Double type-II seesaw scenario, baryon asymmetry, and dark matter for cosmic e± excesses

被引:38
作者
Gu, Pei-Hong [1 ]
He, Hong-Jian [2 ]
Sarkar, Utpal [3 ,4 ,5 ]
Zhang, Xinmin [6 ]
机构
[1] Abdus Salam Int Ctr Theoret Phys, I-34014 Trieste, Italy
[2] Tsinghua Univ, Ctr High Energy Phys, Beijing 100084, Peoples R China
[3] Phys Res Lab, Ahmadabad 380009, Gujarat, India
[4] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[5] Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
[6] Chinese Acad Sci, Inst High Energy Phys, Beijing 100049, Peoples R China
基金
中国国家自然科学基金;
关键词
NEUTRINO MASSES; BARYOGENESIS; HIGGS; MODEL; PARTICLES; VIOLATION; ENERGIES; MIXINGS; TRIPLET;
D O I
10.1103/PhysRevD.80.053004
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We construct a new realization of type-II seesaw for neutrino masses and baryon asymmetry by extending the standard model with one light and two heavy singlet scalars besides one Higgs triplet. The heavy singlets pick up small vacuum expectation values to give a suppressed trilinear coupling between the triplet and doublet Higgs bosons after the light singlet drives the spontaneous breaking of lepton number. The Higgs triplet can thus remain light and be accessible at the LHC. The lepton-number conserving decays of the heavy singlets can generate a lepton asymmetry stored in the Higgs triplet to account for the matter-antimatter asymmetry in the Universe. We further introduce stable gauge bosons from a hidden sector, which obtain masses and annihilate into the Higgs triplet after spontaneous breaking of the associated non-Abelian gauge symmetry. With Breit-Wigner enhancement, the stable gauge bosons can simultaneously explain the relic density of dark matter and the cosmic positron/electron excesses.
引用
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页数:8
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