Research Article

Stability of the Next-to-Tribimaximal Mixings under Radiative Corrections with the Variation of the SUSY Breaking Scale in MSSM

Table 2

The allowed input set of neutrino parameters at the high-energy scale  GeV and encompasses four different patterns. , , , and are estimated values, while the others are arbitrary allowed input values. In this paper, we consider both the NO and IO.

InputNO
Parameters
(eV)0.0120.0120.0120.012
(eV)
(eV)
34.41635.723433.922933.2824
45.809945.531445.636344.3539
8.2128.5728.4768.540
0000
180180180180
208.581200.957203.939203.864
Input
Parameters
(eV)IO0.0090.0090.0090.009
(eV)
(eV)
34.41635.723433.922933.2824
45.809945.531445.636344.3539
8.2128.5728.4768.540
0000
180180180180
208.582200.957203.939203.87