Abstract
We construct a supersymmetric (SUSY) extension of an invisible axion model, in which the Peccei-Quinn symmetry is broken naturally at the intermediate mass scale 1010-1012 GeV by radiative corrections from right-handed neutrino loops. The SUSY-invariant mass of doublet Higgs supermultiplets is forbidden by the Peccei-Quinn symmetry, whose breaking, however, generates an invariant Higgs mass of the order of the Fermi scale. In this model the right-handed neutrinos acquire large Majorana masses which are in a favored range for the Mikheyev-Smirnov-Wolfenstein solution to the solar neutrino problem.
| Original language | English |
|---|---|
| Pages (from-to) | 418-425 |
| Number of pages | 8 |
| Journal | Physics Letters B |
| Volume | 291 |
| Issue number | 4 |
| DOIs | |
| Publication status | Published - Oct 1 1992 |
| Externally published | Yes |
All Science Journal Classification (ASJC) codes
- Nuclear and High Energy Physics
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Murayama, H., Suzuki, H., & Yanagida, T. (1992). Radiative breaking of Peccei-Quinn symmetry at the intermediate mass scale. Physics Letters B, 291(4), 418-425. https://doi.org/10.1016/0370-2693(92)91397-R