Research Article

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

Table 8

Effects on the output of , , and at a low-energy scale, on varying for four different NTBM patterns (NO) at and  GeV.

mS (TeV)
246.57446.31646.39445.10134.43035.73633.93633.2928.6689.0698.9109.009
446.51246.25346.33245.03934.41835.72533.92533.2818.6449.0468.8878.986
646.47546.21646.29545.00334.41235.71833.91933.2748.6309.0338.8738.972
846.45046.19046.27044.97734.40735.71333.91433.2708.6209.0238.8638.962
1046.43046.17046.25044.95834.40335.71033.91033.2668.6129.0158.8558.954
1246.41446.15546.23544.94234.40035.70733.90733.2638.6069.0098.8498.948
1446.38646.12646.20644.91434.39635.70333.90333.2598.5918.9938.8348.933

mS (TeV) () ()
22.0182.0192.0202.0156.6026.6976.6076.6290.06880.06850.06860.0688
42.0332.0342.0352.0306.6756.7696.6816.7050.06870.06870.06870.0686
62.0472.0482.0492.0446.7326.8266.7376.7640.06870.06870.06870.0686
82.0442.0452.0462.0416.7286.8226.7346.7620.06840.06840.06840.0683
102.0452.0462.0472.0426.7366.8296.7426.7700.06830.06830.06830.0683
122.0482.0492.0512.0466.7516.8436.7576.7850.06830.06830.06830.0683
142.0512.0522.0542.0497.0477.1437.0547.0840.06820.06820.06820.0682