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We consider two optimally mixed neutralino dark matter models, based onnonuniversal gaugino masses, which were recently proposed by us to achieve WMAPcompatible relic density over a large part of the MSSM parameter space. Wecompare the resulting predictions for the spin-independent DM scatteringcross-section with the recent CDMS II data, assuming the possibility of the tworeported candidate events being signal events. For one model the predictedcross-section agrees with the putative signal over a small part of theparameter space, while for the other the agreement holds over the entire WMAPcompatible parameter space of the model.

Comparing the Predictions of two Mixed Neutralino Dark Matter Models with the Recent CDMS II Candidate Events