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Generation of Terawatt Attosecond Pulses from Relativistic Transition Radiation

ORAL

Abstract

When a femtosecond duration and hundreds of kiloampere peak current electron beam traverses the vacuum and high-density plasma interface, a new process, that we call relativistic transition radiation (RTR), generates an intense ∼100 as pulse containing ∼1 terawatt power of coherent vacuum ultraviolet (VUV) radiation accompanied by several smaller femtosecond duration satellite pulses. This pulse inherits the radial polarization of the incident beam field and has a ring intensity distribution. This RTR is emitted when the beam density is comparable to the plasma density and the spot size much larger than the plasma skin depth. Physically, it arises from the return current or backward relativistic motion of electrons starting just inside the plasma that Doppler up shifts the emitted photons. The number of RTR pulses is determined by the number of groups of plasma electrons that originate at different depths within the first plasma wake period and emit coherently before phase mixing.

Publication: Physical Review Letters 126, 094801 (2021)

Presenters

  • Xinlu Xu

    SLAC - Natl Accelerator Lab

Authors

  • Xinlu Xu

    SLAC - Natl Accelerator Lab

  • David Cesar

    University of California, Los Angeles

  • Sebastien Corde

    LOA, ENSTA Paris, CNRS, Ecole Polytechnique, Institut Polytechnique de Paris

  • Vitaly Yakimenko

    SLAC - Natl Accelerator Lab

  • Mark J Hogan

    SLAC - Natl Accelerator Lab

  • Chandrashekhar Joshi

    University of California, Los Angeles

  • Agostino Marinelli

    SLAC National Accelerator Laboratory

  • Warren B Mori

    University of California, Los Angeles