4.8 Article

STEREO neutrino spectrum of 235U fission rejects sterile neutrino hypothesis

期刊

NATURE
卷 613, 期 7943, 页码 257-+

出版社

NATURE PORTFOLIO
DOI: 10.1038/s41586-022-05568-2

关键词

-

向作者/读者索取更多资源

Anomalies in past neutrino measurements have led to the discovery of non-zero neutrino mass and oscillation between different flavors. The STEREO experiment aimed to investigate the existence of a supplementary, sterile neutrino state that does not interact via weak interaction. The analysis of data from the STEREO experiment confirms observed anomalies while rejecting the hypothesis of a light sterile neutrino.
Anomalies in past neutrino measurements have led to the discovery that these particles have non-zero mass and oscillate between their three flavours when they propagate. In the 2010s, similar anomalies observed in the antineutrino spectra emitted by nuclear reactors have triggered the hypothesis of the existence of a supplementary neutrino state that would be sterile, that is, not interacting by means of the weak interaction(1). The STEREO experiment(2-6) was designed to investigate this conjecture, which would potentially extend the standard model of particle physics. Here we present an analysis of the full set of data generated by STEREO, confirming observed anomalies while rejecting the hypothesis of a light sterile neutrino. Installed at the Institut Laue-Langevin (ILL) research reactor, STEREO accurately measures the antineutrino energy spectrum associated to the fission of U-235. The segmentation of the detector and its very short distance to the compact core are crucial properties of STEREO for our analysis. The measured antineutrino energy spectrum suggests that anomalies originate from biases in the nuclear experimental data used for the predictions(7,8). Our result supports the neutrino content of the standard model and establishes a new reference for the U-235 antineutrino energy spectrum. We anticipate that this result will allow progress towards finer tests of the fundamental properties of neutrinos but also to benchmark models and nuclear data of interest for reactor physics(9,10) and for observations of astrophysical or geoneutrinos(11,12).

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

4.8
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