Boron isotopes in the PAMELA experiment
- Autores: Bogomolov E.A.1, Vasilyev G.I.1, Menn W.2, Adriani O.3,4, Bazilevskaya G.A.5, Barbarino G.6,4, Bellotti R.7,4, Boezio M.8, Bonvicini V.4, Bongi M.3,4, Bottai S.4, Bruno A.7,4, Vacchi A.4,9, Vannuccini E.4, Voronov S.A.8, Galper A.M.8, De Santis C.4,10, Di Felice V.4,11, Zampa G.4, Zampa N.4, Casolino M.4, Campana D.4, Carlson P.12, Castellini G.13, Cafagna F.4, Kvashnin A.A.5, Kvashnin A.N.5, Koldobskiy S.A.8, Lagoida I.A.8, Leonov A.A.8, Mayorov A.G.8, Malakhov V.V.8, Martucci M.10,14, Marcelli L.10, Merge M.4,10, Mikhailov V.V.8, Mocchiutti E.4, Monaco A.7,4, Mori N.4, Munini R.4,15, Osteria G.4, Panico B.4, Papini P.4, Picozza P.4,10, Ricci M.14, Ricciarini S.4, Simon M.2, Sparvoli R.4,10, Spillantini P.3,4, Stozhkov Y.I.5, Yurkin Y.T.8
-
Afiliações:
- Ioffe Institute
- University Siegen
- University of Florence
- INFN
- Lebedev Physical Institute
- University of Naples “Federico II”
- University of Bari
- National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
- University of Udine
- University of Rome “Tor Vergata”
- Agenzia Spaziale Italiana (ASI)
- KTH Royal Institute of Technology
- IFAC
- INFN, Laboratori Nazionali di Frascati
- University of Trieste
- Edição: Volume 87, Nº 2 (2024)
- Páginas: 73-78
- Seção: ЭЛЕМЕНТАРНЫЕ ЧАСТИЦЫ И ПОЛЯ. Эксперимент
- URL: https://journals.rcsi.science/0044-0027/article/view/265620
- DOI: https://doi.org/10.31857/S0044002724020016
- EDN: https://elibrary.ru/KSAWPE
- ID: 265620
Citar
Resumo
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.
Texto integral

Sobre autores
E. Bogomolov
Ioffe Institute
Autor responsável pela correspondência
Email: Edward.Bogomolov@gmail.com
Rússia, Saint-Petersburg
G. Vasilyev
Ioffe Institute
Email: Edward.Bogomolov@gmail.com
Rússia, Saint-Petersburg
W. Menn
University Siegen
Email: Edward.Bogomolov@gmail.com
Alemanha, Siegen
O. Adriani
University of Florence; INFN
Email: Edward.Bogomolov@gmail.com
Department of Physics, Sezione di Florence
Itália, Florence; FlorenceG. Bazilevskaya
Lebedev Physical Institute
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
G. Barbarino
University of Naples “Federico II”; INFN
Email: Edward.Bogomolov@gmail.com
Department of Physics, Sezione di Naples
Itália, Naples; NaplesR. Bellotti
University of Bari; INFN
Email: Edward.Bogomolov@gmail.com
Department of Physics, Sezione di Bari
Itália, Bari; BariM. Boezio
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
V. Bonvicini
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Trieste
Itália, TriesteM. Bongi
University of Florence; INFN
Email: Edward.Bogomolov@gmail.com
Department of Physics, Sezione di Florence
Itália, Florence; FlorenceS. Bottai
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Florence
Itália, FlorenceA. Bruno
University of Bari; INFN
Email: Edward.Bogomolov@gmail.com
Department of Physics, Sezione di Bari
Itália, Bari; BariA. Vacchi
INFN; University of Udine
Email: Edward.Bogomolov@gmail.com
Sezione di Trieste, Department of Mathematics and Informatics
Itália, Trieste; UdineE. Vannuccini
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Florence
Itália, FlorenceS. Voronov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
A. Galper
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
C. De Santis
INFN; University of Rome “Tor Vergata”
Email: Edward.Bogomolov@gmail.com
Sezione di Rome “Tor Vergata”, Department of Physics
Itália, Rome; RomeV. Di Felice
INFN; Agenzia Spaziale Italiana (ASI)
Email: Edward.Bogomolov@gmail.com
Sezione di Rome “Tor Vergata”, Science Data Center
Itália, Rome; RomeG. Zampa
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Trieste
Itália, TriesteN. Zampa
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Trieste
Itália, TriesteM. Casolino
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Rome “Tor Vergata”
Itália, RomeD. Campana
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Naples
Itália, NaplesP. Carlson
KTH Royal Institute of Technology
Email: Edward.Bogomolov@gmail.com
Department of Physics, and the Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre
Suécia, StockholmG. Castellini
IFAC
Email: Edward.Bogomolov@gmail.com
Itália, Florence
F. Cafagna
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Bari
Itália, BariA. Kvashnin
Lebedev Physical Institute
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
A. Kvashnin
Lebedev Physical Institute
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
S. Koldobskiy
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
