Angular distribution and Josephson plasma modes of THz radiation emitted from Bi2212 mesas with various shapes

ORAL

Abstract

So far, we have measured angular dependence of the intensity of the THz emission from mesas of high-$T_c$ superconductor $\mathrm{Bi_2Sr_2CaCu_2O_{8+\delta}}$ with various shapes such as rectangulars, squares, cylinders, triangulars, etc. and various dimensions larger or smaller than the penetration depth $\lambda_c$. The results have been analized by a model developed by Klemm and Kadowaki{\footnote{Richard A. Klemm and K. Kadowaki, J. Phys. Condens. Matter {\bf{22}} (2010) 375701.}}, which assumes coherent generation of the standing of wave cavity modes in a mesa due to the ac-Josephson effect. The higher harmonic modes are observed in some cases as expected in the model. However, it is often observed that the emission frequency does not obey the simple cavity mode, indicating that the cavity resonance may not be a stringent condition for the emission of the THz radiation. The implication is argued in terms of the emission dynamics from the Bi2212 mesa structure.

*CREST-JST, WPI-MANA, Special project (A) in Univ. of Tsukuba

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Authors

  • Kazuo Kadowaki

    • University of Tsukuba, Tsukuba, Japan
    • Institute of Materials Science, University of Tsukuba
    • University of Tsukuba, Japan

  • Takanari Kashiwagi

    • University of Tsukuba, Tsukuba, Japan
    • Institute of Materials Science, University of Tsukuba

  • Manabu Tsujimoto

    • University of Tsukuba, Tsukuba, Japan
    • Institute of Materials Science, University of tsukuba
    • University of Tsukuba

  • Takashi Yamamoto

    • Institute of Materials Science, University of Tsukuba
    • University of Tsukuba, Japan

  • Hidehiro Asai

    • Institute of Materials Science, University of Tsukuba

  • Hidetoshi Minami

    • Institute of Materials Science, University of tsukuba