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

Table 10

Effects on the output of , , and at a low-energy scale, on varying for four different NTBM patterns (IO) at and  GeV.

mS (TeV)
	2	45.762	45.481	45.590	44.307	34.339	35.646	33.847	33.206	8.190	8.550	8.453	8.522
4	45.791	45.511	45.619	44.335	34.326	35.632	33.833	33.192	8.200	8.561	8.463	8.532
6	45.808	45.528	45.635	44.352	34.318	35.624	33.825	33.184	8.206	8.568	8.470	8.538
8	45.819	45.540	45.647	44.363	34.312	35.619	33.820	33.179	8.210	8.573	8.474	8.542
10	45.828	45.549	45.656	44.372	34.308	35.615	33.816	33.175	8.213	8.577	8.478	8.546
12	45.836	45.556	45.663	44.380	34.305	35.611	33.813	33.171	8.216	8.580	8.481	8.549
14	45.842	45.564	45.670	44.386	34.303	35.610	33.811	33.170	8.219	8.582	8.483	8.551
mS (TeV)	()				()
	2	2.345	2.348	2.347	2.349	12.62	13.04	12.64	12.67	0.1084	0.1085	0.1084	0.1084
4	2.303	2.305	2.304	2.306	14.15	14.59	14.17	14.21	0.1078	0.1079	0.1079	0.1079
6	2.281	2.283	2.282	2.284	14.90	15.36	14.92	14.97	0.1076	0.1077	0.1076	0.1076
8	2.261	2.264	2.262	2.265	15.48	15.96	15.50	15.56	0.1074	0.1075	0.1074	0.1074
10	2.246	2.250	2.249	2.251	15.89	16.37	15.91	15.97	0.1072	0.1073	0.1072	0.1072
12	2.236	2.240	2.239	2.241	16.01	16.61	16.21	16.23	0.1071	0.1072	0.1071	0.1071
14	2.231	2.239	2.235	2.237	16.06	16.65	16.28	16.31	0.1070	0.1071	0.1070	0.1077