The Relative Abundances of Sn, Te, Xe, Ba, and Ce in the Cosmic Radiation
<p>Elements with even atomic number (Z) in the interval 50 ≤ Z ≤ 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...
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| Format: | Others |
| Language: | en |
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1983
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| Online Access: | https://thesis.library.caltech.edu/8685/1/Krombel_ke_1983.pdf Krombel, Keith E. (1983) The Relative Abundances of Sn, Te, Xe, Ba, and Ce in the Cosmic Radiation. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/h4fg-6z05. https://resolver.caltech.edu/CaltechTHESIS:10092014-110007312 <https://resolver.caltech.edu/CaltechTHESIS:10092014-110007312> |
Internet
https://thesis.library.caltech.edu/8685/1/Krombel_ke_1983.pdfKrombel, Keith E. (1983) The Relative Abundances of Sn, Te, Xe, Ba, and Ce in the Cosmic Radiation. Dissertation (Ph.D.), California Institute of Technology. doi:10.7907/h4fg-6z05. https://resolver.caltech.edu/CaltechTHESIS:10092014-110007312 <https://resolver.caltech.edu/CaltechTHESIS:10092014-110007312>