Cosmological constraints on neutrino mass within consistent cosmological models

被引：3

作者：

Pang, Ye-Huang ^{[1
,2
,3
]}

Zhang, Xue ^{[4
]}

Huang, Qing-Guo ^{[1
,2
,3
]}

机构：

[1] UCAS, Hangzhou Inst Adv Study, Sch Fundamental Phys & Math Sci, Hangzhou 310024, Peoples R China

[2] Univ Chinese Acad Sci, Sch Phys Sci, Beijing 100049, Peoples R China

[3] Chinese Acad Sci, Inst Theoret Phys, CAS Key Lab Theoret Phys, Beijing 100190, Peoples R China

[4] Yangzhou Univ, Coll Phys Sci & Technol, Ctr Gravitat & Cosmol, Yangzhou 225009, Jiangsu, Peoples R China

来源：

CHINESE PHYSICS C | 2024年 / 48卷 / 06期

基金：

中国国家自然科学基金;

关键词：

neutrino mass; cosmological tension; early dark energy; EARLY DARK ENERGY; HUBBLE TENSION; HIERARCHY; SCENARIO; MATTER;

D O I：

10.1088/1674-1137/ad34c0

中图分类号：

O57 [原子核物理学、高能物理学];

学科分类号：

070202 ;

摘要：

Recently, the emergence of cosmological tension has raised doubts about the consistency of the Lambda CDM model. In order to constrain the neutrino mass within a consistent cosmological framework, we investigate three massive neutrinos with normal hierarchy (NH) and inverted hierarchy (IH) in both the axion-like EDE (Axi-EDE) model and the AdS-EDE model. We use the joint datasets including cosmic microwave background (CMB) power spectrum from Planck 2018, Pantheon of type Ia supernova, baryon acoustic oscillation (BAO) and H-0 data from SH0ES. For the nu Axi-EDE model, we obtain Sigma mv,NH < 0.152 eV and Sigma mv,IH < 0.178 eV, while for the nu AdS-EDE model, we find Sigma mv,NH < 0.135 eV and Sigma mv,IH < 0.167 eV. Our results exhibit a preference for the normal hierarchy in both the nu Axi-EDE model and the nu AdS-EDE model.

引用

页数：7

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