论文标题
中间烟木和避免脱糊化
Mesotuned WIMPs and Avoided Deconfinement
论文作者
论文摘要
我们讨论了订单$ 10 $ - $ 100 $ tev和$ \ Mathcal {o}（1）$耦合到标准模型的订单的生产，我们称之为“ Mesotuned Wimp”。鉴于在LHC上没有观察到的新物理学，这表明我们生活在一个具有一定程度的微调的世界中，因此这种量表是一种自然的规模，可以期望新粒子出现。然而，在此范围内具有质量的暗物质，并且很难通过通常的机制，而观察到的遗物丰度很难产生大型耦合。在这里，我们讨论了暗物质的非热生产，并表明该机制可以在该质量范围内产生观察到的暗物质，但需要暗物质质量与重新温度之间的特定关系。结果表明，避免的解料模型消除了对再加热温度的依赖性，并预测了可以在Cherenkov望远镜阵列和直接检测实验中测试的暗物质候选者，并为中间带有w imp暗物质的自然设置提供了自然设置。
We discuss the production of dark matter with mass of order $10$-$100$ TeV and $\mathcal{O}(1)$ couplings to the standard model, a scenario we refer to as the `mesotuned WIMP'. Given the lack of new physics observed at the LHC, indicating we live in a world with some degree of fine-tuning, this scale is a natural scale to expect new particles to appear. However, dark matter with mass in this range and large couplings is difficult to produce with the observed relic abundance via the usual mechanisms. Here we discuss the nonthermal production of dark matter and show that this mechanism can produce the observed dark matter in this mass range, but requires a specific relationship between the dark matter mass and the reheat temperature. It is shown that the avoided deconfinement model removes the dependence on the reheat temperature and predicts a dark matter candidate that can be tested at the Cherenkov Telescope Array and direct detection experiments, offering a natural setting for mesotuned WIMP dark matter.
