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We analyse the radiative stability of the next-to-tribimaximal mixings () with the variation of SUSY breaking scale () in MSSM, for both normal ordering (NO) and inverted ordering (IO) at the fixed input value of seesaw scale GeV and two different values of . All the neutrino oscillation parameters receive varying radiative corrections irrespective of the values at the electroweak scale, which are all within range of the latest global fit data at low value of (30). NO is found to be more stable than IO for all four different NTBM mixing patterns.

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