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A family of WISPy dark matter candidates

机译:WISPy暗物质候选人家庭

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Dark matter made from non-thermally produced bosons can have very low, possibly sub-eV masses. Axions and hidden photons are prominent examples of such “dark” very weakly interacting light (slim) particles (WISPs). A suitable mechanism for their non-thermal production is the misalignment mechanism. Their dominant interaction with Standard Model (SM) particles is via photons. In this note we want to go beyond these standard examples and discuss a wide range of scalar and pseudo-scalar bosons interacting with SM matter fermions via derivative interactions. Suitably light candidates arise naturally as pseudo-Nambu–Goldstone bosons. In particular we are interested in examples, inspired by familons, whose interactions have a non-trivial flavor structure.
机译:由非热产生的玻色子制成的暗物质可能具有非常低的质量,可能低于eV。轴和隐藏的光子是这种“暗”相互作用非常弱的轻(细)粒子(WISP)的突出示例。非热产生的合适机制是未对准机制。它们与标准模型(SM)粒子的主要相互作用是通过光子。在本说明中,我们希望超越这些标准示例,并讨论通过导数相互作用与SM物质费米相互作用的大量标量和拟标量玻色子。适当地,轻质的候选物自然会以假纳姆布-戈德斯通玻色子出现。特别是,我们对受家族影响的示例感兴趣,这些示例的相互作用具有不平凡的风味结构。

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