4.7 Article

Primordial lepton asymmetries in the precision cosmology era: Current status and future sensitivities from BBN and the CMB

期刊

PHYSICAL REVIEW D
卷 107, 期 3, 页码 -

出版社

AMER PHYSICAL SOC
DOI: 10.1103/PhysRevD.107.035024

关键词

-

向作者/读者索取更多资源

The EMPRESS survey, using a new sample of extremely metal poor systems, has reported a primordial helium abundance that is 3s smaller than the prediction from standard big bang nucleosynthesis. This could indicate a primordial lepton asymmetry in the electron neutrino flavor. A comprehensive analysis of the lepton asymmetry is presented, using measurements of primordial element abundances and cosmic microwave background (CMB) data from Planck. The results suggest a non-zero lepton asymmetry with a deviation from zero of 2.9s, assuming no dark radiation, or 2.2s if the abundance of dark radiation is not assumed.
Using a new sample of extremely metal poor systems, the EMPRESS survey has recently reported a primordial helium abundance that is 3s smaller than the prediction from the standard big bang nucleosynthesis (BBN) scenario. This measurement could be interpreted as a hint for a primordial lepton asymmetry in the electron neutrino flavor. Motivated by the EMPRESS results, we present a comprehensive analysis of the lepton asymmetry using measurements of the abundances of primordial elements, along with cosmic microwave background (CMB) data from Planck. Assuming that there is no dark radiation in our Universe, we find an electron neutrino chemical potential ?(?e) = 0.043 +/- 0.015, which deviates from zero by 2.9s. If no assumption is made on the abundance of dark radiation in the Universe, the chemical potential is ?(?e) = 0.046 +/- 0.021, which deviates from zero by 2.2s. We also find that this result is rather insensitive to the choice of nuclear reaction rates. If the true helium abundance corresponds to the EMPRESS central value, future CMB observations from the Simons Observatory and CMB-S4 will increase the significance for a nonzero lepton asymmetry to 4s and 5s respectively, assuming no dark radiation, or to 3s when no assumption is made on the abundance of dark radiation.

作者

我是这篇论文的作者
点击您的名字以认领此论文并将其添加到您的个人资料中。

评论

主要评分

4.7
评分不足

次要评分

新颖性
-
重要性
-
科学严谨性
-
评价这篇论文

推荐

暂无数据
暂无数据