  Dynamical interactions in globular clusters (GCs) significantly impact the
formation and evolution of binary sources, including cataclysmic variables
(CVs). This study investigates the connection between dynamical states of GCs
and X-ray luminosity ($L_{x}$) distributions of CV populations through both
simulations and actual observations. Utilizing a Monte Carlo simulation tool,
MOCCA, we categorize the simulated GCs into three different evolutionary stages
which are referred to as Classes I/II/III. Significant differences are found in
the $L_{x}$ distributions of the CVs among these three Classes. In
observational aspects, we have analyzed 179 CV candidates in 18 GCs observed by
the {\it Chandra} X-ray Observatory. By dividing these GCs into three Families
of different dynamical ages, namely Families I/II/III, the $L_{x}$
distributions of the CV candidates also show significant differences among
these three Families. Both simulations and observational results suggest that
CVs in more dynamically evolved clusters (Class/Family III) exhibit brighter
X-ray emission. This highlights the influence of the dynamical status of a GC
on the properties of its hosted compact binaries. Similar to blue stragglers,
CV populations can serve as tracers of a GC's dynamical history. Our findings
provide insights for understanding the interplay between intracluster dynamics
and the evolution of compact binaries in GCs.
