Leptogenesis and LHC Physics with Type III See-Saw
arXiv:0901.1264 · doi:10.1142/S2010194511000067
Abstract
The See-Saw mechanism provides a nice way to explain why neutrino masses are so much lighter than their charged lepton partners. It also provides a nice way to explain baryon asymmetry in our universe via the leptogenesis mechanism. In this talk we review leptogenesis and LHC physics in a See-Saw model proposed in 1989, now termed the Type III See-Saw model. In this model, triplet leptons are introduced with the neutral particles of the triplets playing the role of See-Saw. The triplet leptons have charged partners with standard model gauge interactions resulting in many new features. The gauge interactions of these particles make it easier for leptognesis with low masses, as low as a TeV is possible. The gauge interactions also make the production and detection of triplet leptons at LHC possible. The See-Saw mechanism and leptogenesis due to Type III See-Saw may be tested at LHC.
10 pages with three figures. Invited pleanry talk at COSPA2008, APCTP, Pohang, Korea, 28/10 - 1/11, 2008
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Cited by in corpus (6)
- Leptogenesis in fast expanding Universe
- Radiative Neutrino Mass in Type III Seesaw Model
- Common origin of radiative neutrino mass, dark matter and leptogenesis in scotogenic Georgi-Machacek model
- Neutrino mixing and Leptogenesis with modular symmetry in the framework of type III seesaw
- Minimal Leptogenesis in Brane-inspired Cosmology
- Probing leptogenesis and the minimal neutrino seesaw mechanism through gravitational waves