Upturn in the ratio of nuclei of Z=1624 to iron observed in the ATIC experiment and the Local Bubble

Author:

Panov A.D.,Sokolskaya N.V.,Zatsepin V.I.

Publisher

Elsevier BV

Subject

Nuclear and High Energy Physics,Atomic and Molecular Physics, and Optics

Reference20 articles.

1. Charge composition and energy spectra of cosmic-ray nuclei for elements from Be to Ni – Results from HEAO-3-C2;Engelmann;A&A,1990

2. Cosmic-ray energy spectra between 10 and several hundred GeV per atomic mass unit for elements from Ar-18 to Ni-28 – results from heao 3;Binns;ApJ,1988

3. Relative abundances of secondary and primary cosmic rays at high energies;Swordy;ApJ,1990

4. Composition of relativistic cosmic rays near the Earth and at the sources;Shapiro,1972

5. Energy spectra of elements with 18≤z≤28 between 10 and 300 GeV/amu;Jones,1985

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1. Review of the Results from the NUCLEON Space Experiment;Bulletin of the Russian Academy of Sciences: Physics;2019-08

2. Cosmic Ray Origin – Beyond the Standard Models;Nuclear and Particle Physics Proceedings;2018-04

3. Origin of the spectral upturn in the cosmic-rayC/FeandO/Feratios;Physical Review D;2015-09-02

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