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首页> 外文期刊>Advances in high energy physics >Coherent and Incoherent Neutral Current Scattering for Supernova Detection
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Coherent and Incoherent Neutral Current Scattering for Supernova Detection

机译:相干和非相干中性电流散射用于超新星检测

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The total cross sections as well as the neutrino event rates are calculated in the neutral current neutrino scattering off40Ar and132Xe isotopes at neutrino energies (Ev<100 MeV). The individual contribution coming from coherent and incoherent channels is taking into account. An enhancement of the neutral current component is achieved via the coherent (0gs+→0gs+) channel which is dominant with respect to incoherent (0gs+→Jf) one. The response of the above isotopes as a supernova neutrino detection has been considered, assuming a two parameter Fermi-Dirac distribution for the supernova neutrino energy spectra. The calculated total cross sections are tested on a gaseous spherical TPC detector dedicated for supernova neutrino detection.
机译:在中微子能量(Ev <100 MeV)下,从中性电流中微子在40Ar和132Xe同位素中的中性电流中子散射中计算出了总截面以及中微子的发生率。来自连贯和不连贯渠道的个人贡献正在考虑中。通过相干(0gs +→0gs +)通道可实现中性点电流分量的增强,该通道相对于非相干(0gs +→Jf)通道更为重要。假设超新星中微子能谱具有两个参数费米-狄拉克分布,已经考虑了上述同位素作为超新星中微子探测的响应。在专用于超新星中微子探测的气态球形TPC探测器上对计算出的总截面进行测试。

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