Flavor-specific dark matter signatures through the lens of neutrino oscillations

被引:0
|
作者
Bhattacharya, Subhaditya [1 ]
Fabian, Sven [2 ]
Herms, Johannes [2 ]
Jana, Sudip [2 ]
机构
[1] Indian Inst Technol, Dept Phys, Gauhati 781039, Assam, India
[2] Max Planck Inst Kernphys, Saupfercheckweg 1, D-69117 Heidelberg, Germany
来源
JOURNAL OF COSMOLOGY AND ASTROPARTICLE PHYSICS | 2025年 / 01期
关键词
neutrino properties; cosmic ray theory; dark matter theory; ZEE-BABU MODEL; LEPTON NUMBER; GAMMA-RAY; MASSES; ELECTRONS; SEESAW; VIOLATION; MIXINGS; EXCESS; SIGNAL;
D O I
10.1088/1475-7516/2025/01/110
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We investigate the flavor-specific properties of leptophilic dark matter in neutrino mass models, where dark matter signals are directly correlated with the neutrino oscillation data, providing complementary insights into the neutrino mass hierarchy and CP phases. Notably, this can be accomplished without introducing a flavor-specific portal to dark matter, imposing any new flavor symmetry, or involving flavon fields. As a case study, we analyze the correlation between the flavor-philic nature of dark matter and neutrino oscillation data in the type-II seesaw and Zee-Babu models, and extend this discussion to other neutrino mass models. We analyze the indirect signatures of such leptophilic dark matter, specifically examining the spectrum of the cosmic ray electron/positron flux resulting from the pair annihilation of dark matter in the Galactic halo, and explore correlated lepton-specific signals at collider experiments sensitive to neutrino oscillation data.
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页数:38
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