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Comment on 'The Lamb Shift and Ultra High Energy Cosmic Rays' and Comment on 'Vacuum Polarization Energy Losses of High Energy Cosmic Rays'

机译:评“羊羔位移和超高能宇宙射线”和   评“高能宇宙线的真空极化能量损失”

摘要

The cosmic rays spectrum has been shown to extend well beyond 10^20 eV. Withnearly 20 events observed in the last 40 years, it is now established thatparticles with energies near or above 10^21 eV. No nearby astrophysical objecthas been shown to correlate with the arrival directions of the highest energyevents, yet the exponential cut-off in the high energy end of the spectrum oneexpects to see in the case of far sources is not visible. It was recentlypointed out that the influence of the vacuum of quantum electrodynamics onparticle propagation could explain qualitatively this mystery. This note is acritic to these ideas.
机译:宇宙射线光谱已显示出远远超过10 ^ 20 eV。在过去40年中观察到近20个事件,现在可以确定能量接近或高于10 ^ 21 eV的粒子。没有显示附近的天体物体与最高能量事件的到达方向相关,但是人们看不到在远源情况下期望看到的光谱高能端的指数截止。最近指出,量子电动力学的真空对粒子传播的影响可以从质量上解释这个谜。本说明对这些想法有所评论。

著录项

  • 作者

    Deligny, Olivier;

  • 作者单位
  • 年度 2002
  • 总页数
  • 原文格式 PDF
  • 正文语种 {"code":"en","name":"English","id":9}
  • 中图分类

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