“…They have been widely employed in the baryon sector, to calculate the static [27,28,29,30] and dynamic properties [31,32,33,34,35,36] of the nucleon and to describe strange baryons [28,37,38,39]. The CDM has also been applied in the quark sector, to calculate the EOS of quark matter [40,41,42,43,44] and to study the stability of strange quark matter [45]. Applications of the CDM EOS for quark matter to the study of compact stars have been considered by Ghosh et al [46] and by Drago and collaborators, who studied the structure of hybrid stars [47,48] and the problem of supernova explosions [49], and, more recently by Malheiro et al [50,51] to study pure quark stars.…”