论文标题
宇宙微波背景的su（2）量规原理：宇宙学模型黑暗区域的观点
An SU(2) gauge principle for the Cosmic Microwave Background: Perspectives on the Dark Sector of the Cosmological Model
论文作者
论文摘要
我们审查了宇宙微波背景（CMB）由SU（2）而不是U（1）规格原理控制的宇宙学模型的辐射和暗部门的后果。我们还推测，由于与普朗克质量相当的Peccei-quinn量表的凝结超轻轴的肿块样构型的渗透性构型，可能会积极辅助结构形成。手性 - 反式诱导的轴突冷凝物的潜力从su（2）/su（3）Yang-mills因子因子因子因子而受到筛选（降低）限制相位的尺寸的阳性因子的贡献。
We review consequences for the radiation and dark sectors of the cosmological model arising from the postulate that the Cosmic Microwave Background (CMB) is governed by an SU(2) rather than a U(1) gauge principle. We also speculate on the possibility of actively assisted structure formation due to the de-percolation of lump-like configurations of condensed ultralight axions with a Peccei-Quinn scale comparable to the Planck mass. The chiral-anomaly induced potential of the axion condensate receives contributions from SU(2)/SU(3) Yang-Mills factors of hierarchically separated scales which act in a screened (reduced) way in confining phases.
