The reflectivity of relativistic ultra-thin electron layers
arXiv:0812.0703 · doi:10.1140/epjd/e2009-00082-0
Abstract
The coherent reflectivity of a dense, relativistic, ultra-thin electron layer is derived analytically for an obliquely incident probe beam. Results are obtained by two-fold Lorentz transformation. For the analytical treatment, a plane uniform electron layer is considered. All electrons move with uniform velocity under an angle to the normal direction of the plane; such electron motion corresponds to laser acceleration by direct action of the laser fields, as it is described in a companion paper. Electron density is chosen high enough to ensure that many electrons reside in a volume λ_R^3, where λ_R is the wavelength of the reflected light in the rest frame of the layer. Under these conditions, the probe light is back-scattered coherently and is directed close to the layer normal rather than the direction of electron velocity. An important consequence is that the Doppler shift is governed by γ_x=(1-(V_x/c)^2)^{-1/2} derived from the electron velocity component V_x in normal direction rather than the full γ-factor of the layer electrons.
7 pages, 4 figures, submitted to the special issue "Fundamental Physics with Ultra-High Fields" in The European Physical Journal D
References in corpus (4)
- Theory of high harmonic generation in relativistic laser interaction with overdense plasma
- Relativistic Doppler effect: universal spectra and zeptosecond pulses
- Relativistic plasma control for single attosecond pulse generation
- Coherent Thomson backscattering from laser-driven relativistic ultra-thin electron layers
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- Acceleration of ultra-thin electron layer. Analytical treatment compared with 1D-PIC simulation
- Coherent radiation reaction effects in laser-vacuum acceleration of electron bunches
- Determination of Carrier-Envelope Phase of Relativistic Few-Cycle Laser Pulses by Thomson Backscattering Spectroscopy
- Coherent keV backscattering from plasma-wave boosted relativistic electron mirrors
- Reflectivity and Spectrum of Relativistic Flying Plasma Mirrors
- Thomson backscattering from laser generated, relativistically moving high-density electron layers
- Single attosecond XUV pulse source via light-wave controlled relativistic laser-plasma interaction: Thomson Back Scattering Scheme