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
Recommended Citation
Please use publisher's recommended citation.
COinS
Comments
Published version found here: www.aps.org