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Powerful attosecond pulses from relativistic mirrors

机译:来自相对论镜的强大阿秒脉冲

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Relatvistic Mirrors are an extremely promising route to generating high power attosecond radiation pulses in the XUV. The underlying principle relies on the temporal compression and upshifting of optical radiation when reflected from a relativistic reflector. Practical relativistic mirrors rely producing an electron sheet with a Lorentz factor γ1. Practical demonstration of relativistic mirrors is with can be produced with the ult be done by two Different approaches (Oscillating and Flying Mirror) will be discussed both theoretically and experimentally.
机译:相对反射镜是在XUV中产生高功率阿秒辐射脉冲的极有希望的途径。当从相对论反射器反射时,基本原理依赖于光辐射的时间压缩和上移。实用的相对论镜依赖于产生洛伦兹因数γ>> 1的电子薄片。相对论镜的实际演示可以用两种不同的方法(振荡镜和飞行镜)来完成,将在理论上和实验上进行讨论。

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