论文标题

$θ_{13} $和暗物质中的常见起源在味道对称Scoto-Seesaw框架中

Common origin of $θ_{13}$ and dark matter within the flavor symmetric scoto-seesaw framework

论文作者

Ganguly, Joy, Gluza, Janusz, Karmakar, Biswajit

论文摘要

为了理解中微子质量和混合的观察到的模式,以及考虑到深色物质,我们提出了基于$ a_4 $ a_4 $离散风味对称性的混合型Scoto-Seesaw模型。在此设置中,包括至少两个重型右中微子,对于使用离散的风味对称性至关重要,这些风味对称性曾经模仿曾经流行的Trimimaximal中微子在领先的序列中通过I型Seesaw在领先顺序上混合。然后,Scotogenic的贡献是重现反应器混合角$θ_{13} $(在三层混合方案中)的关键偏差,并适应潜在的暗物质候选物,指向$θ_{13} $的常见起源。该模型预测大气角处于上部八分之一,排除了狄拉克CP阶段的某些区域,并限制了主要阶段。此外,可以针对与复杂的光中微子质量基质相关的相对相的特定值区分正常和倒置的质量层次结构。由于被认为的风味对称性,源自苏格氏剂机制侵犯了违反的衰减,例如$ \ rightarroweγ$,$τ\ rightarroweγ$消失,以及第二右手中微子质量的下限。中性元双β衰减中出现的有效质量参数的预测属于未来实验的灵敏度,例如Legend-1k和Nexo。

To understand the observed pattern of neutrino masses and mixing as well as to account for the dark matter we propose a hybrid scoto-seesaw model based on the $A_4$ discrete flavor symmetry. In this setup, including at least two heavy right-handed neutrinos is essential to employ the discrete flavor symmetry that mimics once popular tribimaximal neutrino mixing at the leading order via type-I seesaw. The scotogenic contribution then acts as a critical deviation to reproduce the observed value of the reactor mixing angle $θ_{13}$ (within the trimaximal mixing scheme) and to accommodate potential dark matter candidates, pointing towards a common origin of $θ_{13}$ and dark matter. The model predicts the atmospheric angle to be in the upper octant, excludes some regions on the Dirac CP phase, and restricts the Majorana phases too. Further, normal and inverted mass hierarchies can be distinguished for specific values of the relative phases associated with the complex light neutrino mass matrix. Owing to the considered flavor symmetry, contributions coming from the scotogenic mechanism towards the lepton flavor violating decays such as $μ\rightarrow e γ$, $τ\rightarrow e γ$ vanish, and a lower limit on the second right-handed neutrino mass can be obtained. Prediction for the effective mass parameter appearing in the neutrinoless double beta decay falls within the sensitivity of future experiments such as LEGEND-1k and nEXO.

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