  Motivated by recent works [1,2], the influences of self-gravitational
interaction on the Hawking radiation are studied both for (3 + 1) and (4 + 1)
dimensional black holes in $z = 4$ Ho\u{r}ava-Lifshitz gravity. It is found
that the tunneling entropies $S_{B(3 + 1)}$ and $S_{B(4 + 1)}$ independent on
particle's mass are consistent with the thermodynamical entropies $S_{BH(3 +
1)}$ and $S_{BH(4 + 1)}$, respectively. There is a very visible degree of
uniformity between thermodynamics and quantum tunneling in $z = 4$
Ho\u{r}ava-Lifshitz gravity. It suggests that the entropies contained corrected
terms could be explained well by the self-gravitational interaction of Hawking
radiation. The study of tunneling process may shed light on understanding the
Ho\u{r}ava-Lifshitz gravity.
