  Many studies have analyzed planetary occurrence rates and their dependence on
the host's properties to provide clues to planet formation, but few have
focused on the mutual occurrence ratio of different kinds of planets. Such
relations reveal whether and how one type of planet evolves into another, e.g.
from a cold Jupiter to a warm or even hot Jupiter, and demonstrate how stellar
properties impact the evolution history of planetary systems. We propose a new
classification of giant planets, i.e. cold Jupiter(CJ), warm Jupiter(WJ), and
hot Jupiter(HJ), according to their position relative to the snow line in the
system. Then, we derive their occurrence rates(${\eta}_{\rm HJ}$, ${\eta}_{\rm
WJ}$, ${\eta}_{\rm CJ}$) with the detection completeness of RV(Radial Velocity)
surveys(HARPS$\&$ CORALIE) considered. Finally, we analyze the correlation
between the mutual occurrence ratios, i.e. ${\eta}{_{\rm CJ}} / {\eta}_{\rm
WJ}$, ${\eta}{_{\rm CJ}} / {\eta}_{\rm HJ}$ or ${\eta}{_{\rm WJ}}/{\eta}_{\rm
HJ}$, and various stellar properties, e.g. effective temperature $T_{\rm eff}$.
Our results show that the ${\eta}_{\rm HJ}$, ${\eta}_{\rm WJ}$ and ${\eta}_{\rm
CJ}$ are increasing with the increasing $T_{\rm eff}$ when $T_{\rm eff}\in
(4600,6600] K$. Furthermore, the mutual occurrence ratio between CJ and WJ,
i.e. ${\eta}{_{\rm CJ}} /{\eta}_{\rm WJ}$, shows a decreasing trend with the
increasing $T_{\rm eff}$. But, both ${\eta}{_{\rm CJ}}/{\eta}_{\rm HJ}$ and
${\eta}{_{\rm WJ}}/{\eta}_{\rm HJ}$ are increasing when the $T_{\rm eff}$
increases. Further consistency tests reveal that the formation processes of WJ
and HJ may be dominated by orbital change mechanisms rather than the in-situ
model. However, unlike WJ, which favors gentle disk migration, HJ favors a more
violent mechanism that requires further investigation.
