11.12.2012 Views

Lecture Notes in Physics

Lecture Notes in Physics

Lecture Notes in Physics

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

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]).

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!