An understanding of radiation effects on the evolution of shock waves is of
great importance to many problems in astrophysics. Shock waves driven by a
laser-heated plasma are attractive for laboratory investigation of these p
henomena. Recent studies of intense short-pulse laser interactions with gas
es of atomic clusters indicate a potential avenue to access this regime of
radiative hydrodynamics. We have measured the energy absorption efficiency
of high-intensity, picosecond laser pulses in low-density gases composed of
large atomic clusters and find that the energy absorption can be very high
(> 95%), producing a high-temperature plasma filament which consequently p
roduces a strong blast wave. Interferometric characterization of these shoc
k waves indicates that in high-Z gases such as Xe, radiation transport play
s an important role in the evolution of the shock wave.