The Space Mission PAMELA, launched in orbit on June 15th 2006, represents the stateof- the-art of the investigation of the cosmic radiation to addressing the most compelling issues facing astrophysics and cosmology: the nature of the dark matter that pervades the universe, the apparent absence of cosmological antimatter, the origin and evolution of matter in the galaxy. The primary scientific goal of the Pamela investigation is the search for evidence of non baryonic particles falling outside Standard Model particle physics and of heavy antinuclei. Concomitant, but not secondary, goals are the study of the energy dependence of cosmic ray lifetimes in the Galaxy, the validation of models of acceleration, transport and secondary production of cosmic radiation in the Galaxy, the monitoring of the solar activity and the knowledge of the role of solar and terrestrial relationships in the energetic particle propagation in the heliosphere. The observational objectives are the measurements of the fluxes and the energy spectra of antiprotons, protons, positrons, electrons and light nuclei in a very large energy range and the search for antinuclei with a sensitivity of the order of 10-8 in He/He.
The physics of PAMELA space mission / Picozza, P.; Adriani, O.; Ambriola, M.; Barbarino, G.C.; Basili, A.; Bazilevskaja, G.A.; Bellotti, R.; Boezio, M.; Bogomolov, E.A.; Bonechi, L.; Bongi, M.; Bongiorno, L.; Bonvicini, V.; Bruno, A.; Cafagna, F.; Campana, D.; Carlson, P.; Casolino, M.; Castellini, G.; De Marzo, C.; Conrad, J.; De Pascale, M.P.; De Rosa, G.; Di Felice, V.; Fedele, D.; Galper, A.M.; Hofverberg, P.; Koldashov, S.V.; Krutkov, S.Yu.; Kvashnin, A.N.; Lundquist, J.; Maksumov, O.; Malvezzi, V.; Marcelli, L.; Menn, W.; Mikhailov, V.V.; Minori, M.; Misin, S.; Mocchiutti, E.; Morselli, A.; Nikonov, N.N.; Orsi, S.; Osteria, G.; Papini, P.; Pearce, M.; Picozza, P.; Ricci, M.; Ricciarini, S.B.; Runtso, M.F.; Russo, S.; Simon, M.; Sparvoli, R.; Spillantini, P.; Stozhkov, Yu.I.; Taddei, E.; Vacchi, A.; Vannuccini, E.; Vasilyev, G.; Voronov, S.A.; Yurkin, Y.T.; Zampa, G.; Zampa, N.; Zverev, V.G.. - ELETTRONICO. - 2:(2007), pp. 19-22. (Intervento presentato al convegno 30th International Cosmic Ray Conference, ICRC 2007 tenutosi a Merida, Yucatan, mex nel 2007).
The physics of PAMELA space mission
ADRIANI, OSCAR;BONGI, MASSIMO;
2007
Abstract
The Space Mission PAMELA, launched in orbit on June 15th 2006, represents the stateof- the-art of the investigation of the cosmic radiation to addressing the most compelling issues facing astrophysics and cosmology: the nature of the dark matter that pervades the universe, the apparent absence of cosmological antimatter, the origin and evolution of matter in the galaxy. The primary scientific goal of the Pamela investigation is the search for evidence of non baryonic particles falling outside Standard Model particle physics and of heavy antinuclei. Concomitant, but not secondary, goals are the study of the energy dependence of cosmic ray lifetimes in the Galaxy, the validation of models of acceleration, transport and secondary production of cosmic radiation in the Galaxy, the monitoring of the solar activity and the knowledge of the role of solar and terrestrial relationships in the energetic particle propagation in the heliosphere. The observational objectives are the measurements of the fluxes and the energy spectra of antiprotons, protons, positrons, electrons and light nuclei in a very large energy range and the search for antinuclei with a sensitivity of the order of 10-8 in He/He.
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