Dirac neutrino mass generation from a Majorana messenger

被引:12
作者
Calle, Julian [1 ]
Restrepo, Diego [1 ,2 ]
Zapata, Oscar [1 ,3 ]
机构
[1] Univ Antioquia, Inst Fis, Calle 70 52-21,Apartado Aereo 1226, Medellin, Colombia
[2] Univ Fed Rio Grande do Norte, Int Inst Phys, Campus Univ, BR-59078970 Natal, RN, Brazil
[3] Abdus Salam Int Ctr Theoret Phys, Str Costiera 11, I-34151 Trieste, Italy
关键词
DARK-MATTER; SYMMETRY; MODEL;
D O I
10.1103/PhysRevD.101.035004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The radiative type-I seesaw has been already implemented to explain the lightness of Majorana neutrinos with both Majorana and Dirac heavy fermions, and the lightness of Dirac neutrinos with Dirac heavy fermions. In this work, we present a minimal implementation of the radiative type-I seesaw with light Dirac neutrinos and heavy Majorana fcrmions. An inert doublet and a complex singlet scalar complete the dark sector, which is protected by an Abelian fermiophobic gauge symmetry that also forbids tree level mass contributions for the full set of light neutrinos. A fermion vectorlike extension of the model is also proposed where the light right-handed neutrinos can thermalize in the primordial plasma and the extra gauge boson can be directly produced at colliders. In particular, the current upper bound on Delta N-eff reported by PLANCK points to large ratios of M-Z'/g' greater than or similar to 40 TeV, which can be competitive with collider constraint for g' sufficiently large in the ballpark of the Standard Model values, while future cosmic microwave background experiments may probe all the no minimal models presented here.
引用
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页数:10
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