中国科学院机构知识库网格
Chinese Academy of Sciences Institutional Repositories Grid
CHARGE SPECTRUM OF HEAVY AND SUPERHEAVY COMPONENTS OF GALACTIC COSMIC RAYS: RESULTS OF THE OLIMPIYA EXPERIMENT

文献类型:期刊论文

作者Alexeev, Victor1; Bagulya, Alexander2; Chernyavsky, Mikhail2; Gippius, Alexei2; Goncharova, Lyudmila2; Gorbunov, Sergei2; Gorshenkov, Mikhail3; Kalinina, Galina1; Konovalova, Nina2; Liu, Jie4
刊名ASTROPHYSICAL JOURNAL
出版日期2016-10-01
卷号829页码:18
ISSN号0004-637X
关键词acceleration of particles elementary particles nuclear reactions, nucleosynthesis, abundances Physical data and processes
DOI10.3847/0004-637X/829/2/120
英文摘要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 Vetch 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.
WOS关键词OLIVINE CRYSTALS ; FOSSIL TRACK ; ION TRACKS ; R-PROCESS ; NUCLEI Z-GREATER-THAN-OR-EQUAL-TO-110 ; CHEMICAL-COMPOSITION ; METEORITE OLIVINES ; SUPERNOVA REMNANT ; PARTICLE TRACKS ; ELEMENTS
资助项目Russian Foundation for Basic Research, Russia[16-38-00877] ; Russian Foundation for Basic Research, Russia[15-02-02875]
WOS研究方向Astronomy & Astrophysics
语种英语
出版者IOP PUBLISHING LTD
WOS记录号WOS:000385377200062
资助机构Russian Foundation for Basic Research, Russia
源URL[http://119.78.100.186/handle/113462/24484]  
专题中国科学院近代物理研究所
通讯作者Alexeev, Victor
作者单位1.Russian Acad Sci, Vernadsky Inst Geochem & Analyt Chem, 19 Kosygin Str, Moscow 119991, Russia
2.Russian Acad Sci, Lebedev Phys Inst, 53 Leninsky Prosp, Moscow 119991, Russia
3.Natl Univ Sci & Technol MISIS, 4 Leninsky Prosp, Moscow 119049, Russia
4.Chinese Acad Sci, Inst Modern Phys, 509 Nanchang Rd, Lanzhou 730000, Peoples R China
5.Natl Res Nucl Univ MEPhI, 31 Kashirskoe Shosse, Moscow 115409, Russia
6.GSI Helmholtzzentrum Schwerionenforsch, Darmstadt, Germany
7.Tech Univ Darmstadt, Darmstadt, Germany
8.Natl Res Ctr, Kurchatov Inst, 1 Kurchatov Sq, Moscow 123182, Russia
9.Joint Inst Nucl Res, Flerov Lab Nucl React, 6 Joliot Curie St, Dubna 141980, Russia
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Alexeev, Victor,Bagulya, Alexander,Chernyavsky, Mikhail,et al. CHARGE SPECTRUM OF HEAVY AND SUPERHEAVY COMPONENTS OF GALACTIC COSMIC RAYS: RESULTS OF THE OLIMPIYA EXPERIMENT[J]. ASTROPHYSICAL JOURNAL,2016,829:18.
APA Alexeev, Victor.,Bagulya, Alexander.,Chernyavsky, Mikhail.,Gippius, Alexei.,Goncharova, Lyudmila.,...&Volkov, Alexander.(2016).CHARGE SPECTRUM OF HEAVY AND SUPERHEAVY COMPONENTS OF GALACTIC COSMIC RAYS: RESULTS OF THE OLIMPIYA EXPERIMENT.ASTROPHYSICAL JOURNAL,829,18.
MLA Alexeev, Victor,et al."CHARGE SPECTRUM OF HEAVY AND SUPERHEAVY COMPONENTS OF GALACTIC COSMIC RAYS: RESULTS OF THE OLIMPIYA EXPERIMENT".ASTROPHYSICAL JOURNAL 829(2016):18.

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来源:近代物理研究所

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