PAMELA and indirect dark matter searches (Articolo in rivista)

Type
Label
  • PAMELA and indirect dark matter searches (Articolo in rivista) (literal)
Anno
  • 2009-01-01T00:00:00+01:00 (literal)
Alternative label
  • S.V. Borisov, M. Boezio, S.A. Voronov, A.M. Galper, O. Adriani, P. Picozza, G. Castellini, et al. (2009)
    PAMELA and indirect dark matter searches
    in New journal of physics
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • S.V. Borisov, M. Boezio, S.A. Voronov, A.M. Galper, O. Adriani, P. Picozza, G. Castellini, et al. (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 11 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#affiliazioni
  • 1. Ist Nazl Fis Nucl, Sez Trieste, I-34012 Trieste, Italy 2. KTH, Dept Phys, S-10691 Stockholm, Sweden 3. AlbaNova Univ Ctr, Oskar Klein Ctr Cosmoparticle Phys, S-10691 Stockholm, Sweden 4. Univ Roma Tor Vergata, Dept Phys, I-00133 Rome, Italy 5. Ist Nazl Fis Nucl, Sez Roma Tor Vergata, I-00133 Rome, Italy 6. Univ Florence, Dept Phys, I-50019 Florence, Italy 7. Ist Nazl Fis Nucl, Sez Florence, I-50019 Florence, Italy 8. Univ Naples Federico 2, Dept Phys, I-80126 Naples, Italy 9. Ist Nazl Fis Nucl, Sez Naples, I-80126 Naples, Italy 10. PN Lebedev Phys Inst, RU-119991 Moscow, Russia 11. Univ Bari, Dept Phys, I-70126 Bari, Italy 12. Ist Nazl Fis Nucl, Sez Bari, I-70126 Bari, Italy 13. AF Ioffe Phys Tech Inst, RU-194021 St Petersburg, Russia 14. Moscow Engn & Phys Inst, RU-11540 Moscow, Russia 15. IFAC, I-50019 Florence, Italy 16. Univ Siegen, D-57068 Siegen, Germany 17. Ist Nazl Fis Nucl, Lab Nazl Frascati, I-00044 Frascati, Italy (literal)
Titolo
  • PAMELA and indirect dark matter searches (literal)
Abstract
  • We present a review of the experimental results obtained by PAMELA in measuring the (p, (p) over bar ) and e(+/-) abundance in cosmic rays. In this context, we discuss the interpretation of the observed anomalous positron excess in terms of the annihilation of dark matter particles as well as in terms of standard astrophysical sources. Moreover we show the constraints on dark matter models from (p) over bar data. (literal)
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