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首页> 外文期刊>Progress in Particle and Nuclear Physics >Studying low-energy astrophysical neutrinos with neutrino nucleus cross-section calculations and beta beam neutrino spectra
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Studying low-energy astrophysical neutrinos with neutrino nucleus cross-section calculations and beta beam neutrino spectra

机译:利用中微子核截面计算和β射线中微子谱研究低能天体中微子

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摘要

We first calculate total neutrino-nucleus cross-sections for the reactions ~(66)Zn(~(ν?,ν?′))66Zn ~* and ~(130)Te(~(ν?,ν?′)) ~(130)Te* within the context of the quasiparticle random phase approximation. The isotopes ~(66)Zn and ~(130)Te are contents of the COBRA double beta decay detector at Gran Sasso. We then use synthetic low-energy beta-beam antineutrino spectra, originating from boosted β- radioactive 6He ions for the interpretation of various SN-neutrino signals.
机译:我们首先计算〜(66)Zn(〜(ν?,ν?'))66Zn〜*和〜(130)Te(〜(ν?,ν?'))〜的反应的总中微子核截面(130)Te *在准粒子随机相位近似的范围内。同位素〜(66)Zn和〜(130)Te是Gran Sasso处COBRA双β衰变探测器的含量。然后,我们使用合成的低能量β束抗中微子光谱(源自增强的β放射性6He离子)来解释各种SN中微子信号。

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