  In this paper we present the spectrum of entropy/area for Kehagias-Sfetsos
(KS) black hole in Ho$\check{\textbf{r}}$ava-Lifshitz (HL)gravity via
quasi-normal modes (QNM) approach. We show that in the massive case the mass
parameter $\mu$ disappears in the entropy spectrum and only the quasinormal
modes modified by a term which is proportional to the mass square term. Our
calculations show that the charge like parameter $\frac{1}{2\omega}=Q^{2}$
appears in the surface gravity and our calculations can be applied to any
spherically symmetric spacetime which has only one physically acceptable
horizon. Our main difference between our calculations and what was done in
\cite{1} is that the portion of charge and mass is included explicitly in the
surface gravity and consequently in the QNM expression. Since the imaginary
part of the QNM is related to the adiabatic invariance of the system and also
to the entropy, surprisingly the mass parameter do not appear in the entropy
spectrum. Our conclusion supported by some acclaims about that the scalar field
parameters (charges) can not change the fundamental parameters in the
4-dimensional black holes.
