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Direct-Drive Inertial Confinement Fusion Implosions on Omega

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High Energy Density Laboratory Astrophysics

Abstract.

Direct-drive inertial confinement fusion (ICF) creates extreme states of matter. In current direct-drive cryogenic target implosions on the 60-beam OMEGA laser system, the compressed target has a measured pressure of 5 Gbar. These targets are hydrodynamically scaled from ignition targets for the National Ignition Facility. The ignition targets are predicted to have peak pressures of 3 Tbar after the target ignites. ICF target acceleration and deceleration are realized when hot, low-density plasma pushes against cold, high-density plasma, making the target implosion inherently susceptible to the Rayleigh-Taylor hydrodynamic instability (RTI). The unstable RTI growth causes mixing of cold, high-density shell plasma with the low-density, hot-spot plasma and reduces the primary neutron yield of the implosion. The strategy to control the RTI growth is to reduce the seeds (e.g., laser imprint and target-surface roughness) and the growth rates of the dominant modes. This paper reports on our recent experiments, progress in validating the hydrodynamics codes that are used to design future high-gain cryogenic DT targets, and techniques to improve target performance. A brief description is given of a new high energy petawatt laser — OMEGA EP (extended performance) — that is being added to the OMEGA compression facility.

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G.A. Kyrala

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© 2005 Springer

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Regan, S. et al. (2005). Direct-Drive Inertial Confinement Fusion Implosions on Omega. In: Kyrala, G. (eds) High Energy Density Laboratory Astrophysics. Springer, Dordrecht. https://doi.org/10.1007/1-4020-4162-4_32

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  • DOI: https://doi.org/10.1007/1-4020-4162-4_32

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  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-1-4020-3483-1

  • Online ISBN: 978-1-4020-4162-4

  • eBook Packages: Physics and AstronomyPhysics and Astronomy (R0)

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