arXivDaily arXiv每日学术速递 周一至周五更新
arXiv 1907.11228hep-phastro-ph.COhep-th
收藏

从自对偶规范/希格斯动力学研究暗物质

Dark Matter from self-dual gauge/Higgs dynamics

Dario Buttazzo, Luca Di Luzio, Giacomo Landini, Alessandro Strumia, Daniele Teresi

摘要:

我们表明,一个新的规范群与一个新的标量导致自动稳定的暗物质候选人。我们考虑希格斯相与受限相对偶的理论:已知SU(2)规范理论与标量偶态(如标准模型)服从这一非平凡特征。我们给出了一个一般的判据,证明了这种自对偶性对SU(N),SO(N),Sp(N)和G_2规范动力学在基本表象中具有标量场时都成立。由此产生的暗物质现象学具有非平凡的特征,这些特征是该组的特征,我们将逐一讨论。仅举几例,SU(N)有一个偶然守恒的暗重子数,SO(2N+1)由于特殊的宇称导致稳定的胶球,G_2导致类似于中性K介子的暗物质系统。宇宙学上的暗物质丰度通常在100 TeV左右的质量下重现:所有的约束都得到满足,较轻的暗胶球可以影响希格斯物理。这些理论获得了额外的兴趣和预测性,假设暗和弱尺度都是动态生成的。

英文摘要:

We show that a new gauge group with one new scalar leads to automatically stable Dark Matter candidates. We consider theories where the Higgs phase is dual to the confined phase: it is known that SU(2) gauge theories with a scalar doublet (like the Standard Model) obey this non-trivial feature. We provide a general criterion, showing that this self-duality holds for SU(N), SO(N), Sp(N) and G_2 gauge dynamics with a scalar field in the fundamental representation. The resulting Dark Matter phenomenology has non-trivial features that are characteristic of the group, and that we discuss case by case. Just to mention a few, SU(N) has an accidental conserved dark baryon number, SO(2N+1) leads to stable glue-balls thanks to a special parity, G_2 leads to a Dark Matter system analogous to neutral kaons. The cosmological Dark Matter abundance is often reproduced for masses around 100 TeV: all constraints are satisfied and lighter dark glue-balls can affect Higgs physics. These theories acquire additional interest and predictivity assuming that both the dark and weak scales are dynamically generated.

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。

↑