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We propose a new scenario in a radiative seesaw model based on A_4 flavorsymmetry. In this model, we explore a possibility of linking non-zero\theta_{13} to dark matter. And we analyze the lepton sector to predict theobserved neutrinos and mixings, especially obtaining a lower bound of\theta_{13}~3.5 [Deg.]. We show that the non-zero \theta_{13} is correlatedwith our heavy Majorana type of dark matter. Also we predict that the mass beO(1-10) TeV, as a result of analyzing the Wilkinson-Microwave-Anisotropy-Probeand lepton flavor violation.

Non-zero \theta_{13} linking to Dark Matter from Non-Abelian Discrete Flavor Model in Radiative Seesaw