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Boron Isotopes in the PAMELA Experiment

Bogomolov, E. A. (author)
Russian Acad Sci, Ioffe Inst, St Petersburg 194021, Russia.
Carlson, Per (author)
KTH,Partikelfysik, astrofysik och medicinsk bildbehandling
Yurkin, Yu. T. (author)
Natl Res Nucl Univ, MEPhI Moscow Engn Phys Inst, Moscow 115409, Russia.
Russian Acad Sci, Ioffe Inst, St Petersburg 194021, Russia Partikelfysik, astrofysik och medicinsk bildbehandling (creator_code:org_t)
Pleiades Publishing Ltd, 2024
2024
English.
In: Physics of Atomic Nuclei. - : Pleiades Publishing Ltd. - 1063-7788 .- 1562-692X. ; 87:2, s. 71-76
  • Journal article (peer-reviewed)
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  • In this work, a new analysis of the isotopic composition of boron nuclei (B) in galactic cosmic rays (GCRs) in the range of rigidities of 1-5 GV (nuclear energies 0.1-1.5 GeV/nucleon) was carried out using data from the PAMELA space experiment 2006-2014 on the rigidity of detected nuclei and their velocity (time-of-flight analysis and ionization losses in the instrument's multilayer calorimeter). The new results of the PAMELA experiment expand the energy range of previous measurements, are consistent with the few existing data, and indicate deviations of the B isotope ratios from the GALPROP simulation data for the GCR, similar to the deviations for the Li and Be isotopes in the PAMELA data, which can be interpreted as evidence of observation against the background of the GCR of the contribution of several local sources from explosions of nearby (hundreds of parsecs) supernovae.

Subject headings

NATURVETENSKAP  -- Fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences (hsv//eng)

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Bogomolov, E. A.
Carlson, Per
Yurkin, Yu. T.
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NATURAL SCIENCES
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Physics of Atomi ...
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