ABUNDANCE ANOMALIES PRODUCED BY NUCLEAR REACTIONS IN STELLAR SURFACE LAYERS: I. NUCLEAR-REACTION RATES
- 1 October 1967
- journal article
- Published by Canadian Science Publishing in Canadian Journal of Physics
- Vol. 45 (10) , 3275-3296
- https://doi.org/10.1139/p67-275
Abstract
A preliminary investigation of the effects on abundances in stellar surfaces of extensive nuclear bombardment required the calculation of more than 105 nuclear-reaction cross sections. It was necessary to develop simplified methods for using the statistical theory of nuclear reactions to make these calculations in order that the computer time should not be prohibitive. These methods are described here and the results are compared with experiment. The accuracy of the calculations is, in general, about as good as, or somewhat better than, that obtained in previous applications of the statistical theory, probably because the use of an accurate level density formula outweighed the crudity of other approximations.Keywords
This publication has 26 references indexed in Scilit:
- () Reactions in Some Elements in the Region ofPhysical Review B, 1964
- Isomer Ratios from () Reactions on SilverPhysical Review B, 1964
- Comparison Between Reactions of Alpha Particles With Scandium-45 and Deuterons with Titanium-47Physical Review B, 1964
- Evidence of nuclear shell effects in Ni58 reactions induced with 0-48 MeV alpha particlesNuclear Physics, 1964
- Statistical Theory Predictions for 5- to 11-MeV () and () Nuclear Reactions in , , , , andPhysical Review B, 1962
- Proton Interactions withandPhysical Review B, 1961
- Proton Cross Sections ofPhysical Review B, 1956
- Survey of () Reactions at 12 MevPhysical Review B, 1955
- An Experimental Verification of the Theory of Compound NucleusPhysical Review B, 1950
- The (α,n) Cross Sections of Beryllium, Magnesium, and AluminumPhysical Review B, 1949