Email this article Inelastic Neutrino Scattering on Hot Nuclei of Supernova Matter within the Theory of Finite Fermi Systems
- Authors: Tolokonnikov S.V.1,2, Saperstein E.E.1,3
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Affiliations:
- National Research Center Kurchatov Institute
- Moscow Institute of Physics and Technology (State University)
- National Research Nuclear University MEPhI
- Issue: Vol 80, No 6 (2017)
- Pages: 1157-1163
- Section: Elementary Particles and Fields Theory
- URL: https://journals.rcsi.science/1063-7788/article/view/192844
- DOI: https://doi.org/10.1134/S1063778817060217
- ID: 192844
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Abstract
The Nozières–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.
About the authors
S. V. Tolokonnikov
National Research Center Kurchatov Institute; Moscow Institute of Physics and Technology (State University)
Author for correspondence.
Email: tolkn@nrcki.ru
Russian Federation, pl. Akademika Kurchatova 1, Moscow, 128182; Institutskii per. 9, Dolgoprudnyi, Moscow oblast, 141700
E. E. Saperstein
National Research Center Kurchatov Institute; National Research Nuclear University MEPhI
Email: tolkn@nrcki.ru
Russian Federation, pl. Akademika Kurchatova 1, Moscow, 128182; Kashirskoe sh. 31, Moscow, 115409
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