Non-standard interactions in radiative neutrino mass models

被引:98
|
作者
Babu, K. S. [1 ,2 ]
Dev, P. S. Bhupal [2 ,3 ,4 ]
Jana, Sudip [1 ,2 ]
Thapa, Anil [1 ,2 ]
机构
[1] Oklahoma State Univ, Dept Phys, Stillwater, OK 74078 USA
[2] Fermilab Natl Accelerator Lab, Theoret Phys Dept, POB 500, Batavia, IL 60510 USA
[3] Washington Univ, Dept Phys, St Louis, MO 63130 USA
[4] Washington Univ, McDonnell Ctr Space Sci, St Louis, MO 63130 USA
关键词
Beyond Standard Model; Neutrino Physics; LEPTON NUMBER VIOLATION; HIGGS-BOSON PRODUCTION; ZEE-BABU MODEL; STANDARD MODEL; PP COLLISIONS; DECAY MODES; MAJORANA; PARITY; CONSTRAINTS; PHYSICS;
D O I
10.1007/JHEP03(2020)006
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
Models of radiative Majorana neutrino masses require new scalars and/or fermions to induce lepton-number-violating interactions. We show that these new particles also generate observable neutrino non-standard interactions (NSI) with matter. We classify radiative models as type-I or II, with type-I models containing at least one Standard Model (SM) particle inside the loop diagram generating neutrino mass, and type- II models having no SM particle inside the loop. While type-II radiative models do not generate NSI at tree-level, popular models which fall under the type-I category are shown, somewhat surprisingly, to generate observable NSI at tree-level, while being consistent with direct and indirect constraints from colliders, electroweak precision data and charged-lepton flavor violation (cLFV). We survey such models where neutrino masses arise at one, two and three loops. In the prototypical Zee model which generates neutrino masses via one-loop diagrams involving charged scalars, we find that diagonal NSI can be as large as (8%, 3.8%, 9.3%) for (epsilon(ee), epsilon(mu mu), epsilon(tau tau)), while off-diagonal NSI can be at most (10(-3)%, 0.56%, 0.34%) for (epsilon(e mu), epsilon(e tau), epsilon(mu tau)). In one-loop neutrino mass models using leptoquarks (LQs), (epsilon(mu mu), epsilon(tau tau)) can be as large as (21.6%, 51.7%), while epsilon(ee) and (epsilon(e mu), epsilon(e tau), epsilon(mu tau)) can at most be 0.6%. Other two- and three-loop LQ models are found to give NSI of similar strength. The most stringent constraints on the diagonal NSI are found to come from neutrino oscillation and scattering experiments, while the off-diagonal NSI are mostly constrained by low-energy processes, such as atomic parity violation and cLFV. We also comment on the future sensitivity of these radiative models in long-baseline neutrino experiments, such as DUNE. While our analysis is focused on radiative neutrino mass models, it essentially covers all NSI possibilities with heavy mediators.
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页数:120
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