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 = \eta J_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 = \eta J_b,
full Ohm's law). This stems from the electrons being too energetic to fully
stop in the optimal hot spot depth.Comment: Minor revisions in response to referee comment
