Inelastic Neutrino Scattering on Hot Nuclei of Supernova Matter within the Theory of Finite Fermi Systems
| Autor: | E. E. Saperstein, S. V. Tolokonnikov |
|---|---|
| Rok vydání: | 2017 |
| Předmět: |
Physics
Nuclear and High Energy Physics Isotope Basis (linear algebra) 010308 nuclear & particles physics Astrophysics::High Energy Astrophysical Phenomena Neutron scattering 01 natural sciences Atomic and Molecular Physics and Optics Neutrino scattering Nuclear physics Supernova Cross section (physics) 0103 physical sciences Fermi liquid theory 010306 general physics Fermi Gamma-ray Space Telescope |
| Zdroj: | Physics of Atomic Nuclei. 80:1157-1163 |
| ISSN: | 1562-692X 1063-7788 |
| DOI: | 10.1134/s1063778817060217 |
| Popis: | The Nozieres–Pines method for describing neutron scattering on a heated Fermi liquid (liquid 3He) is used to calculate cross sections for inelastic neutrino scattering on the isotope 54Fe, which is an element that plays a key role in the cooling of supernovae. The calculation in question is performed on the basis of the the theory of finite Fermi systems with the aid of the DF3-a Fayans energy density functional. |
| Databáze: | OpenAIRE |
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