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

Cataclysmic variables in Globular clusters: First results on the analysis of the MOCCA simulations database