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      Bursts of Terahertz Radiation from Large-Scale Plasmas Irradiated by Relativistic Picosecond Laser Pulses.

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          Abstract

          Powerful terahertz (THz) radiation is observed from large-scale underdense preplasmas in front of a solid target irradiated obliquely with picosecond relativistic intense laser pulses. The radiation covers an extremely broad spectrum with about 70% of its energy located in the high frequency regime over 10 THz. The pulse energy of the radiation is found to be above 100  μJ per steradian in the laser specular direction at an optimal preplasma scale length around 40-50  μm. Particle-in-cell simulations indicate that the radiation is mainly produced by linear mode conversion from electron plasma waves, which are excited successively via stimulated Raman scattering instability and self-modulated laser wakefields during the laser propagation in the preplasma. This radiation can be used not only as a powerful source for applications, but also as a unique diagnostic of parametric instabilities of laser propagation in plasmas.

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          Author and article information

          Journal
          Phys. Rev. Lett.
          Physical review letters
          American Physical Society (APS)
          1079-7114
          0031-9007
          Jun 26 2015
          : 114
          : 25
          Affiliations
          [1 ] Beijing National Laboratory for Condensed Matter Physics, Institute of Physics, Chinese Academy of Sciences, Beijing 100190, China.
          [2 ] IFSA Collaborative Innovation Center, Shanghai Jiao Tong University, Shanghai 200240, China.
          [3 ] Lawrence Livermore National Laboratory, 7000 East Avenue, Livermore, California 94551, USA.
          [4 ] Key Laboratory for Laser Plasmas (MoE) and Department of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China.
          [5 ] Photon Pioneers Center, Osaka University, 2-1 Yamada-oka, Suita, Osaka, 565-0871, Japan.
          [6 ] SUPA, Department of Physics, University of Strathclyde, Glasgow G4 0NG, United Kingdom.
          Article
          10.1103/PhysRevLett.114.255001
          26197129
          aac558e7-d45e-488b-9f83-14ae3879c8d0
          History

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