http://www.cnr.it/ontology/cnr/individuo/prodotto/ID23013
PAMELA Results on the Cosmic-Ray Antiproton Flux from 60 MeV to 180 GeV in Kinetic Energy (Articolo in rivista)
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- 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
- Rivista
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- 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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