Interaction-Induced Shift of the Cyclotron Resonance of Graphene Using Infrared Spectroscopy

E. A. Henriksen, P. Cadden-Zimansky, Z. Jiang, Z. Q. Li, L.-C. Tung, M. E. Schwartz, M. Takita, Y.-J. Wang, P. Kim, and H. L. Stormer
Phys. Rev. Lett. 104, 067404 – Published 12 February 2010

Abstract

We report a study of the cyclotron resonance (CR) transitions to and from the unusual n=0 Landau level (LL) in monolayer graphene. Unexpectedly, we find the CR transition energy exhibits large (up to 10%) and nonmonotonic shifts as a function of the LL filling factor, with the energy being largest at half filling of the n=0 level. The magnitude of these shifts, and their magnetic field dependence, suggests that an interaction-enhanced energy gap opens in the n=0 level at high magnetic fields. Such interaction effects normally have a limited impact on the CR due to Kohn’s theorem [W. Kohn, Phys. Rev. 123, 1242 (1961)], which does not apply in graphene as a consequence of the underlying linear band structure.

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  • Received 18 September 2009

DOI:https://doi.org/10.1103/PhysRevLett.104.067404

©2010 American Physical Society

Authors & Affiliations

E. A. Henriksen1,*, P. Cadden-Zimansky1,2, Z. Jiang3, Z. Q. Li1, L.-C. Tung2, M. E. Schwartz1, M. Takita1, Y.-J. Wang2, P. Kim1, and H. L. Stormer1,4,5

  • 1Department of Physics, Columbia University, New York, New York 10027, USA
  • 2National High Magnetic Field Laboratory, Tallahassee, Florida 32310, USA
  • 3School of Physics, Georgia Institute of Technology, Atlanta, Georgia 30332, USA
  • 4Department of Applied Physics and Applied Mathematics, Columbia University, New York, New York 10027, USA
  • 5Bell Labs, Alcatel-Lucent, Murray Hill, New Jersey 07974, USA

  • *erikku@caltech.edu

Comments & Replies

Comment on “Interaction-Induced Shift of the Cyclotron Resonance of Graphene Using Infrared Spectroscopy”

W. Zhu, Q. W. Shi, J. G. Hou, and X. R. Wang
Phys. Rev. Lett. 105, 159703 (2010)

Henriksen et al. Reply:

E. A. Henriksen, P. Cadden-Zimansky, Z. Jiang, Z. Q. Li, and P. Kim
Phys. Rev. Lett. 105, 159704 (2010)

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Vol. 104, Iss. 6 — 12 February 2010

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