Plasma heating by the oscillating component of the pondermotive force of a very intense light wave is discussed.

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A high Mach number, radiatively cooled jet of astrophysical interest has been produced using intense laser irradiation of a gold cone. The evolution of the jet was imaged in emission and in radiography, and the temperature was measured with Thomson scattering. Comparison with numerical simulations shows that radiative cooling is a dominant mechanism in the collapse of the Au plasma jet on axis, with temperatures plummeting and peak densities increasing, each by an order of magnitude in ϳ 1 2 ns. In dimensionless terms, aspects of this jet are similar to radiative astrophysical jets. PACS numbers: 52.50.Jm, 52.65.Kj, 95.30.Qd, 98.62.Nx

In an experimental study of the physics of fast ignition the characteristics of the hot electron source at laser intensities up to 10 " Wcm"2and the heating produced at depth by hot electrons have been measured. Efficient generation of hot electrons but less than the anticipated heating have been observed.The concept of isochoric fast ignition originated by Tabak et al. ' is of importance through its potential to give higher inertially confined fusion (ICF) gain than isobaric central spark ignition used in the more developed indirect and direct drive schemes 'and thereby to reduce the driver efficiency required for inertial fusion energy (IFE). The physics is new and challenging involving strongly relativistic laser plasma interactions and transport of energy by MeV electrons where electrostatic potentials and self generated magnetic fields may strongly modify the transport 3. Experimental and theoretical studies aimed at assessing the feasibilityof fastignitionas a newrouteto ICF arenowbeing carried out at many laboratories world wide including the Lawrence Livennore National Laboratory (LLNL), where the Nova laser facility has been adapted to generate petawatt pulses using chirped puke ampliilcation (CPA)4 . Experimental FaciIityTwo beam lines at Nova have been adapted for CPA operation and for experiments reported here, generated typically 20J and 500J pulses respectively of duration in the range 0.4 to 20 ps (maximum power up to 1 PW). Focusing of the two beams respectively was with an off axis f73parabolic mirror of focal length 42 cm in a focal spot of 15 yrn diameter 1 and an axial f14parabola of focal length 170 cm in an asymmetrical spot of 40 pm x 20SThe focal spots had a speckle ,pattern sub structure with a broad power spec& of intensity. Work is in progress to correct the wavefront using a deformable mirror. T&b eam line produced a power weighted average intensity on target in 0.45 ps pulses estimated at 210'9 Wcm"2. The 500J, beam line produced 10 N Wcm'2 in 1 PW, 0.45 ps pulses. A thick glass plate debris shield protected the parabola in the 500J beam line for longer pulse operation down to 5 ps. Non linear effects precluded the me of the debris shield for lPW shots and here a plasma mirror was used to reverse the beam direction thus projecting ablated target debris away from the un-protected parabola. The off axis parabola was used with a thin debris shield for all pulse lengths in the 20 J experiments. Targets in these experiments were exposed to ASE and leakage prepulses before the main pulse. ASE in a typically 3 ns period before the pulse varied in experiments reported here from 210-5 to 2104 of the main pulse energy. The energy of leakage pulses ranged from 104 to 10'2of the main pulse, occurring 2 ns or 4 ns before the main pulse but could be made as low as 104 with precise adjustment of Pockels cell gates. The hot electron sourceA central theme of the experimental work has been the characterization of the hot electron source produced at a solid target. Electrons directed into the t...

We present the first simultaneous observations of ion acoustic and electron plasma waves in laserproduced dense plasmas with Thomson scattering. In addition to measuring the standard plasma parameters, electron temperature and density, this novel experimental technique is shown to be a sensitive method for temporally and spatially resolved measurements of the averaged ionization stage of the plasma. Experiments with highly ionized gold plasmas clearly show that the inclusion of dielectronic recombination in radiation-hydrodynamic modeling is critically important to model cooling plasmas.[S0031-9007(98)

Type Ia supernova explosion models: Homogeneity versus diversity AIP Conf.In studying complex astrophysical phenomena such as supernovae, one does not have the luxury of setting up clean, well-controlled experiments in the universe to test the physics of current models and theories. Consequently, creating a surrogate environment to serve as an experimental astrophysics testbed would be highly beneficial. The existence of highly sophisticated, modern research lasers, developed largely as a result of the world-wide effort in inertial confinement fusion, opens a new potential for creating just such an experimental testbed utilizing well-controlled, well-diagnosed laser-produced plasmas. Two areas of physics critical to an understanding of supernovae are discussed that are amenable to supporting research on large lasers: ͑1͒ compressible nonlinear hydrodynamic mixing and ͑2͒ radiative shock hydrodynamics.

We report a laser experiment of astrophysical interest on radiative jet formation. Conically shaped targets are irradiated by intense laser light. An ablated plasma flow collides at the axis of the cone targets, then propagates at high Mach number, forming a jetlike structure. We measure time-resolved x-ray self-emission images from the jets. The diameter of the jet increases with decreasing atomic number of the irradiated target, suggesting that the collimation is due to radiative cooling. Two-dimensional simulations reproduce essential features of the experimental results.