ACADSTAFF UGM
| Title | : | Inflation in a modified radiative seesaw model |
| Author | : |
Romy Hanang Setya Budhi, S.Si., M,Sc., Ph.D. (1) |
| Date | : | 2014 |
| Keyword | : | |
| Abstract | : | The existence of the inflationary era in the early Universe seems to be strongly supported by recent CMB observations. However, only a few realistic inflation scenarios which have close relation to particle physics seem to have been known unfortunately. The radiative neutrino mass model with inert doublet dark matter is a promising model for the present experimental issues which cannot be explained within the standard model. In order to make the model include inflation, we extend it by a complex scalar field with a specific potential. This scalar could be closely related to the neutrino mass generation at a TeV scale as well as inflation. We show that the inflation favored by the CMB observations could be realized even if inflaton takes sub-Planck values during inflation. |
| Group of Knowledge | : | Fisika |
| Original Language | : | |
| Level | : | Internasional |
| Status | : |
Published
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