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Detecting galactic cosmic ray transuranium nuclei in olivine crystals from meteorites
Authors:A B Alexandrov  A V Bagulya  M S Vladimirov  L A Goncharova  A I Ivliev  G V Kalinina  L L Kashkarov  N S Konovalova  N M Okateva  N G Polukhina  A S Roussetski  N I Starkov
Institution:1. Lebedev Physical Institute, Russian Academy of Sciences, Moscow, 119991, Russia
2. Vernadsky Institute of Geochemistry and Analytical Chemistry, Russian Academy of Sciences, Moscow, 119991, Russia
Abstract:Results from the experimental search for and identification of tracks from the superheavy and transuranium nuclei of galactic cosmic rays in pallacite olivine crystals, conducted as part of project OLIMPIA 1], are presented. To date, 170 crystals from Marjalahti and Eagle Station pallacites have been processed and 6800 tracks corresponding to nuclei with charges Z > 55 have been found; 45 of these are from nuclei with charges of 88 < Z < 92 and three super-long ones were produced by nuclei with Z > 105. The charge of one of these nuclei is estimated in the first approximation as Z = 119(+10,?6). Our data confirm the hypothesis of islands of stability for natural trans-Fermi nuclei.
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