Limits on the parameter space of (3+2) sterile neutrino scenario by IceCube data

IF 5.3 2区 物理与天体物理 Q1 ASTRONOMY & ASTROPHYSICS
Emilse Cabrera, Arman Esmaili and Alexander A. Quiroga
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引用次数: 0

Abstract

The neutrino sector of the standard model of particles can contain more than one sterile neutrino states. Generally, existence of more sterile states leads to better, or at least equally good, fit to the short baseline anomalous data due to the larger number of parameters and interferences which create features in the oscillation pattern. However, for experiments like IceCube, where the sterile states distort the oscillation pattern of high energy atmospheric neutrinos through parametric and MSW resonances, addition of more sterile states leads to a more intense effect. Although the limits on one additional sterile neutrino state by IceCube data have been studied in the literature, bounds on the models with more sterile states are lacking. We analyze the one-year data set of atmospheric neutrinos collected by IceCube during the 2011–2012 and derive the limits on the parameter space of (3+2) scenario with two sterile neutrino states, taking into account the relevant systematic and statistical uncertainties and atmospheric neutrino flux variants. To facilitate the joint analysis of IceCube and short baseline data, we provide the table of χ2 values from IceCube's data analysis as function of the parameters.
冰立方数据对(3+2)不育中微子情景参数空间的限制
粒子标准模型的中微子扇区可以包含不止一个不育中微子态。一般来说,存在更多的不育态会使短基线异常数据的拟合效果更好,或者至少是同样好,这是因为参数和干扰的数量增加了,从而在振荡模式中产生了一些特征。然而,对于像冰立方这样的实验,不育态会通过参数和 MSW 共振扭曲高能大气中微子的振荡模式,增加更多的不育态会导致更强烈的影响。尽管文献中已经研究了冰立方数据对一个额外不育中微子态的限制,但还缺乏对具有更多不育态的模型的限制。我们分析了冰立方在2011-2012年间收集的一年大气中微子数据集,并在考虑了相关的系统和统计不确定性以及大气中微子通量变体的情况下,推导出了具有两个不育中微子态的(3+2)情景参数空间的限制。为了便于联合分析冰立方和短基线数据,我们提供了冰立方数据分析中χ2值与参数的函数关系表。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Journal of Cosmology and Astroparticle Physics
Journal of Cosmology and Astroparticle Physics 地学天文-天文与天体物理
CiteScore
10.20
自引率
23.40%
发文量
632
审稿时长
1 months
期刊介绍: Journal of Cosmology and Astroparticle Physics (JCAP) encompasses theoretical, observational and experimental areas as well as computation and simulation. The journal covers the latest developments in the theory of all fundamental interactions and their cosmological implications (e.g. M-theory and cosmology, brane cosmology). JCAP''s coverage also includes topics such as formation, dynamics and clustering of galaxies, pre-galactic star formation, x-ray astronomy, radio astronomy, gravitational lensing, active galactic nuclei, intergalactic and interstellar matter.
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