Second, we investigate the effects of the nonlinearity on the asymptotic behavior of the solutions. It is worthwhile to mention that for
0 < s < 12
, the asymptotic dominant term of Eq. (16) is charge term, Γ (r), and the presented solutions are not asymptotically AdS, but for
the cases s < 0 or s > 12
(include of s = n
2 ), the asymptotic behavior of rotating Einstein–nonlinear Maxwell field solutions are the same
as linear AdS case. It is easy to show that the electromagnetic field is zero for the cases s = 0, 1/2, and the metric function (16) does not
possess a charge term (Γ (r) = 0) and it corresponds to uncharged asymptotically AdS one.