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Charge spectrum of heavy and superheavy components of galactic cosmic rays: results of the Olimpiya Experiment

Alexeev, Victor ; Bagulya, Alexander ; Chernyavsky, Mikhail ; Gippius, Alexei ; Goncharova, Lyudmila ; Gorbunov, Sergei ; Gorshenkov, Mikhail ; Kalinina, Galina ; Konovalova, Nina ; Liu, Jie ; Zhai, Pengfei ; Okatyeva, Natalia ; Pavlova, Tatyana ; Polukhina, Natalia ; Starkov, Nikolai ; Soe, Than Naing ; Trautmann, Christina ; Savchenko, Elena ; Shchedrina, Tatyana ; Vasiliev, Alexander ; Volkov, Alexander (2016)
Charge spectrum of heavy and superheavy components of galactic cosmic rays: results of the Olimpiya Experiment.
In: The Astrophysical Journal, 829 (2)
doi: 10.3847/0004-637X/829/2/120
Artikel, Bibliographie

Kurzbeschreibung (Abstract)

The aim of the OLIMPIYA experiment is to search for and identify traces of heavy and superheavy nuclei of galactic cosmic rays (GCR) in olivine crystals from stony–iron meteorites serving as nuclear track detectors. The method is based on layer-by-layer grinding and etching of particle tracks in these crystals. Unlike the techniques of other authors, this annealing-free method uses two parameters: the etching rate along the track (V etch) and the total track length (L), to identify charge Z of a projectile. A series of irradiations with different swift heavy ions at the accelerator facilities of GSI (Darmstadt) and IMP (Lanzhou) were performed in order to determine and calibrate the dependence of projectile charge on V etch and L. To date, one of the most essential results of the experiment is the obtained charge spectrum of GCR nuclei within the range of Z > 40, based on about 11.6 thousand processed tracks. As the result of data processing, 384 nuclei with charges Z ≥ 75 have been identified, including 10 nuclei identified as actinides (90 < Z < 103). Three tracks were identified to be produced by nuclei with charges 113 < Z < 129. Such nuclei may be part of the Island of Stability of transfermium elements.

Typ des Eintrags: Artikel
Erschienen: 2016
Autor(en): Alexeev, Victor ; Bagulya, Alexander ; Chernyavsky, Mikhail ; Gippius, Alexei ; Goncharova, Lyudmila ; Gorbunov, Sergei ; Gorshenkov, Mikhail ; Kalinina, Galina ; Konovalova, Nina ; Liu, Jie ; Zhai, Pengfei ; Okatyeva, Natalia ; Pavlova, Tatyana ; Polukhina, Natalia ; Starkov, Nikolai ; Soe, Than Naing ; Trautmann, Christina ; Savchenko, Elena ; Shchedrina, Tatyana ; Vasiliev, Alexander ; Volkov, Alexander
Art des Eintrags: Bibliographie
Titel: Charge spectrum of heavy and superheavy components of galactic cosmic rays: results of the Olimpiya Experiment
Sprache: Englisch
Publikationsjahr: 28 September 2016
Verlag: IOP Publishing
Titel der Zeitschrift, Zeitung oder Schriftenreihe: The Astrophysical Journal
Jahrgang/Volume einer Zeitschrift: 829
(Heft-)Nummer: 2
DOI: 10.3847/0004-637X/829/2/120
Kurzbeschreibung (Abstract):

The aim of the OLIMPIYA experiment is to search for and identify traces of heavy and superheavy nuclei of galactic cosmic rays (GCR) in olivine crystals from stony–iron meteorites serving as nuclear track detectors. The method is based on layer-by-layer grinding and etching of particle tracks in these crystals. Unlike the techniques of other authors, this annealing-free method uses two parameters: the etching rate along the track (V etch) and the total track length (L), to identify charge Z of a projectile. A series of irradiations with different swift heavy ions at the accelerator facilities of GSI (Darmstadt) and IMP (Lanzhou) were performed in order to determine and calibrate the dependence of projectile charge on V etch and L. To date, one of the most essential results of the experiment is the obtained charge spectrum of GCR nuclei within the range of Z > 40, based on about 11.6 thousand processed tracks. As the result of data processing, 384 nuclei with charges Z ≥ 75 have been identified, including 10 nuclei identified as actinides (90 < Z < 103). Three tracks were identified to be produced by nuclei with charges 113 < Z < 129. Such nuclei may be part of the Island of Stability of transfermium elements.

Fachbereich(e)/-gebiet(e): 11 Fachbereich Material- und Geowissenschaften
11 Fachbereich Material- und Geowissenschaften > Materialwissenschaft
11 Fachbereich Material- und Geowissenschaften > Materialwissenschaft > Fachgebiet Ionenstrahlmodifizierte Materialien
Hinterlegungsdatum: 29 Dez 2017 09:36
Letzte Änderung: 13 Mär 2024 12:14
PPN:
Sponsoren: S.A. Gorbunov and A.E. Volkov acknowledge financial support from the Russian Foundation for Basic Research, Russia (Grants 16-38-00877 and 15-02-02875, respectively).
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