WIMP-like Dark Matter Without Thermalization At Freeze-Out
类WIMP暗物质无需冻结时热化
Dan Hooper, Gordan Krnjaic, Gabriele Montefalcone
AI总结 该研究探讨了在冻结时无需热化的隐藏扇区模型中,如何通过极小的耦合实现与观测相符的暗物质 relic 密度,从而推翻传统热 relic 情况下的交叉截面假设。
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- 16 pages, 4 figures
在标准热 relic 情景中,暗物质在冻结时 $T \sim m_X/20$ 之前与标准模型辐射浴保持化学平衡,其中 $m_X$ 是暗物质质量。在这一常见模型中,观测到的 relic 密度由约 $σv \sim 10^{-26}$ cm$^3$/s 的湮灭截面获得。我们展示,类似截面可以在隐藏扇区模型中自然实现,其中暗物质和标准模型部分在非常高的温度 $T \gg m_X$ 时解耦,随后各自发展出独立的热历史。尽管解耦,冻结时两个部分的温度相似,导致通常的热 relic 密度。因此,标准模型与隐藏部分之间的耦合可以极小,可能使直接探测和对撞机信号远低于可预见的灵敏度。
In the standard thermal relic scenario, dark matter remains in chemical equilibrium with the Standard Model radiation bath until freeze-out occurs at $T \sim m_X/20$, where $m_X$ is the dark matter mass. In this familiar class of models, the observed relic density is obtained for annihilation cross sections of order $σv \sim 10^{-26}$ cm$^3$/s. We show that comparable cross sections can naturally be realized in hidden-sector models in which the dark matter and Standard Model sectors decouple at a very high temperature, $T \gg m_X$, and subsequently evolve with separate thermal histories. Despite this decoupling, the two sectors have similar temperatures during freeze-out, leading to the usual thermal relic abundance. As a consequence, the coupling between the Standard Model and hidden sectors can be extremely small, potentially placing direct detection and collider signals far below foreseeable sensitivities.