Particle-Induced Electromagnetic De-Excitation of Nuclei in Stellar Matter

Details Particle-Induced Electromagnetic De-Excitation of Nuclei in Stellar Matter Particle-Induced Electromagnetic De-Excitation of Nuclei in Stellar Matter

Aug 1967

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1967phrv..160.1193s&link_type=abstract

Physical Review, vol. 160, Issue 5, pp. 1193-1202

Astronomy and Astrophysics

Astrophysics

13

Scientific paper

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

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