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Cosmic-ray signatures of dark matter from a flavor dependent gauge symmetry model with neutrino mass mechanism

机译:用中微子质量机制来自风味依赖性仪表对称模型的暗物质思路

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We propose an extension to the Standard Model accommodating two families of Dirac neutral fermions and Majorana fermions under additional U ( 1 ) e ? μ × Z 3 × Z 2 symmetries where U ( 1 ) e ? μ is a flavor dependent gauge symmetry related to the first and second family of the lepton sector, which features a two-loop induced neutrino mass model. The two families are favored by minimally reproducing the current neutrino oscillation data and two mass difference squares and canceling the gauge anomalies at the same time. As a result, we have a prediction for neutrino masses. The lightest Dirac neutral fermion is a dark matter candidate with tree-level interaction restricted to electron, muon and neutrinos, which makes it difficult to detect in direct dark matter search as well as indirect search focusing on the τ -channel, such as through γ -rays. It may however be probed by search for dark matter signatures in electron and positron cosmic rays, and allows interpretation of a structure appearing in the CALET electron + positron spectrum around 350–400?GeV as its signature, with a boost factor ~ 40 Breit-Wigner enhancement of the annihilation cross section.
机译:我们提出了在额外的U(1)e(1)e下的标准模型的标准模型,可容纳两个Dirac中性码头和Majorana Fermions的家庭? μ×z 3×z 2对称,U(1)E? μ是与Lepton扇区的第一和第二家族有关的风味依赖性仪表对称,其具有双环诱导的中微子质量模型。通过最小地再现目前的中微子振荡数据和两个质量差分并同时取消仪表异常来青睐这两个家庭。结果,我们对中菌群众进行了预测。最轻的DIRAC中性度码头是一个暗物质候选的候选候选者,其被限制为电子,μ子和中微子,这使得难以在直接的暗物质搜索中检测到直接的暗物质搜索以及专注于τ-Channel的间接搜索,例如通过γ - 是。然而,可以通过搜索电子和正电子宇宙射线中的暗质质签名来探测,并且允许解释在C +正电子频谱中出现的结构+正电子频率约为350-400?GEV作为其签名,具有升压因子〜40 breit-湮灭横截面的Wigner增强。

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