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Neutrino-Mass Effects on the CMB Anisotropies in a Cosmological Model with a Primordial Magnetic Field

科研成果: 书/报告/会议事项章节会议稿件同行评审

摘要

In recent years neutrino oscillation experiments have showed that neutrinos have finite mass. One can determine the neutrino mass from neutrinoless double-beta decay experiments, but the exact mass of neutrinos is still unknown. However, we can also constrain the neutrino mass from a precise analysis of the CMB data, which constrains the mass to be smaller than 2 eV (2σ) in a standard ΛCDM model [1]. In recent studies it has beddn shown that a primordial magnetic field (PMF) exists, and it makes important effects on the CMB anisotropies. In this work, we constrain the total neutrino mass from the CMB anisotropies with the PMF effect. We thus a obtained a smaller upper limit on the neutrino mass, i.e. <1.3 eV(2σ). We will also discuss the dependence on the power law spectral index of the PMF and on the vector CMB anisotropies.

源语言英语
主期刊名Origin of Matter and Evolution of Galaxies - 10th International Symposium on Origin of Matter and Evolution of Galaxies
主期刊副标题From the Dawn of Universe to the Formation of Solar System, OMEG 2007
编辑Toshitaka Kajino, Takuma Suda, Takaya Nozawa, Akira Ohnishi, Masayuki Y. Fujimoto, Shigeru Kubono, Kiyoshi Kato
出版商American Institute of Physics Inc.
454-456
页数3
ISBN(电子版)9780735405370
DOI
出版状态已出版 - 2008
已对外发布
活动10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, OMEG 2007 - Sapporo, 日本
期限: 4 12月 20077 12月 2007

出版系列

姓名AIP Conference Proceedings
1016
ISSN(印刷版)0094-243X
ISSN(电子版)1551-7616

会议

会议10th International Symposium on Origin of Matter and Evolution of Galaxies: From the Dawn of Universe to the Formation of Solar System, OMEG 2007
国家/地区日本
Sapporo
时期4/12/077/12/07

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