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16 H. Schwoerer<br />
Emax =4γ 2 wm0c 2 , lmax ≈ γ 2 w ·c/ωp , with γw =<br />
1<br />
. (2.10)<br />
1 − (ωp/ω) 2<br />
Remark that the Lorentz factor γw of the plasma wave does depend only on<br />
its phase velocity, which is determ<strong>in</strong>ed by the dispersion relation of the plasma<br />
or, <strong>in</strong> other words, by the ratio of the plasma density to the critical density.<br />
In particular, the maximum energy ga<strong>in</strong> of an electron <strong>in</strong> a wakefield does not<br />
depend on the light <strong>in</strong>tensity. The light <strong>in</strong>tensity basically has to provide the<br />
plasma density modulation over a long distance. As <strong>in</strong> the case of the ponderomotive<br />
acceleration, electrons enter the wakefield with different velocities<br />
and on different phases with respect to the plasma wave. Consequently, the<br />
energy ga<strong>in</strong> and the correspond<strong>in</strong>g spectrum of the emitted electrons is broad<br />
and even Boltzmann like, so that aga<strong>in</strong> a temperature can be attributed to<br />
the wakefield accelerated electrons. Typical experimentally achieved energy<br />
ga<strong>in</strong>s are <strong>in</strong> the MeV range (see [8, 10] and references there<strong>in</strong>).<br />
2.3.4 Self-Focuss<strong>in</strong>g and Relativistic Channel<strong>in</strong>g<br />
In the discussion so far we have described only the effect of the light field<br />
onto the plasma. Because of its dispersion relation, the plasma modifies vice<br />
versa the propagation of the laser pulse. We will see that even though complex<br />
<strong>in</strong> detail, the overall effect simplifies and optimizes the electron acceleration<br />
process.<br />
The <strong>in</strong>dex of refraction of a plasma was given by (2.1):<br />
<br />
npl =<br />
1 − ω2 pl<br />
=<br />
ω2 1 −<br />
nee2 . (2.11)<br />
γm0ɛ0ω2 In the current context we have to discuss the <strong>in</strong>fluence of the electron density<br />
ne on the light propagation. We know that the ponderomotive force of<br />
the laser beam pushes electrons <strong>in</strong> radial direction out of the optical axis: a<br />
hollow channel is generated along the laser propagation (see Fig. 2.6 [left]).<br />
From the numerator <strong>in</strong> (2.1) we see that the speed of light <strong>in</strong> the plasma<br />
(determ<strong>in</strong>ed by vp = c/npl) <strong>in</strong>creases with <strong>in</strong>creas<strong>in</strong>g electron density. Therefore,<br />
the ponderomotively <strong>in</strong>duced plasma channel acts as a positive lens on<br />
the laser beam. From the denom<strong>in</strong>ator <strong>in</strong> (2.1) we see that the same effect is<br />
caused by the relativistic mass <strong>in</strong>crease of the electrons, which is larger on the<br />
optical axis of the beam than <strong>in</strong> its w<strong>in</strong>gs. From their orig<strong>in</strong> these mechanisms<br />
are called ponderomotive and relativistic self-focuss<strong>in</strong>g, respectively. In competition<br />
with the natural diffraction of the beam and further ionization, both<br />
effects lead to a filamentation of the laser beam over a distance, which can<br />
be much longer than the confocal length (Rayleigh length) of the focuss<strong>in</strong>g<br />
geometry. This channel<strong>in</strong>g can be beautifully monitored through the nonl<strong>in</strong>ear<br />
Thomson scatter<strong>in</strong>g of the relativistic electrons <strong>in</strong> the channel, which is<br />
the emission of the figure-of-eight electron motion at harmonics of the laser<br />
frequency (see Fig. 2.6 and [11, 12]).