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Astrophysical signatures of asymmetric dark matter bound states

机译:不对称暗物质束缚态的天体物理特征

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Nuggets—very large stable bound objects arising in the presence of a sufficiently attractive and long-range force and in the absence of a dark Coulomb force—are a smoking gun signature for asymmetric dark matter (ADM). The cosmology of ADM nuggets is both generic and unique: nuggets feature highly exothermic fusion processes, which can impact the shape of the core in galaxies, as well as give rise to rare dark star formation. We find, considering the properties of nuggets in a generic extended nuclear model with both attractive and repulsive forces, that self-interaction constraints place an upper bound on nugget masses at the freeze-out of synthesis in the ballpark of M fo ? 10 16 ? ? GeV . We also show that indirect detection strongly constrains models where the scalar mediator binding the nuggets mixes with the Higgs.
机译:核金块-在没有足够的吸引力和远距离力且没有暗库仑力的情况下产生的非常大的稳定结合物-是不对称暗物质(ADM)的吸烟枪特征。 ADM核的宇宙学既有通用性又有独特性:核具有高度放热的融合过程,这会影响星系核心的形状,并导致罕见的暗星形成。我们发现,考虑到在具有吸引力和排斥力的通用扩展核模型中,核的性质,自相互作用的约束在M fo球场的合成冻结中给核块质量设置了上限。 10 16? ? GeV。我们还表明,间接检测强烈地约束了绑定掘金的标量介体与希格斯混合的模型。

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