论文标题

暗能量和中微子超流体

Dark Energy and Neutrino Superfluids

论文作者

Addazi, Andrea, Capozziello, Salvatore, Gan, Qingyu, Marcianò, Antonino

论文摘要

我们表明,可以在一个统一的框架中解释中微子质量,暗物质和暗能量,并假设一个新的无形式内菲尔德领域,我们将其命名为“非线性深色光子”,并经历了MEV规模的动力传输,并耦合到中子中微子。深色能量的起源被动态解释为深色光子凝结的副产品,诱导裸露的无质量中微子在MEV量表周围获得有效的质量。考虑到非线性暗光子引起的通道,导致非相关性中微子配对,从而产生宇宙学超流体状态,这是令人着迷的。结果,预测光中微子复合玻色子的外观,提供了良好的冷暗物质候选者。特别是,如果我们的模型被额外的全球Lepton数字$ u_l(1)$对称性所丰富,那么中微子对可以用复合材料的Maparon领域来识别,具有对中微子 - 双贝塔 - β-赛季($0νββ$)的迷人现象学意义。我们的模型具有有趣的现象学含义,因为由于非线性出生式侵蚀术语,暗能量,暗物质和中微子质量是时间变化的动力学变量。还讨论了由Planck+SNE+BAO协作数据引起的限制。最后,我们的模型允许中微子质量的逆层次结构,对Juno实验具有有趣的影响。

We show that the neutrino mass, the dark matter and the dark energy can be explained in a unified framework, postulating a new invisible Born-Infeld field, which we name "non-linear dark photon", undergoing a meV-scale dynamical transmutation and coupled to neutrinos. Dark energy genesis is dynamically explained as a byproduct of the dark photon condensation, inducing the bare massless neutrinos to acquire an effective mass around the meV scale. It is fascinating to contemplate the channel induced by the non-linear dark photon leading to the pairing of the non-relativistic neutrinos, hence generating a cosmological superfluid state. As a consequence, the appearance of a light neutrino composite boson is predicted, providing a good cold dark matter candidate. In particular, if our model is enriched by an extra global Lepton number $U_L(1)$ symmetry, then the neutrino pair can be identified with a composite Majoron field with intriguing phenomenological implications for the neutrinoless-double-beta-decay ($0νββ$). Our model carries interesting phenomenological implications since dark energy, dark matter and the neutrino mass are time-varying dynamical variables, as a consequence of the non-linear Born-Infeld interaction terms. Limits arising from PLANCK+SNe+BAO collaborations data are also discussed. Finally, our model allows for an inverse hierarchy of neutrino masses, with interesting implications for the JUNO experiment.

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