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A GRMHD model of disk outflows with neutrino-driven mass ejection ispresented. The model is used to calculate the structure of the outflow in thesub-slow magnetosonic region and the mass loading of the outflow, underconditions anticipated in the central engines of gamma-ray bursts. It isconcluded that magnetic launching of ultra-relativistic polar outflows is inprinciple possible along low inclination field lines (with respect to thesymmetry axis), provided the neutrino luminosity is sufficiently low,$L_\nu\simlt10^{52}$ erg s$^{-1}$.Comment: 6 pages, 2 figure

Neutrino‐Driven Mass Loading of GRMHD Outflows