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arXiv 2307.04662hep-phhep-ex
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镜像双希格斯模型中的重子生成与暗物质

Baryogenesis and Dark Matter in the Mirror Twin Higgs

Pedro Bittar, Gustavo Burdman, Larissa Kiriliuk

AI总结:

本研究在镜像双希格斯框架下构建自然非对称暗物质模型,无需硬破缺$\n\b_2$对称性即可通过双重子暗物质得到符合观测的丰度,给出约1GeV的暗物质质量及直接探测率估算。

摘要:

我们研究了镜像双希格斯(Mirror Twin Higgs,MTH)框架下一种自然的非对称暗物质(asymmetric dark matter,ADM)模型。研究表明,当双重子作为暗物质(DM)候选者时,无需在无量纲耦合中显式破坏MTH的$\n\b_2$对称性(即无硬$\n\b_2$破缺),即可得到符合观测的暗物质丰度。我们通过一个同时产生非对称暗物质的特定重子生成机制,阐释了该过程的实现原理。在最简方案中,我们得到暗物质质量$m_{\rm DM}\sim O(1)$GeV,略高于质子质量。本文还给出了当前及未来实验的直接探测率估算结果。

英文摘要:

We consider a natural asymmetric dark matter (ADM) model in the mirror twin Higgs (MTH). We show that it is possible to obtain the correct dark matter (DM) abundance when a twin baryon is the DM without the need of explicit breaking of the MTH $\mathbb{Z}_2$ symmetry in the dimensionless couplings (i.e. without hard $\mathbb{Z}_2$ breaking). We illustrate how this is possible in a specific baryogenesis setup, which also leads to ADM. In the simplest scenario we obtain $m_{\rm DM}\sim O(1)$GeV, just above the proton mass. We show estimates for direct detection rates at present and future experiments.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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