I. Lagoida
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
A. Leonov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
A. Mayorov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
V. Malakhov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
M. Martucci
University of Rome “Tor Vergata”; INFN, Laboratori Nazionali di Frascati
Email: Edward.Bogomolov@gmail.com
Department of Physics
Itália, Rome; FrascatiL. Marcelli
University of Rome “Tor Vergata”
Email: Edward.Bogomolov@gmail.com
Department of Physics
Itália, RomeM. Merge
INFN; University of Rome “Tor Vergata”
Email: Edward.Bogomolov@gmail.com
Sezione di Rome “Tor Vergata”, Department of Physics
Itália, Rome; RomeV. Mikhailov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
E. Mocchiutti
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Trieste
Itália, TriesteA. Monaco
University of Bari; INFN
Email: Edward.Bogomolov@gmail.com
Department of Physics, Sezione di Bari
Itália, Bari; BariN. Mori
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Florence
Itália, FlorenceR. Munini
INFN; University of Trieste
Email: Edward.Bogomolov@gmail.com
Sezione di Trieste, Department of Physics
Itália, Trieste; TriesteG. Osteria
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Naples
Itália, NaplesB. Panico
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Naples
Itália, NaplesP. Papini
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Florence
Itália, FlorenceP. Picozza
INFN; University of Rome “Tor Vergata”
Email: Edward.Bogomolov@gmail.com
Sezione di Rome “Tor Vergata”, Department of Physics
Itália, Rome; RomeM. Ricci
INFN, Laboratori Nazionali di Frascati
Email: Edward.Bogomolov@gmail.com
Itália, Frascati
S. Ricciarini
INFN
Email: Edward.Bogomolov@gmail.com
Sezione di Florence
Itália, FlorenceM. Simon
University Siegen
Email: Edward.Bogomolov@gmail.com
Alemanha, Siegen
R. Sparvoli
INFN; University of Rome “Tor Vergata”
Email: Edward.Bogomolov@gmail.com
Sezione di Rome “Tor Vergata”, Department of Physics
Itália, Rome; RomeP. Spillantini
University of Florence; INFN
Email: Edward.Bogomolov@gmail.com
Department of Physics, Sezione di Florence
Itália, Florence; FlorenceY. Stozhkov
Lebedev Physical Institute
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
Y. Yurkin
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: Edward.Bogomolov@gmail.com
Rússia, Moscow
Bibliografia
- O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Bottai, A. Bruno, F. Cafagna, D. Campana, P. Carlson, M. Casolino, G. Castellini, et al., Nature 458, 607 (2009).
- E. Petrov, A. M. Bykov, and S. M. Osipov, J. Phys.: Conf. Ser. 1697, 012002 (2020).
- V. Moskalenko, A. W. Strong, S. G. Mashnik, and F. C. Jones, astro-ph/0306349.
- E. A. Bogomolov, G. I. Vasilyev, W. Menn, and S. A. Voronov (on behalf of the PAMELA Collab.), Phys. At. Nucl. 82, 704 (2019).
- W. Menn, E. A. Bogomolov, M. Simon, G. Vasilyev, O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, M. Bongi, V. Bonvicini, S. Bottai, A. Bruno, F. Cafagna, D. Campana, P. Carlson, et al., Astrophys. J. 862, 141 (2018).
- Э. А. Богомолов, Г. И. Васильев, В. Менн, Изв. РАН. Сер. физ. 85, 466 (2021) [Bull. Russ. Acad. Sci.: Phys. 85, 341 (2021)].
- T. Hams, L. M. Barbier, M. Bremerich, E. R. Christian, G. A. de Nolfo, S. Geier, H. Göbel, S. K. Gupta, M. Hof, W. Menn, R. A. Mewaldt, J. W. Mitchell, S. M. Schindler, M. Simon, and R. E. Streitmatter, Astrophys. J. 611, 892 (2004).
- Э. А. Богомолов, Г. И. Васильев, В. Менн, О. Адриани, Г. А. Базилевская, Дж. Барбарино, Р. Белотти, М. Боецио, В. Бонвичини, М. Бонджи, С. Боттаи, А. Бруно, А. Вакки, Е. Ваннуччини, С. А. Воронов, А. М. Гальпер и др., Изв. РАН. Сер. физ. 87, 918 (2023) [Bull. Russ. Acad. Sci.: Phys. 87, 863 (2023)].
- M. Aguilar, L. Ali Cavasonza, G. Ambrosi, L. Arruda, N. Attig, F. Barao, L. Barrin, A. Bartoloni, S. Başeğmez-du Pree, J. Bates, R. Battiston, M. Behlmann, B. Beischer, J. Berdugo, B. Bertucci, V. Bindi, et al., Phys. Rep. 894, 1 (2021), Supplemental material and data.
- M. Aguilar et al. (AMS Collab.), Phys. Rev. Lett. 123, 181102 (2019), Supplemental material and data.
- M. J. Boschini, S. Della Torre, M. Gervasi, D. Grandi, G. Jóhannesson, G. La Vacca, N. Masi, I. V. Moskalenko, S. Pensotti, T. A. Porter, L. Quadrani, P. G. Rancoita, D. Rozza, and M. Tacconi, Astrophys. J. 913, 5 (2021).
- M. Aguilar et al. (AMS Collab.), Phys. Rev. Lett. 126, 041104 (2021), Supplemental material and data.
Arquivos suplementares

Nota
Памяти А.М. Гальпера посвящается