On the nuclear response of 56Fe to supernova neutrino spectra

被引：0

作者：

Tsakstara, V. A. ^{[1
]}

Kosmas, T. S. ^{[1
]}

Chasioti, V. C. ^{[1
]}

Sinatkas, J. ^{[2
]}

机构：

[1] Univ Ioannina, Sect Theoret Phys, GR-45110 Ioannina, Greece

[2] TEI Western Macedonia, Dept Informat & Comp Technol, Kastoria 52100, Greece

来源：

EXOTIC NUCLEI AND NUCLEAR /PARTICLE ASTROPHYSICS (II) | 2008年 / 972卷

关键词：

supernova neutrinos; Neutrino-nucleus interactions; neutrino detection; nuclear response to neutrino spectra; convolution method;

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Neutral current cross sections of scattering of v. on the nuclear isotope Fe-56, which play a significant role in astrophysical neutrino studies, are used in order to explore the response of this detector to supernova. neutrino spectra. We assume a two-parameter Fermi-Dirac distribution for the supernova neutrino spectra and evaluate the flux averaged cross sections for various values of the neutrino temperature and chemical potential parameters.

引用

页码：562 / +

页数：2

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