Abstract. Simulations are presented of ignition-scale fast ignition targets with the integrated Zuma-Hydra PIC-hydrodynamic capability. We consider a 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, ignition can be achieved with fast electron energy E ig f = 30 kJ. This is 3.5× 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 = J b gives E ig f = 20 kJ, while using the full Ohm's law gives E ig f > 40 kJ. This is due to magnetic self-guiding in the former case, and ∇n × ∇T magnetic fields in the latter. Using a realistic, quasi two-temperature energy spectrum derived from PIC laser-plasma simulations increases E ig f to (102, 81, 162) kJ for (no E/B, E = J b , full Ohm's law). Such electrons are too energetic to stop in the optimal hot spot depth. This paper presents work on ignition-scale transport modelling of fast ignition [1] designs. By "transport" we mean the propagation and deposition of fast electrons, with reasonably self-consistent coupling to the background radiation-hydrodynamics. To achieve this we coupled the hybrid-PIC code Zuma [2,3] to the rad-hydro code Hydra [4]. A detailed publication on this work [3] reports laserplasma PIC modelling that shows a large fast-electron divergence, along with mitigation ideas based on imposed magnetic fields. Here we discuss the fast-electron energy needed for ignition, E ig f , of an artificially-collimated source. Using the resistive Ohm's law E = J b leads to magnetic self-guiding and reduces E ig f compared to runs with no E or B fields. However, using a more complete Ohm's law increases E ig f compared to the no-field case. This ordering applies both for a mono-energetic 1.5 MeV and PIC-based fast electron energy spectrum. The latter gives electrons that are too energetic to stop in the optimal hot spot, and raises E ig f ∼ 3.4× over the 1.5 MeV spectrum.