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Axionlike Origin of the Primordial Density Perturbation.
Physical Review Letters ( IF 8.1 ) Pub Date : 2020-07-01 , DOI: 10.1103/physrevlett.125.011302
Takeshi Kobayashi 1
Affiliation  

We show that an axionlike field coupled to a new confining gauge group can generate the primordial density perturbation in the postinflation Universe. The axion decay constant and strong coupling scale are uniquely determined by observations of the density perturbation, which further suggest a temporal deconfinement of the gauge group after inflation. The resulting temperature-dependent axion potential, together with its periodic nature, gives rise to the red-tilted density perturbation, with a positive local-type non-Gaussianity of order unity.

中文翻译:

原始密度摄动的轴状起源。

我们表明,与新的约束规子组耦合的轴状场可以在膨胀后的宇宙中产生原始密度扰动。轴突衰减常数和强耦合尺度由对密度扰动的观察唯一地确定,这进一步表明了充气后标尺组的时间限制。所产生的依赖温度的轴突电位及其周期性性质引起了红色倾斜的密度扰动,具有正阶的局部局部非高斯性。
更新日期:2020-07-01
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