Inverted Hierarchical Model of Neutrino Masses Revisited

Mahadev Patgiri; N. Nimai Singh

doi:10.1016/j.physletb.2003.06.021

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arXiv · hep-ph/0306252

Inverted Hierarchical Model of Neutrino Masses Revisited

Mahadev Patgiri·N. Nimai Singh

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Abstract

In this letter we highlight the inherent problems associted with the inverted hierarchical model of neutrinos with only three generations and suggest possible solutions within the MSSM. we discuss the new parametrisation of the solar mixing angle which can identify the light side and dark side of the data. We then argue whether the inverted hierarchical neutrino mass matrix can explain the large mixing angle(LMA) MSW solution of the solar neutrino anomaly in the presence of an appropriate texture of charged lepton mass matrix. In model independent way we explore such specific form of the charged lepton mass matrix having special structure in 1-2 block. The contribution to the solar mass splitting arising out of radiative corrections in MSSM, is calculated, thus making the model stable under radiative corrections.

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Mahadev Patgiri, N. Nimai Singh. 2003-06-25. Inverted Hierarchical Model of Neutrino Masses Revisited. https://doi.org/10.1016/j.physletb.2003.06.021

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