The Relative Abundances of Tin, Tellurium, Xenon, Barium, and Cerium in the Cosmic Radiation.
Abstract
Elements with even atomic number (Z) in the interval 50 (LESSTHEQ) Z (LESSTHEQ) 58 have been resolved in the cosmic radiation using the Heavy Nuclei Experiment on the HEAO-3 satellite. Their relative abundances have been compared with the results expected from pure r-process material, pure s-process material, and solar system material, both with and without a modification due to possible first ionization potential effects. Such effects may be the result of the preferential accleration, and hence enhancement in the cosmic rays, of those elements having low first ionization potentials. We find that our measurements are inconsistent with pure r-process material at the greater than 98% confidence level whether or not the first ionization potential adjustments are made. In addition, we have compared our results with mixtures having varying ratios of pure r-process material to pure s-process material. We find that, if no first ionization potential effects are included,. (DIAGRAM, TABLE OR GRAPHIC OMITTED...PLEASE SEE DAI). where CRS refers to the cosmic ray source and SS refers to the solar system, consistent with having an almost pure s-process source. If the first ionization potential adjustments are applied. (DIAGRAM, TABLE OR GRAPHIC OMITTED...PLEASE SEE DAI). consistent with a solar system mixture.
- Publication:
-
Ph.D. Thesis
- Pub Date:
- 1983
- Bibcode:
- 1983PhDT.........4K
- Keywords:
-
- Physics: Astronomy and Astrophysics;
- Barium;
- Cerium;
- Cosmic Rays;
- Tellurium;
- Tin;
- Xenon;
- Heao 3;
- Heavy Nuclei;
- Ionization Potentials;
- Solar Physics