,2,3
1Physics Department, Ben-Gurion University, Beer Sheva 84105, Israel
2The Ilse Katz Center for Meso- and Nano-scale Science and Technology, Ben-Gurion University, Beer Sheva 84105, Israel
3Department of Applied Physics, University of Tokyo, Hongo Bunkyo-ku, Tokyo 113, Japan
(Received 12 July 2006; published 14 November 2006)
In a recent experiment, the local current distribution of a two-dimensional electron gas in the quantum Hall regime was probed by measuring the variation of the conductance due to local gating. The main experimental finding was the existence of "hot spots," i.e., regions with a high degree of sensitivity to local gating, whose density increases as one approaches the quantum Hall transition. However, the direct connection between these hot spots and regions of high current flow is not clear. Here, based on a recent model for the quantum Hall transition consisting of a mixture of perfect and quantum links, the relation between the hot spots and the current distribution in the sample has been investigated. The model reproduces the observed dependence of the number and sizes of hot spots on the filling factor. It is further demonstrated that these hot spots are not located in regions where most of the current flows, but rather, in places where the currents flow both when injected from the left or from the right. A quantitative measure, the harmonic mean of these currents is introduced and correlates very well with the hot spots positions.
©2006 The American Physical Society
URL: http://link.aps.org/abstract/PRB/v74/e205314
doi:10.1103/PhysRevB.74.205314
PACS: 73.43.-f, 73.50.-h
Additional Information
Full Text: PDF
From PRB (you may need a password for this)
PDF
Only references to articles in journals published by the American Physical Society and the American Institute of Physics are displayed. The complete list is available to subscribers only. Non-subscribers have the option to purchase the articles on this list.
- B. I. Halperin, Phys. Rev. B 25, 2185 (1982);
M. Buttiker, ibid. 38, 9375 (1988);
D. B. Chklovskii, B. I. Shklovskii, and L. I. Glazman, ibid. 46, 4026 (1992).
- H. Hirai and S. Komiyama, Phys. Rev. B 49, 14012 (1994);
- E. Yahel, A. Tsukernik, A. Palevski, and H. Shtrikman, Phys. Rev. Lett. 81, 5201 (1998).
- K. L. McCormick, M. T. Woodside, M. Huang, M. Wu, P. L. McEuen, C. Duruoz, and J. S. Harris, Phys. Rev. B 59, 4654 (1999);
-
B. J. Van Wees, H. van Houten, C. W. J. Beenakker, J. G. Williamson, L.
P. Kouwenhoven, D. van der Marel, and C. T. Foxon, Phys. Rev. Lett. 60, 848 (1988);
- G. Metalidis and P. Bruno, Phys. Rev. B 72, 235304 (2005).
- A. Kicin, A. Pioda, T. Ihn, K. Ensslin, D. C. Driscoll, and A. C. Gossard, Phys. Rev. B 70, 205302 (2004).
- Y. Dubi, Y. Meir, and Y. Avishai, Phys. Rev. B 71, 125311 (2005);
Y. Dubi, Y. Meir, and Y. Avishai, Phys. Rev. Lett. 94, 156406 (2005).
- For a review see, e.g., B. Huckestein, Rev. Mod. Phys. 67, 357 (1995).
- S. Cho and M. P. A. Fisher, Phys. Rev. B 55, 1637 (1997).
- A. Cresti, G. Grosso, and G. P. Parravicini, Phys. Rev. B 69, 233313 (2004).
Full Text:
Buy Article
PDF