γ-ray strength function for astrophysical applications in the IAEA-CRP

γ-ray strength function for astrophysical applications in the IAEA-CRP

The γ-ray strength function (γSF) is a nuclear quantity that governs photoabsorption in (γ, n) and photoemission in (n, γ) reactions. Within the framework of the γ-ray strength function method, we use (γ, n) cross sections as experimental constraints on the γSF from the Hartree-Fock-Bogolyubov plus...

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Bibliographic Details
Main Authors: Utsunomiya Hiroaki, Goriely Stephane, Renstrøm Therese, Tveten Gry M., Ari-izumi Takashi, Miyamoto Shuji, Lui Yiu-Wing, Larsen Ann-Cecilie, Siem Sunniva, Hilaire Stephane, Péru Sophie, Koning Arjan J.
Format: Article
Language:English
Published: EDP Sciences 2020-01-01
Series:EPJ Web of Conferences
Online Access:https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_07005.pdf

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https://www.epj-conferences.org/articles/epjconf/pdf/2020/15/epjconf_nd2019_07005.pdf

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