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Measurement of Boron and Carbon Fluxes in Cosmic Rays with the Pamela Experiment

Adriani, O. (author)
Barbarino, G. C. (author)
Bazilevskaya, G. A. (author)
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Bellotti, R. (author)
Boezio, M. (author)
Bogomolov, E. A. (author)
Bongi, M. (author)
Bonvicini, V. (author)
Bottai, S. (author)
Bruno, A. (author)
Cafagna, F. (author)
Campana, D. (author)
Carbone, R. (author)
Carlson, Per (author)
KTH,Fysik
Casolino, M. (author)
Castellini, G. (author)
Danilchenko, I. A. (author)
De Donato, C. (author)
De Santis, C. (author)
De Simone, N. (author)
Di Felice, V. (author)
Formato, V. (author)
Galper, A. M. (author)
Karelin, A. V. (author)
Koldashov, S. V. (author)
Koldobskiy, S. (author)
Krutkov, S. Y. (author)
Kvashnin, A. N. (author)
Leonov, A. (author)
Malakhov, V. (author)
Marcelli, L. (author)
Martucci, M. (author)
Mayorov, A. G. (author)
Menn, W. (author)
Merge, M. (author)
Mikhailov, V. V. (author)
Mocchiutti, E. (author)
Monaco, A. (author)
Mori, N. (author)
Munini, R. (author)
Osteria, G. (author)
Palma, F. (author)
Panico, B. (author)
Papini, P. (author)
Pearce, Mark (author)
KTH,Partikel- och astropartikelfysik,Oskar Klein Centre for Cosmoparticle Physics, AlbaNova University Centre, Sweden
Picozza, P. (author)
Pizzolotto, C. (author)
Ricci, M. (author)
Ricciarini, S. B. (author)
Rossetto, L. (author)
Sarkar, R. (author)
Scotti, V. (author)
Simon, M. (author)
Sparvoli, R. (author)
Spillantini, P. (author)
Stozhkov, Y. I. (author)
Vacchi, A. (author)
Vannuccini, E. (author)
Vasilyev, G. I. (author)
Voronov, S. A. (author)
Yurkin, Y. T. (author)
Zampa, G. (author)
Zampa, N. (author)
Zverev, V. G. (author)
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 (creator_code:org_t)
2014
2014
English.
In: Astrophysical Journal. - 0004-637X .- 1538-4357. ; 791:2, s. 93-
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The propagation of cosmic rays inside our galaxy plays a fundamental role in shaping their injection spectra into those observed at Earth. One of the best tools to investigate this issue is the ratio of fluxes for secondary and primary species. The boron-to-carbon (B/C) ratio, in particular, is a sensitive probe to investigate propagation mechanisms. This paper presents new measurements of the absolute fluxes of boron and carbon nuclei as well as the B/C ratio from the PAMELA space experiment. The results span the range 0.44-129 GeV/n in kinetic energy for data taken in the period 2006 July to 2008 March.

Subject headings

NATURVETENSKAP  -- Fysik -- Astronomi, astrofysik och kosmologi (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Astronomy, Astrophysics and Cosmology (hsv//eng)

Keyword

astroparticle physics
cosmic rays

Publication and Content Type

ref (subject category)
art (subject category)

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