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arXiv 1111.5089physics.plasm-ph
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Cone-Guided Fast Ignition with no Imposed Magnetic Fields

D. J. Strozzi, M. Tabak, D. J. Larson, M. M. Marinak, M. H. Key, L. Divol, A. J. Kemp, C. Bellei, H. D. Shay

英文摘要:

Simulations of ignition-scale fast ignition targets have been performed with the new integrated Zuma-Hydra PIC-hydrodynamic capability. We consider an idealized spherical DT fuel assembly with a carbon cone, and an artificially-collimated fast electron source. We study the role of E and B fields and the fast electron energy spectrum. For mono-energetic 1.5 MeV fast electrons, without E and B fields, the energy needed for ignition is E_f^{ig} = 30 kJ. This is about 3.5x the minimal deposited ignition energy of 8.7 kJ for our fuel density of 450 g/cm^3. Including E and B fields with the resistive Ohm's law E = ηJ_b gives E_f^{ig} = 20 kJ, while using the full Ohm's law gives E_f^{ig} > 40 kJ. This is due to magnetic self-guiding in the former case, and \nabla n \times \nabla T magnetic fields in the latter. Using a realistic, quasi two-temperature energy spectrum derived from PIC laser-plasma simulations increases E_f^{ig} to (102, 81, 162) kJ for (no E/B, E = ηJ_b, full Ohm's law). This stems from the electrons being too energetic to fully stop in the optimal hot spot depth.

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