标题： III型生热模型：暴胀、暗物质与对撞机现象学 显示英文标题

标题： Type-III Scotogenic Model: Inflation, Dark Matter and Collider Phenomenology

摘要： 我们研究了类型-III scotogenic 模型的一个扩展，通过引入一个实单态标量。 该标量由于与里奇标量的非最小耦合而作为暴胀子起着关键作用。 随后，暴胀子场衰变为类型-III scotogenic 框架内的其他粒子。 在此框架中，惰性标量双态和费米子三重态对于中微子质量生成至关重要，并且是宇宙中25%能量预算或暗物质的强候选者。 我们研究了它们的残留丰度和直接探测的潜力。 此外，我们讨论了未来对撞机实验中可能被识别的观测信号。 显示英文摘要

摘要： We investigate an extension of the Type-III scotogenic model by incorporating a real singlet scalar. This scalar plays a crucial role as the inflaton due to its non-minimal coupling with the Ricci scalar. The inflaton field subsequently decays into other particles within the Type-III scotogenic framework. In this framework, the inert scalar doublet and fermion triplet are crucial for neutrino mass generation and present strong candidates for 25\% energy budget or dark matter in the Universe. We study their relic abundance and potential for direct detection. Furthermore, we discuss possible observational signals that could be identified in future collider experiments.