Cosmological constraints on neutrino mass within consistent cosmological models* * We acknowledge the use of HPC Cluster of ITP-CAS. XZ is supported by the National Natural Science Foundation of China (12005183). QGH is supported by the National Natural Science Foundation of China (12250010, 11975019, 11991052, 12047503), and the Key Research Program of Frontier Sciences, CAS, (ZDBS-LY-7009)

IF 3.6 2区物理与天体物理 Q1 PHYSICS, NUCLEAR

中国物理C Pub Date : 2024-06-01 DOI:10.1088/1674-1137/ad34c0

Ye-Huang Pang, Xue Zhang, Qing-Guo Huang

{"title":"Cosmological constraints on neutrino mass within consistent cosmological models* * We acknowledge the use of HPC Cluster of ITP-CAS. XZ is supported by the National Natural Science Foundation of China (12005183). QGH is supported by the National Natural Science Foundation of China (12250010, 11975019, 11991052, 12047503), and the Key Research Program of Frontier Sciences, CAS, (ZDBS-LY-7009)","authors":"Ye-Huang Pang, Xue Zhang, Qing-Guo Huang","doi":"10.1088/1674-1137/ad34c0","DOIUrl":null,"url":null,"abstract":"Recently, the emergence of cosmological tension has raised doubts about the consistency of the ΛCDM model. 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 early dark energy (Axi-EDE) and AdS-EDE models. We use joint datasets including the cosmic microwave background power spectrum from <italic toggle=\"yes\">Planck</italic> 2018, Pantheon of type Ia supernova, baryon acoustic oscillation, and <inline-formula>\n<tex-math><?CDATA $ H_0 $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_6_065102_M1.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> data from SH0ES. For the <italic toggle=\"yes\">ν</italic>Axi-EDE model, we obtain <inline-formula>\n<tex-math><?CDATA $\\sum m_{\\nu,\\mathrm{NH}}$?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_6_065102_M2.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> < 0.152 eV and <inline-formula>\n<tex-math><?CDATA $\\sum m_{\\nu,\\mathrm{IH}}$?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_6_065102_M3.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> < 0.178 eV, whereas for the <italic toggle=\"yes\">ν</italic>AdS-EDE model, we find <inline-formula>\n<tex-math><?CDATA $\\sum m_{\\nu,\\mathrm{NH}}$?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_6_065102_M4.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> < 0.135 eV and <inline-formula>\n<tex-math><?CDATA $\\sum m_{\\nu,\\mathrm{IH}} $?></tex-math>\n<inline-graphic xlink:href=\"cpc_48_6_065102_M5.jpg\" xlink:type=\"simple\"></inline-graphic>\n</inline-formula> < 0.167 eV. Our results exhibit a preference for NH in both the <italic toggle=\"yes\">ν</italic>Axi-EDE and <italic toggle=\"yes\">ν</italic>AdS-EDE models.","PeriodicalId":10250,"journal":{"name":"中国物理C","volume":"45 1","pages":""},"PeriodicalIF":3.6000,"publicationDate":"2024-06-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"中国物理C","FirstCategoryId":"101","ListUrlMain":"https://doi.org/10.1088/1674-1137/ad34c0","RegionNum":2,"RegionCategory":"物理与天体物理","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q1","JCRName":"PHYSICS, NUCLEAR","Score":null,"Total":0}

引用次数: 0

Abstract

Recently, the emergence of cosmological tension has raised doubts about the consistency of the ΛCDM model. 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 early dark energy (Axi-EDE) and AdS-EDE models. We use joint datasets including the cosmic microwave background power spectrum from Planck 2018, Pantheon of type Ia supernova, baryon acoustic oscillation, and

data from SH0ES. For the νAxi-EDE model, we obtain

< 0.152 eV and

< 0.178 eV, whereas for the νAdS-EDE model, we find

< 0.135 eV and

< 0.167 eV. Our results exhibit a preference for NH in both the νAxi-EDE and νAdS-EDE models.

查看原文本刊更多论文

一致宇宙学模型中对中微子质量的宇宙学约束* * 感谢使用ITP-CAS的高性能计算集群。XZ受国家自然科学基金资助（12005183）。QGH 得到国家自然科学基金（12250010, 11975019, 11991052, 12047503）和中科院前沿科学重点研究计划（ZDBS-LY-7009）的资助。

最近，宇宙学张力的出现使人们对ΛCDM模型的一致性产生了怀疑。为了在一致的宇宙学框架内约束中微子质量，我们研究了类轴子早期暗能量（Axi-EDE）和AdS-EDE模型中具有正常层次（NH）和倒层次（IH）的三种大质量中微子。我们使用了联合数据集，包括来自普朗克 2018 的宇宙微波背景功率谱、Ia 型超新星 Pantheon、重子声学振荡和来自 SH0ES 的数据。对于νAxi-EDE模型，我们得到了< 0.152 eV和< 0.178 eV，而对于νAdS-EDE模型，我们发现了< 0.135 eV和< 0.167 eV。我们的结果表明，νAxi-EDE 和 νAdS-EDE 模型都更倾向于 NH。

本文章由计算机程序翻译，如有差异，请以英文原文为准。

求助全文

约1分钟内获得全文求助全文

来源期刊

中国物理C 物理-物理：核物理

CiteScore

6.50

自引率

8.30%

发文量

8976

审稿时长

1.3 months

期刊介绍： Chinese Physics C covers the latest developments and achievements in the theory, experiment and applications of: Particle physics; Nuclear physics; Particle and nuclear astrophysics; Cosmology; Accelerator physics. The journal publishes original research papers, letters and reviews. The Letters section covers short reports on the latest important scientific results, published as quickly as possible. Such breakthrough research articles are a high priority for publication. The Editorial Board is composed of about fifty distinguished physicists, who are responsible for the review of submitted papers and who ensure the scientific quality of the journal. The journal has been awarded the Chinese Academy of Sciences ‘Excellent Journal’ award multiple times, and is recognized as one of China''s top one hundred key scientific periodicals by the General Administration of News and Publications.