  In this work, the s-wave, p-wave and d-wave holographic superconductors in
the Ho\v{r}ava-Lifshitz gravity are investigated in the probe limit. For the
present approach, it is shown that the equations of motion for different wave
states in Einstein gravity can be written into a unified form, and condensates
take place in all three cases. This scheme is then generalized to
Ho\v{r}ava-Lifshitz gravity, and an unified equation for multiple holographic
states is obtained. Furthermore, the properties of the condensation and the
optical conductivity are studied numerically. It is found that, in the case of
Ho\v{r}ava-Lifshitz gravity, it is always possible to find some particular
parameters in the corresponding Einstein case where the condensation curves are
identical. For fixed scalar field mass $m$, a non-vanishing $\alpha$ becomes
the condensation easier than in Einstein gravity for s-wave superconductor.
However, the p-wave and d-wave superconductors have $T_c$ greater than s-wave
one.
