School of Mathematics and Physics, The Queen's University of Belfast, BT7 1NN Belfast, United Kingdom.
Phys Rev Lett. 2013 Jun 21;110(25):255002. doi: 10.1103/PhysRevLett.110.255002. Epub 2013 Jun 20.
The generation of ultrarelativistic positron beams with short duration (τ(e+) ≃ 30 fs), small divergence (θ(e+) ≃ 3 mrad), and high density (n(e+) ≃ 10(14)-10(15) cm(-3)) from a fully optical setup is reported. The detected positron beam propagates with a high-density electron beam and γ rays of similar spectral shape and peak energy, thus closely resembling the structure of an astrophysical leptonic jet. It is envisaged that this experimental evidence, besides the intrinsic relevance to laser-driven particle acceleration, may open the pathway for the small-scale study of astrophysical leptonic jets in the laboratory.
报道了一种从全光学装置中产生具有短持续时间(τ(e+) ≃ 30 fs)、小发散度(θ(e+) ≃ 3 mrad)和高密度(n(e+) ≃ 10(14)-10(15) cm(-3))的超相对论正电子束的方法。检测到的正电子束与具有相似光谱形状和峰值能量的高密度电子束和γ射线一起传播,因此非常类似于天体物理射流的结构。预计除了对激光驱动粒子加速具有内在的相关性之外,这种实验证据还可能为在实验室中对天体物理射流中的电子进行小规模研究开辟道路。