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

Type
Label
  • PAMELA Results on the Cosmic-Ray Antiproton Flux from 60 MeV to 180 GeV in Kinetic Energy (Articolo in rivista) (literal)
Anno
  • 2010-01-01T00:00:00+01:00 (literal)
Alternative label
  • O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, et al. (2010)
    PAMELA Results on the Cosmic-Ray Antiproton Flux from 60 MeV to 180 GeV in Kinetic Energy
    in Physical review letters (Print)
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • O. Adriani, G. C. Barbarino, G. A. Bazilevskaya, R. Bellotti, M. Boezio, E. A. Bogomolov, L. Bonechi, M. Bongi, V. Bonvicini, S. Borisov, S. Bottai, A. Bruno, F. Cafagna, D. Campana, R. Carbone, P. Carlson, M. Casolino, G. Castellini, et al. (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 105 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • 1. Univ Florence, Dept Phys, I-50019 Florence, Italy 2. INFN, Sez Firenze, I-50019 Florence, Italy 3. Univ Naples Federico 2, Dept Phys, I-80126 Naples, Italy 4. INFN, Sez Napoli, I-80126 Naples, Italy 5. PN Lebedev Phys Inst, RU-119991 Moscow, Russia 6. Univ Bari, Dept Phys, I-70126 Bari, Italy 7. INFN, Sez Bari, I-70126 Bari, Italy 8. INFN, Sez Trieste, I-34149 Trieste, Italy 9. AF Ioffe Phys Tech Inst, RU-194021 St Petersburg, Russia 10. INFN, Sez Roma Tor Vergata, I-00133 Rome, Italy 11. Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy 12. Moscow Engn & Phys Inst, RU-11540 Moscow, Russia 13. AlbaNova Univ Ctr, Oskar Klein Ctr Cosmoparticle Phys, SE-10691 Stockholm, Sweden 14. KTH, Dept Phys, SE-10691 Stockholm, Sweden 15. IFAC, I-50019 Florence, Italy 16. Univ Trieste, Dept Phys, I-34147 Trieste, Italy 17. Univ Siegen, Dept Phys, D-57068 Siegen, Germany 18. Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy (literal)
Titolo
  • PAMELA Results on the Cosmic-Ray Antiproton Flux from 60 MeV to 180 GeV in Kinetic Energy (literal)
Abstract
  • 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. (literal)
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