| Autor: |
Bagulya, A. V., Chernyavsky, M. M., Goncharova, L. A., Granich, G. M., Gorshenkov, M. V., Kalinina, G. V., Konovalova, N. S., Okat'eva, N. M., Pavlova, T. A., Polukhina, N. G., Shchedrina, T. V., Savchenko, E. S., Starkov, N. I., Soe, Tan Naing, Vladymyrov, M. S. |
| Předmět: |
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| Zdroj: |
AIP Conference Proceedings; 2015, Vol. 1702, p1-6, 6p, 1 Color Photograph, 1 Black and White Photograph, 5 Graphs |
| Abstrakt: |
An original method of studying chemically etched tracks of heavy nuclei in olivine from pallasite meteorites was used to obtain a charge distribution of approximately 9000 nuclei with charges above 55 in galactic cosmic rays. Three superheavy nuclei with the charges in the range of 105+10-6 with the probability of 95%. Such nuclei have to form islands of stability of superheavy elements; their occurrence in nature supports the validity of theoretical predictions and justifies efforts for their synthesis under the Earth conditions. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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