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PAMELA: Measurements of matter and antimatter in space

  • N. De Simone
  • , G. Jerse
  • , E. Mocchiutti
  • , 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, L. Consiglio, M. P. DePascale, C. De Santis, V. Di Felice, A. M. Galper, W. Gillard, L. Grishantseva, A. V. Karelin, S. V. Koldashov, S. Y. Krutkov, A. N. Kvashnin, A. Leonov, O. Maksumov, V. Malakhov, V. Malvezzi, L. Marcelli, A. G. Mayorov, W. Menn, A. Monaco, V. V. Mikhailov, N. Mori, N. N. Nikonov, G. Osteria, F. Palma, P. Papini, M. Pearce, P. Picozza, C. Pizzolotto, M. Ricci, S. B. Ricciarini, L. Rossetto, M. Runtso, R. Sarkar, M. Simon, R. Sparvoli, P. Spillantini, Y. I. Stozhkov, A. Vacchi, E. Vannuccini, G. Vasilyev, S. A. Voronov, J. Wu, Y. T. Yurkin, G. Zampa, N. Zampa, V. G. Zverev
  • National Institute for Nuclear Physics
  • University of Rome Tor Vergata
  • University of Florence
  • University of Naples Federico II
  • RAS - P.N. Lebedev Physics Institute
  • University of Bari
  • RAS - Ioffe Physico Technical Institute
  • Moscow Engineering Physics Institute
  • AlbaNova University Center
  • IFAC
  • University of Siegen

Research output: Contribution to journalArticlepeer-review

Abstract

On the 15th of June 2006, the PAMELA satellite-borne experiment was launched from the Baikonur cosmodrome and it has been collecting data since July 2006. The apparatus comprises a time-of-flight system, a silicon-microstrip magnetic spectrometer, a silicon-tungsten electromagnetic calorimeter, an anticoincidence system, a shower tail counter scintillator and a neutron detector. The combination of these devices allows precision studies of the charged cosmic radiation to be conducted over a wide energy range (100 MeV-100's GeV) with high statistics. The primary scientific goal is the measurement of the antiproton and positron energy spectra in order to search for exotic sources, such as dark matter particle annihilations. PAMELA is also searching for primordial antinuclei (antihelium), and testing cosmic-ray propagation models through precise measurements of the antiparticle energy spectrum and precision studies of light nuclei and their isotopes. Moreover, PAMELA investigates phenomena connected with solar and earth physics. The main results and updated data will be presented.

Original languageEnglish
Pages (from-to)79-87
Number of pages9
JournalNuovo Cimento della Societa Italiana di Fisica C
Volume34
Issue number3
DOIs
StatePublished - 2011
Externally publishedYes

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