Dirac dark matter in U (1)B - L with the Stueckelberg mechanism

被引:13
|
作者
Han, Chengcheng [1 ,2 ]
Lopez-Ibanez, Ml [3 ,4 ]
Peng, Bo [3 ,4 ]
Yang, Jin Min [3 ,4 ,5 ]
机构
[1] Sun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China
[2] KIAS, Sch Phys, 85 Hoegiro, Seoul 02455, South Korea
[3] Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
[4] Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R China
[5] Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, Japan
基金
中国国家自然科学基金;
关键词
NEUTRINO MASS; GENERATION;
D O I
10.1016/j.nuclphysb.2020.115154
中图分类号
O412 [相对论、场论]; O572.2 [粒子物理学];
学科分类号
摘要
We investigate a U(1)(B-L) gauge extension of the Standard Model (SM) where the gauge boson mass is generated by the Stueckelberg mechanism. Three right-handed neutrinos are added to cancel the gauge anomaly and hence the neutrino masses can be explained. A new Dirac fermion could be a WIMP dark matter whose interaction with the SM sector is mediated by the new gauge boson. Assuming the perturbativity of the gauge coupling up to the Planck scale, we find that only the resonance region is feasible for the dark matter abundance. After applying the Delta N-eff constraints from the current Planck experiment, the collider search constraints as well as the dark matter direct detection limits, we observe that the B - L charge of dark matter satisfies vertical bar Q(chi)vertical bar > 0.11. Such a scenario might be probed conclusively by the projected CMB-S4 experiment, assuming the right-handed neutrinos are thermalized with the SM sector in the early universe. (C) 2020 The Authors. Published by Elsevier B.V.
引用
收藏
页数:9
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