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Neutral-current neutrino-nucleus cross sections for A similar to 50-65 nuclei

机译:A的中性电流中微子核横截面类似于50-65核

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摘要

We study neutral-current neutrino-nucleus reaction cross sections for Mn, Fe, Co and Ni isotopes. An earlier study for a few selected nuclei has shown that in the supernova environment the cross sections are increased for low energy neutrinos due to finite-temperature effects. Our work supports this finding for a much larger set of nuclei. Furthermore we extend previous work to higher neutrino energies considering allowed and forbidden multipole contributions to the cross sections. The allowed contributions are derived from large-scale shell model calculations of the Gamow-Teller strength, while the other multipole contributions are calculated within the random phase approximation. We present the cross sections as functions of initial and final neutrino energies and for a range of supernova-relevant temperatures. These cross sections will allow improved estimates of inelastic neutrino reactions on nuclei in supenova simulations. (C) 2004-Elsevier B.V. All rights reserved.
机译:我们研究Mn,Fe,Co和Ni同位素的中性电流中微子核反应截面。先前对一些选定原子核的研究表明,在超新星环境中,由于有限的温度效应,低能中微子的横截面会增加。我们的工作支持更大范围的原子核的这一发现。此外,考虑到允许和禁止的多极截面贡献,我们将先前的工作扩展到更高的中微子能量。允许的贡献是根据Gamow-Teller强度的大型壳模型计算得出的,而其他多极贡献是在随机相位近似内计算的。我们介绍了横截面作为初始中微子能量和最终中微子能量的函数以及与超新星有关的温度范围的函数。这些横截面将允许在supenova模拟中改进对核无弹性中微子反应的估计。 (C)2004-Elsevier B.V.保留所有权利。

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