Boron isotopes in the PAMELA experiment

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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.

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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; Florence

G. 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; Naples

R. Bellotti

University of Bari; INFN

Email: Edward.Bogomolov@gmail.com

Department of Physics, Sezione di Bari

Itália, Bari; Bari

M. 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, Trieste

M. Bongi

University of Florence; INFN

Email: Edward.Bogomolov@gmail.com

Department of Physics, Sezione di Florence

Itália, Florence; Florence

S. Bottai

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Florence

Itália, Florence

A. Bruno

University of Bari; INFN

Email: Edward.Bogomolov@gmail.com

Department of Physics, Sezione di Bari

Itália, Bari; Bari

A. Vacchi

INFN; University of Udine

Email: Edward.Bogomolov@gmail.com

Sezione di Trieste, Department of Mathematics and Informatics

Itália, Trieste; Udine

E. Vannuccini

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Florence

Itália, Florence

S. 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; Rome

V. Di Felice

INFN; Agenzia Spaziale Italiana (ASI)

Email: Edward.Bogomolov@gmail.com

Sezione di Rome “Tor Vergata”, Science Data Center

Itália, Rome; Rome

G. Zampa

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Trieste

Itália, Trieste

N. Zampa

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Trieste

Itália, Trieste

M. Casolino

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Rome “Tor Vergata”

Itália, Rome

D. Campana

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Naples

Itália, Naples

P. 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, Stockholm

G. Castellini

IFAC

Email: Edward.Bogomolov@gmail.com
Itália, Florence

F. Cafagna

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Bari

Itália, Bari

A. 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; Frascati

L. Marcelli

University of Rome “Tor Vergata”

Email: Edward.Bogomolov@gmail.com

Department of Physics

Itália, Rome

M. Merge

INFN; University of Rome “Tor Vergata”

Email: Edward.Bogomolov@gmail.com

Sezione di Rome “Tor Vergata”, Department of Physics

Itália, Rome; Rome

V. 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, Trieste

A. Monaco

University of Bari; INFN

Email: Edward.Bogomolov@gmail.com

Department of Physics, Sezione di Bari

Itália, Bari; Bari

N. Mori

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Florence

Itália, Florence

R. Munini

INFN; University of Trieste

Email: Edward.Bogomolov@gmail.com

Sezione di Trieste, Department of Physics

Itália, Trieste; Trieste

G. Osteria

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Naples

Itália, Naples

B. Panico

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Naples

Itália, Naples

P. Papini

INFN

Email: Edward.Bogomolov@gmail.com

Sezione di Florence

Itália, Florence

P. Picozza

INFN; University of Rome “Tor Vergata”

Email: Edward.Bogomolov@gmail.com

Sezione di Rome “Tor Vergata”, Department of Physics

Itália, Rome; Rome

M. 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, Florence

M. 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; Rome

P. Spillantini

University of Florence; INFN

Email: Edward.Bogomolov@gmail.com

Department of Physics, Sezione di Florence

Itália, Florence; Florence

Y. 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

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  4. E. A. Bogomolov, G. I. Vasilyev, W. Menn, and S. A. Voronov (on behalf of the PAMELA Collab.), Phys. At. Nucl. 82, 704 (2019).
  5. 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).
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Arquivos suplementares

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1. JATS XML
2. Fig. 1. 11B/10B ratios depending on the hardness of the nuclei.

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3. Fig. 2. Spectra of 10B and 11B nuclei depending on hardness.

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4. Fig. 3. Spectra of nuclei 10B and 11B depending on energy.

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5. Fig. 4. 11B/10B ratios as a function of nuclear energy.

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6. Fig. 5. AMS-02 and PAMELA, antiproton spectra at hardness 1–10 GV.

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Nota

Памяти А.М. Гальпера посвящается


Declaração de direitos autorais © Russian Academy of Sciences, 2024