Inflation in a modified radiative seesaw model
| Autor: | Daijiro Suematsu, Shoichi Kashiwase, Romy H. S. Budhi |
|---|---|
| Rok vydání: | 2014 |
| Předmět: |
Physics
Inflation (cosmology) Nuclear and High Energy Physics Particle physics Cosmology and Nongalactic Astrophysics (astro-ph.CO) Physics beyond the Standard Model Dark matter Mass generation Cosmic microwave background FOS: Physical sciences Astrophysics::Cosmology and Extragalactic Astrophysics Inflaton High Energy Physics - Phenomenology General Relativity and Quantum Cosmology High Energy Physics - Phenomenology (hep-ph) Inflationary epoch Neutrino Astrophysics - Cosmology and Nongalactic Astrophysics |
| Zdroj: | Physical Review D. 90 |
| ISSN: | 1550-2368 1550-7998 |
| DOI: | 10.1103/physrevd.90.113013 |
| Popis: | 金沢大学理工研究域数物科学系 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. © 2014 American Physical Society. |
| Databáze: | OpenAIRE |
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