Relativistic Electron Transport in Preformed Overdense Plasma
One of the central issues in the concept of fast ignition is the energy transport from the ignition pulse through the overdense plasma corona of the precompressed fuel core. The laser converts a fraction of its energy into relativistic electrons in the MeV range, which have to propagate over a distance of a few 100 μm of overdense plasma to finally deposit their energy in the core and ignite it. The electron propagation in this environment is expected to be affected by collective effects due to fields and currents induced by the electron beam itself. The aim of this experiment is to investigate the mechanisms of energy losses of the hot electrons in overdense plasma.
In our experiment using the ATLAS-10 facility (setup in figure 1), the hot electron production occurs in a long scale length plasma produced by a synchronised Nd:glass laser delivering 12J in 3ns at 2ω. Using thin plastic, aluminum or copper foils as targets, 1D hydrodynamic simulations using the MULTI-code show the creation of a long underdense plasma with scale lengths of a few 100 μm and a region of overdense plasma several 10 μm thick. Sideview interferograms obtained by using a Wollaston prism (figure 2) and a subsequent Abel-inversion give excellent agreement between theory and experiment for the preplasma creation (figure 3).
A detailed characterization of the electron spectrum under different experimental conditions is under way.
Other diagnostics are ion TOF-detectors and a Thomson parabola to investigate the spectrum of ions that are accelerated at the backside of the target. The electrons exiting the target at the backside build up a strong electric field that ionises atoms on the back surface and subsequently accelerates them. The spectrum of these ions is directly correlated to the electron spectrum at the back surface of the target.