Speaker
Description
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.
| Session | Neutrino Physics |
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