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Axino dark matter and baryon number asymmetry from Q-ball decay in gauge mediation

机译:axino暗物质和重子数不对称来自Q球衰减   调解

摘要

We investigate the Q-ball decay into the axino dark matter in thegauge-mediated supersymmetry breaking. In our scenario, the Q ball decaysmainly into nucleons and partially into axinos to account for the baryonasymmetry and the dark matter of the universe simultaneously. The Q ball decayswell before the big bang nucleosynthesis so that it is not affected by thedecay. The decay into the supersymmetric particles of the minimalsupersymmetric standard model is kinematically prohibited until the very end ofthe decay, and we could safely make their abundances small enough for thesuccessful big bang nucleosynthesis. We show the regions of axino modelparameters and the Q-ball parameters which realize this scenario.
机译:我们在量规介导的超对称破坏中研究了Q球向轴突暗物质的衰变。在我们的场景中,Q球主要衰变为核子,部分衰变为轴突,同时解释了宇宙的重子不对称和暗物质。 Q球在大爆炸核合成之前衰变,因此不受衰变影响。运动学上禁止在最小超对称标准模型中衰减到超对称粒子,直到衰减结束为止,我们可以安全地使其丰度小到足以成功进行大爆炸核合成。我们显示了实现此方案的轴心模型参数区域和Q球参数。

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