Time evolution of the accretion rate, Eddington outflow, and black hole mass of the simulation with Σ₀ = 30 M_⊙ pc⁻² and b_cool = 6. Even before the bar potential is switched on completely (186 Myr), there is strong clumpy accretion. The inner disk mass rises quickly and high accretion rates up to 2 M_⊙   yr ⁻¹ are attained. Later on the Eddington outflow declines much more quickly than the accretion rate. This suggests a decrease in the clumpy accretion.