Dirac dark matter in U (1)B - L with the Stueckelberg mechanism
被引:13
|
作者:
Han, Chengcheng
论文数: 0引用数: 0
h-index: 0
机构:
Sun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China
KIAS, Sch Phys, 85 Hoegiro, Seoul 02455, South KoreaSun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China
Han, Chengcheng
[1
,2
]
Lopez-Ibanez, Ml
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R ChinaSun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China
Lopez-Ibanez, Ml
[3
,4
]
Peng, Bo
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R ChinaSun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China
Peng, Bo
[3
,4
]
Yang, Jin Min
论文数: 0引用数: 0
h-index: 0
机构:
Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China
Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R China
Tohoku Univ, Dept Phys, Sendai, Miyagi 9808578, JapanSun Yat Sen Univ, Sch Phys, Guangzhou 510275, Peoples R China
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
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.
机构:
Univ Fed Sao Paulo, Dept Ciencias Exatas & Terra, BR-09972270 Sao Paulo, BrazilUniv Fed Sao Paulo, Dept Ciencias Exatas & Terra, BR-09972270 Sao Paulo, Brazil
Alves, Alexandre
论文数: 引用数:
h-index:
机构:
Berlin, Asher
Profumo, Stefano
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA
Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USAUniv Fed Sao Paulo, Dept Ciencias Exatas & Terra, BR-09972270 Sao Paulo, Brazil
Profumo, Stefano
Queiroz, Farinaldo S.
论文数: 0引用数: 0
h-index: 0
机构:
Univ Calif Santa Cruz, Dept Phys, Santa Cruz, CA 95064 USA
Univ Calif Santa Cruz, Santa Cruz Inst Particle Phys, Santa Cruz, CA 95064 USA
Texas A&M Univ, Mitchell Inst Fundamental Phys & Astron, Dept Phys & Astron, College Stn, TX 77843 USA
Max Planck Inst Kernphys, D-69117 Heidelberg, GermanyUniv Fed Sao Paulo, Dept Ciencias Exatas & Terra, BR-09972270 Sao Paulo, Brazil