  Plasmas of geometrically thick, black hole (BH) accretion flows in active
galactic nuclei (AGNs) are generally collisionless for protons, and involve
magnetic field turbulence. Under such conditions a fraction of protons can be
accelerated stochastically and create relativistic neutrons via nuclear
collisions. These neutrons can freely escape from the accretion flow and decay
into protons in dilute polar region above the rotating BH to form relativistic
jets. We calculate geometric efficiencies of the neutron energy and mass
injections into the polar region, and show that this process can deposit
luminosity as high as L_j ~ 2e-3 dot{M} c^2 and mass loading dot{M}_j ~ 6e-4
dot{M} for the case of the BH mass M ~ 1e8 M_sun, where dot{M} is mass
accretion rate. The terminal Lorentz factors of the jets are Gamma ~ 3, and
they may explain the AGN jets having low luminosities. For higher luminosity
jets, which can be produced by additional energy inputs such as Poynting flux,
the neutron decay still can be a dominant mass loading process, leading to
e.g., Gamma ~ 50 for L_{j,tot} ~ 3e-2 dot{M}c^2.
