Boron isotopes in the PAMELA experiment

In this work, a new analysis of the isotopic composition of boron nuclei (B) in galactic cosmic rays (GCR) 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 the contribution of several local sources from explosions of nearby (hundreds of parsec) supernovae.

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Ядерная физика
Published
2024-10-07
DOI
https://doi.org/10.31857/s0044002724020016
Primary Topic
Dark Matter and Cosmic Phenomena
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article
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article

Boron isotopes in the PAMELA experiment

P. Carlson, G. Osteria, S. Ricciarini, G. C. Barbarino et al.
Ядерная физика
Dark Matter and Cosmic Phenomena
article

Boron isotopes in the PAMELA experiment

P. Carlson, G. Osteria, S. Ricciarini, G. C. Barbarino, V. V. Mikhailov, Alfonso Monaco, D. Campana, A. M. Galper, R. Bellotti, S. A. Voronov, E. Mocchiutti, А. Н. Квашнин, N. Mōri, Y. I. Stozhkov, S. Koldobskiy, A. Vacchi, M. Martucci, W. Menn, M. Bongi, R. Munini, V. Bonvicini, G. Vasilyev, M. Boezio, P. Papini, М. Мерге, V. Malakhov, G. A. Bazilevskaya, I. A. Lagoida, G. Zampa, M. Ricci, N. Zampa, G. Castellini, É. A. Bogomolov, Aleksey A. Leonov, B. Panico, F. Cafagna, C. De Santis, Y. T. Yurkin, A. Bruno, R. Sparvoli, L. Marcelli, M. Casolino, P. Picozza, E. Vannuccini, O. Adriani, A. G. Mayorov, V. Di Felice, A. A. Kvashnin, S. Bottai, П. Спиллантини, M. Simon
article en

Abstract

In this work, a new analysis of the isotopic composition of boron nuclei (B) in galactic cosmic rays (GCR) 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 the contribution of several local sources from explosions of nearby (hundreds of parsec) supernovae.

Ядерная физикаVol. 87(2)
University of Rome Tor Vergata (IT), P.N. Lebedev Physical Institute of the Russian Academy of Sciences (RU), University of Udine (IT), University of Trieste (IT), University of Siegen (DE), Agenzia Spaziale Italiana (IT), Nello Carrara Institute of Applied Physics (IT), Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali di Frascati (IT), University of Florence (IT), University of Bari Aldo Moro (IT), University of Naples Federico II (IT), KTH Royal Institute of Technology (SE), National Research Nuclear University MEPhI (RU), Ioffe Institute (RU)
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