A neutrino mass model with reflection symmetry

We demonstrate that an SU(2)(L) X U(1)(Y) model with the same particle content as Standard Model (SM) and discrete reflection symmetry between second and third generations of leptons gives rise to charged lepton and neutrino mass matrices which can accommodate the present solar, atmospheric, WMAP neutrino experimental results. The model predicts the value of \U-13\ which could be tested in neutrino factories and the effective Majorana neutrino mass (m) which is at the lower end of the present experimental value. Neutrino masses are generated through dim = 5 operators and the scale of which are constrained by the value of (m(ee)). If, in future neutrinoless double beta decay experiments namely, MOON, EXO, GENIUS shift the lower bound on (m(ee)) by one order, the present model will fail to accommodate the solar neutrino mixing angle due to LMA solution.