Effects of Variations of SUSY Breaking Scale on Neutrino Oscillaton Parameters at Low Energy Scale Under Radiative Corrections for Different Values of  \(\tan \beta \)

Using renormalisation group equations (RGEs) we study the radiative corrections of different models of neutrino mass patterns at different values of high seesaw scale \(M _R\) and \(\tan \beta \) with the variation of SUSY breaking scale \(m_s\) . Different neutrino mass patterns are found to behave differently under the analysis. Small value of \(\tan \beta \) is found preferable for NH case wheres higher value of \(\tan \beta \) is found favorable for IH case. A self-complementarity relation among the three leptonic mixing angles is employed and it is found to be invariant against radiative correction. Both NH and IH prefer the high SUSY breaking scale \(m_s\) . Different neutrino oscillation parameters receive varying radiative corrections under the analysis.