| Pramana | |
| Renormalization of seesaw neutrino masses in the standard model with two-Higgs doublets | |
| S Biramani Singh1  N Nimai Singh1 21  | |
| [1] Physics Department, Gauhati University, Guwahati 781 014, India$$ | |
| 关键词: Neutrino masses; radiative corrections; seesaw formula.; | |
| DOI : | |
| 学科分类:物理(综合) | |
| 来源: Indian Academy of Sciences | |
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【 摘 要 】
Using the theoretical ambiguities inherent in the seesaw mechanism, we derive the new analytic expressions for both quadratic and linear seesaw formulae for neutrino masses at low energies, with either up-type quark masses or charged lepton masses. This is possible through full radiative corrections arising out of the renormalizations of the Yukawa couplings, the coefï¬cients of the neutrino-mass-operator in the standard model with two-Higgs doublets, and also the QCD–QED rescaling factors below the top-quark mass scale, at one-loop level. We also investigate numerically the uniï¬cation of top-ð‘-ðœ Yukawa couplings at the scale ð‘€ð¼=0.59× 108GeV for a ï¬xed value of tan ð›½=58.77, and then evaluate the seesaw neutrino masses which are too large in magnitude to be compatible with the presently available solar and atmospheric neutrino oscillation data. However, if we consider a higher but arbitrary value of ð‘€ð¼=0.59× 1011GeV, the predictions from linear seesaw formulae with charged lepton masses, can accommodate simultaneousely both solar atmospheric neutrino oscillation data.
【 授权许可】
Unknown
【 预 览 】
| Files | Size | Format | View |
|---|---|---|---|
| RO201912040495576ZK.pdf | 135KB |
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