2001
DOI: 10.1063/1.1373416
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Late-time hohlraum pressure dynamics in supernova remnant experiments

Abstract: It is shown that laser driven hohlraums obtain significant internal pressures which affect the hydrodynamics of high-energy density shock-tube experiments. By incorporating this previously neglected hohlraum pressure effect (in addition to the usual x-ray drive) into computer simulations which model the NOVA laser driven supernova remnant experiment [R. P. Drake, S. G. Glendinning, K. Estabrook, B. A. Remington, R. McCray, R. J. Williams, L. J. Suter, T. B. Smith, J. J. Carroll III, R. A. London, and E. Liang,… Show more

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Cited by 8 publications
(3 citation statements)
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“…Accelerating samples over such long time duration with a hohlraum generated x-ray drive (even multibarrel hohlraums [36,37]) without stagnation effects seems difficult. It has been known for years that significant late-time hohlraum internal pressures affect the hydrodynamics of HED experiments [38]. DD planar experiments are therefore a more attractive avenue for creating a long-duration (hundreds of ns) acceleration drive.…”
Section: Introductionmentioning
confidence: 99%
“…Accelerating samples over such long time duration with a hohlraum generated x-ray drive (even multibarrel hohlraums [36,37]) without stagnation effects seems difficult. It has been known for years that significant late-time hohlraum internal pressures affect the hydrodynamics of HED experiments [38]. DD planar experiments are therefore a more attractive avenue for creating a long-duration (hundreds of ns) acceleration drive.…”
Section: Introductionmentioning
confidence: 99%
“…Knowledge of this late-time pressure drive, and its accurate modeling, are important in the interpretation of experiments driven by hohlraum targets. 21,22 The target assembly consists of a 200-or 400-m-diam aluminum disk, set ͑flush with both faces͒ within a 1000-m-diam gold washer ͓Fig. 1͑b͔͒.…”
Section: Planar-shock Experimentsmentioning
confidence: 99%
“…Whereas this drive would allow to observe for the first time bubble-merging and bubble-competition in indirect-drive, it is unlikely that hundred of ns X-ray drive could be achieved that way. Hohlraum wall plasma expansion and stagnation on axis [18] constitute the final limiting parameters either from a diagnostic point of view or for the simulation of the experiments. Notwithstanding the fact that direct-drive illumination with beams concatenation in time is the most promising road to create a very long acceleration drive, we present an alternative approach to create a longer X-ray drive.…”
Section: Introductionmentioning
confidence: 99%