Numerical consistency check between two approaches to radiative corrections for neutrino masses and mixings
arXiv:hep-ph/0407185 · doi:10.1007/BF02705276
Abstract
We briefly outline the two popular approaches on radiative corrections to neutrino masses and mixing angles, and then carry out a detailed numerical analysis for a consistency check between them in MSSM. We find that the two approaches are nearly consistent with a small discrepancy of a factor of 13 percent in mass eigenvalues at low energy scale, but the predictions on mixing angles are almost consistent. We check the stability of the three types of neutrino models, i.e., hierarchical, inverted hierarchical and degenerate models, under radiative corrections, using both approaches, and find consistent conclusions. The neutrino mass models which are found to be stable under radiative corrections in MSSM are the normal hierarchical model and the inverted hierarchical model with opposite CP parity. We also carry out numerical analysis on some important conjectures related to radiative corrections in MSSM, viz., radiative magnification of solar and atmospheric mixings in case of nearly degenerate model having same CP parity (MPR conjecture) and radiative generation of solar mass scale in exactly two-fold degenerate model with opposite CP parity and non-zero reactor angle (JM conjecture). We observe certain exceptions to these conjectures. Finally the effect of scale-dependent vacuum expectation value in neutrino mass renormalisation is discussed.
26 pages, 5 figures,references added, typos corrected and text modified
References in corpus (23)
- Renormalization of the Neutrino Mass Operator
- Running Neutrino Masses, Mixings and CP Phases: Analytical Results and Phenomenological Consequences
- Renormalization Group Equations for Seesaw Neutrino Masses
- Neutrino Mass Operator Renormalization Revisited
- Can Neutrinos be Degenerate in Mass?
- Quantum corrections to neutrino masses and mixing angles
- The Dark Side of the Solar Neutrino Parameter Space
- Naturalness of nearly degenerate neutrinos
- Fixed points in the evolution of neutrino mixings
- Renormalisation Group Analysis of Single Right-handed Neutrino Dominance
- Stability of the Lepton-Flavor Mixing Matrix Against Quantum Corrections
- The LMA Solution from Bimaximal Lepton Mixing at the GUT Scale by Renormalization Group Running
- Neutrino Unification
- Testing neutrino mass matrices with approximate L_e-L_mu-L_tau symmetry
- Large mixing angles for neutrinos from infrared fixed points
- Predictive Framework with a Pair of Degenerate Neutrinos at a high scale
- Radiative origin of solar scale and U_{e3}
- Lepton Flavor Violation and Radiative Neutrino Masses
- Bimaximal Mixings from the Texture of the Right-handed Majorana Neutrino Mass Matrix
- Right-handed Majorana Neutrino Mass Matrices for Generating Bimaximal Mixings in Degenerate and Inverted Models of Neutrinos
- Theory of Neutrino Masses and Mixings
- Effects of the Scale-dependent Vacuum Expectation Values in the Renormalization Group Analysis of Neutrino Masses
- Inverted Hierarchical Model of Neutrino Masses Revisited
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- Discriminating neutrino mass models using Type II seesaw formula
- Quasi-Degenerate Neutrinos in Type II Seesaw Models
- Lowering solar mixing angle in inverted hierarchy without charged lepton corrections
- Deviations from Tribimaximal and Golden Ratio mixings under radiative corrections of neutrino masses and mixings