Final abundances in the static simulations after one second of neutron bombardment and at different physical conditions. Top left: n_n = 10²⁶ cm^-3 and T₉ = 2, top right: n_n = 10²⁸ cm^-3 and T₉ = 2, bottom left: n_n = 10²⁶ cm^-3 and T₉ = 4, bottom right: n_n = 10²⁸ cm^-3 and T₉ = 4. The solar abundance is shown in each case with vertical lines marking the location of the important peaks.