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PAMELA Results on the Cosmic-Ray Antiproton Flux from 60 MeV to 180 GeV in Kinetic Energy

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)
Bonechi, L. (author)
Bongi, M. (author)
Bonvicini, V. (author)
Borisov, S. (author)
Bottai, S. (author)
Bruno, A. (author)
Cafagna, F. (author)
Campana, D. (author)
Carbone, R. (author)
Carlson, Per (author)
KTH,Partikel- och astropartikelfysik
Casolino, M. (author)
Castellini, G. (author)
Consiglio, L. (author)
De Pascale, M. P. (author)
De Santis, C. (author)
De Simone, N. (author)
Di Felice, V. (author)
Galper, A. M. (author)
Gillard, William (author)
KTH,Partikel- och astropartikelfysik
Grishantseva, L. (author)
Hofverberg, Petter (author)
KTH,Partikel- och astropartikelfysik
Jerse, G. (author)
Karelin, A. V. (author)
Koldashov, S. V. (author)
Krutkov, S. Y. (author)
Kvashnin, A. N. (author)
Leonov, A. (author)
Malvezzi, V. (author)
Marcelli, L. (author)
Mayorov, A. G. (author)
Menn, W. (author)
Mikhailov, V. V. (author)
Mocchiutti, E. (author)
Monaco, A. (author)
Mori, N. (author)
Nikonov, N. (author)
Osteria, G. (author)
Papini, P. (author)
Pearce, Mark (author)
KTH,Partikel- och astropartikelfysik
Picozza, P. (author)
Pizzolotto, C. (author)
Ricci, M. (author)
Ricciarini, S. B. (author)
Rossetto, Laura (author)
KTH,Partikel- och astropartikelfysik
Simon, M. (author)
Sparvoli, R. (author)
Spillantini, P. (author)
Stozhkov, Y. I. (author)
Vacchi, A. (author)
Vannuccini, E. (author)
Vasilyev, G. (author)
Voronov, S. A. (author)
Wu, Juan (author)
KTH,Partikel- och astropartikelfysik
Yurkin, Y. T. (author)
Zampa, G. (author)
Zampa, N. (author)
Zverev, V. G. (author)
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 (creator_code:org_t)
2010
2010
English.
In: Physical Review Letters. - 0031-9007 .- 1079-7114. ; 105:12, s. 121101-
  • Journal article (peer-reviewed)
Abstract Subject headings
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  • The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray antiproton flux and the antiproton-to-proton flux ratio which extends previously published measurements down to 60 MeV and up to 180 GeV in kinetic energy. During 850 days of data acquisition approximately 1500 antiprotons were observed. The measurements are consistent with purely secondary production of antiprotons in the Galaxy. More precise secondary production models are required for a complete interpretation of the results.

Subject headings

NATURVETENSKAP  -- Fysik -- Subatomär fysik (hsv//swe)
NATURAL SCIENCES  -- Physical Sciences -- Subatomic Physics (hsv//eng)

Keyword

Antiproton flux
Proton flux
Satellite-borne experiment
Secondary production
Cosmic rays
Electron energy loss spectroscopy
High energy physics
Kinetic energy
Astroparticle physics
Astropartikelfysik

Publication and Content Type

ref (subject category)
art (subject category)

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