Document Type

Article

Publication Date

8-25-1967

Publication Title

The Physical Review

Publisher

The American Physical Society

Abstract

The rate for electromagnetic de-excitation of excited nuclei by inelastic scattering with electrons and ions in stellar matter is calculated as a function of temperature, density, transition energy, and multipole type. The results of this paper indicate that for temperatures in the range 109°K

Comments

Published version found here: www.aps.org

Download

Share

COinS