2012 Fiscal Year Final Research Report
Extended standard model with neutrino masses and dark matter
| Project/Area Number |
22740137
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| Research Category |
Grant-in-Aid for Young Scientists (B)
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| Allocation Type | Single-year Grants |
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| Research Field |
Particle/Nuclear/Cosmic ray/Astro physics
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| Research Institution | Kanazawa University |
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Principal Investigator |
AOKI Mayumi 金沢大学, 数物科学系, 助教 (70425601)
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| Project Period (FY) |
2010 – 2012
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| Keywords | ニュートリノ / 暗黒物質 |
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| Research Abstract |
Tiny neutrino masses and dark matter are beyond the scope of the standard model, so that an extension of the standard model is required to explain these phenomena. The radiative seesaw models can explain the neutrino masses by radiative corrections due to TeV-scale physics and some of them contain dark matter candidates. We studied phenomenological aspects of these models. It was found that such models are tested by future experiments.
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