138 / 2023-04-14 16:55:36
Coherent subcycle optical shock from superluminal plasma wake
subcycle pulse,coherent radiation,superluminal plasma wake,attosecond pulse
摘要录用
浩 彭 / Shenzhen Technology University
Taiwu Huang / Shenzhen Technology University
Ke Jiang / Shenzhen Technology University
Ran Li / Shenzhen Technology University
Chaoneng Wu / Shenzhen Technology University
Mingyang Yu / Shenzhen Technology University
Caterina Riconda / CNRS;LULI;Sorbonne university;Ecole Polytechnique;CEA
Stefan Weber / ELI-Beamlines; Academy of Sciences of the CR
Cangtao Zhou / Shenzhen Technology University
Shuangchen Ruan / Shenzhen Technology University
High-energy subcycle radiation pulses are useful for many applications. For many applications, it is desired to have high intensity, tunable frequency, stable carrier envelope phase (CEP), and foremost a simple setup. However, to our best knowledge, currently there is not such a radiation source that possesses all these desired properties simultaneously. We report a new regime of generating subcycle pulses by simply directing a relativistic electron beam (REB) into a plasma with slowly varying density up-ramp[1]. We show that the sheath electrons flowing along the boundary of the REB-induced plasma wake emit strong spontaneous radiations at the rear of

the bubble (ROB), and they are coherently overlapped at the Cherenkov angle when the wake phase velocity is superluminal. This new coherence mechanism[2] does not require bunching the radiating particles in a spatial region smaller than the radiation wavelength as that in existing coherent radiation sources[3]. Three-dimensional (3D) particle-in-cell (PIC) and far-field time-domain radiation simulations confirm that an isolated subcycle pulse in the form of an optical shock is generated at the rear of a superluminal wake bubble induced by the REB. In particular, such radiation has many interesting and unique features. It is CEP stable, as well as of subcycle attosecond-scale duration. It has also excellent directionality, namely at the Cherenkov angle with very small angular divergence, and high intensity that scales with the square of the propagation distance. In addition, the frequency can be readily tuned by adjusting the densities of the plasma and REB.

 
重要日期
  • 会议日期

    06月05日

    2023

    06月09日

    2023

  • 04月30日 2023

    提前注册日期

  • 05月01日 2023

    摘要截稿日期

  • 05月01日 2023

    摘要录用通知日期

  • 05月01日 2023

    初稿截稿日期

  • 05月31日 2023

    注册截止日期

主办单位
等离子体物理重点实验室
北京师范大学天文系
承办单位
Matter and Radiation at Extremes期刊
中国工程物理研究院流体物理研究所
北京应用物理与计算数学研究所
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