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Simulation of laser-driven,ablated plasma flows in collisionless shock experiments on OMEGA and the NIF
Authors:MJ Grosskopf  RP Drake  CC Kuranz  EM Rutter  JS Ross  NL Kugland  C Plechaty  BA Remington  A Spitkovsky  L Gargate  G Gregori  A Bell  CD Murphy  J Meinecke  B Reville  Y Sakawa  Y Kuramitsu  H Takabe  H-S Park
Institution:1. University of Michigan, Ann Arbor, MI, USA;2. Lawrence Livermore National Laboratory, Livermore, CA, USA;3. Princeton Univertsity, Princeton, NJ, USA;4. University of Oxford, Oxford, Oxfordshire, England, UK;5. Osaka University, Suita, Osaka, Japan;6. Laboratory for Laser Energetics, Rochester, NY, USA;7. ETH Science and Technology University, Zurich, Switzerland;8. Ecole Polytechnique, Palaiseau, France;9. Rice University, Houston, TX, USA;10. University of York, York, England, UK
Abstract:Experiments investigating the physics of interpenetrating, collisionless, ablated plasma flows have become an important area of research in the high-energy-density field. In order to evaluate the feasibility of designing experiments that will generate a collisionless shock mediated by the Weibel instability on the National Ignition Facility (NIF) laser, computer simulations using the Center for Radiative Shock Hydrodynamics (CRASH) radiation-hydrodynamics model have been carried out. This paper reports assessment of whether the experiment can reach the required scale size while maintaining the low interflow collisionality necessary for the collisionless shock to form. Comparison of simulation results with data from Omega experiments shows the ability of the CRASH code to model these ablated systems. The combined results indicate that experiments on the NIF are capable of reaching the regimes necessary for the formation of a collisionless shock in a laboratory experiment.
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