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 instrument 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 spectrum in order to search for exotic sources, such as dark matter particle annihilations. PAMELA is also searching for primordial antinuclei (anti‐helium), 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 is investigating phenomena connected with solar and earth physics. Results of the antiproton and positron data will be presented.
The PAMELA Space Mission for Antimatter and Dark Matter Searches in Cosmic Rays / O. Adriani;G. C. Barbarino;G. A. Bazilevskaja;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. De Pascale;C. D. Santis;N. D. Simone;V. D. Felice;A. M. Galper;W. Gillard;P. Hofverberg;S. V. Koldashov;S. Y. Krutkov;A. N. Kvashnin;A. Leonov;V. Malvezzi;L. Marcelli;W. Menn;V. V. Mikhailov;E. Mocchiutti;N. Mori;N. N. Nikonov;G. Osteria;P. Papini;M. Pearce;P. Picozza;M. Ricci;S. B. Ricciarini;M. Simon;R. Sparvoli;P. Spillantini;Y. I. Stozhkov;A. Vacchi;E. Vannuccini;G. Vasilyev;S. A. Voronov;Y. T. Yurkin;G. Zampa;N. Zampa;V. G. Zverev. - STAMPA. - (2010), pp. 33-42. (Intervento presentato al convegno SCIENCE WITH THE NEW GENERATION OF HIGH ENERGY GAMMA‐RAY EXPERIMENTS) [10.1063/1.3395994].
The PAMELA Space Mission for Antimatter and Dark Matter Searches in Cosmic Rays
ADRIANI, OSCAR;BONECHI, LORENZO;BONGI, MASSIMO;MORI, NICOLA;SPILLANTINI, PIERO;
2010
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 instrument 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 spectrum in order to search for exotic sources, such as dark matter particle annihilations. PAMELA is also searching for primordial antinuclei (anti‐helium), 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 is investigating phenomena connected with solar and earth physics. Results of the antiproton and positron data will be presented.
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