  In this first investigation of the MOCCA database with respect to cataclysmic
variables, we found that for models with Kroupa initial distributions,
considering the standard value of the efficiency of the common-envelope phase
adopted in BSE, no single cataclysmic variable was formed only via binary
stellar evolution, i. e., in order to form them, strong dynamical interactions
have to take place. Our results also indicate that the population of
cataclysmic variables in globular clusters are, mainly, in the last stage of
their evolution and observational selection effects can change drastically the
expected number and properties of observed cataclysmic variables.
