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首页> 外文期刊>European physical journal >Connecting light dirac neutrinos to a multi-component dark matter scenario in gauged (B-L) model
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Connecting light dirac neutrinos to a multi-component dark matter scenario in gauged (B-L) model

机译:将灯光中微子连接到仪表(B-L )模型中的多组分暗物地方案

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We propose a new gauged $$B-L$$ B-L extension of the standard model where light neutrinos are of Dirac type, naturally acquiring sub-eV mass after electroweak symmetry breaking, without any additional global symmetries. This is realised by choosing a different $$B-L$$ B-L charge for right handed neutrinos than the usual $$-1$$ -1 so that the Dirac Yukawa coupling involves an additional neutrinophilic scalar doublet instead of the usual Higgs doublet. The model can be made anomaly free by considering four additional chiral fermions which give rise to two massive Dirac fermions by appropriate choice of singlet scalars. The choice of scalars not only helps in achieving the desired particle mass spectra via spontaneous symmetry breaking, but also leaves a remnant $$Z_2 imes Z'_2$$ Z2×Z2′ symmetry to stabilise the two dark matter candidates. Apart from this interesting link between Dirac nature of light neutrinos and multi-component dark matter sector, we also find that the dark matter parameter space is constrained mostly by the cosmological upper limit on effective relativistic degrees of freedom $$Delta N_{mathrm{eff}}$$ ΔNeff which gets enhanced in this model due to the thermalisation of the light right handed neutrinos by virtue of their sizeable $$B-L$$ B-L gauge interactions.
机译:我们提出了一种新的衡量标准型号的标准型号的标准型号,其中浅中微子是DIRAC型,自然获取电牛约对称后的副EV质量,没有任何额外的全局对称。这是通过选择不同的$$ B-L N $$ B-L比通常的$$ - 1 $$ -1 -1来实现这一目标,使Dirac Yukawa联轴器涉及另外的中非中性级标量级,而不是通常的Higgs Doublet。 The model can be made anomaly free by considering four additional chiral fermions which give rise to two massive Dirac fermions by appropriate choice of singlet scalars.标量的选择不仅有助于通过自发对称性破碎实现所需的粒子质谱,而且还留下了一个残余的$$ Z_2 timesZ'_2 $$ Z2×Z2的对称性以稳定两个暗物质候选者。除了光中微子和多组分暗物片部门的Dirac性质之间的这种有趣联系之外,我们还发现暗物质参数空间主要受到有效相对论自由度的宇宙学上限$$ delta n _ { mathrm的限制{Eff}} $$Δneff由于借助于光右手NeverInos的热化,在该模型中得到增强,因为它借助于其相当的$$ BL $$ BL仪表互动。

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