Abstract
We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma.
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Notes
\(T _{{\scriptscriptstyle H}}\) grows with the oscillation amplitude \(\zeta \), but goes to the nonrelativistic period \(T _{{\scriptscriptstyle H}}^{{\scriptscriptstyle nr}} = \sqrt{\pi m/n_0e^2}\) as \(\zeta \rightarrow 0\).
With the initial conditions (6) and a non-vanishing v as considered here the invertibility of the map \(\mathbf{X}\mapsto \mathbf{x}_e(t,\mathbf{X})\) breaks also in an intermediate Z-range (\(Z_{{\scriptscriptstyle M}}\le Z \le Z_{{\scriptscriptstyle M}}'\)) for \(t \gtrsim T _{{\scriptscriptstyle H}}\).
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Fiore, G. On very short and intense laser–plasma interactions. Ricerche mat 65, 491–503 (2016). https://doi.org/10.1007/s11587-016-0270-3
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DOI: https://doi.org/10.1007/s11587-016-0270-3