GAMMA-400 is a new space mission scheduled to be launched at the end of the current decade on-board the Russian space platform Navigator. Theexperimental apparatus is designed for simultaneous detection of gamma and cosmic rays in a broad energy range: 100 MeV - 3 TeV for photons, 1 GeV - 20 TeV for electrons and positrons, and up to 1015-1016 eV for p and He. The characteristics of the instrument are optimized to address some of the most impelling science topics, such as search for signatures of dark matter, studies of Galactic and extragalactic gamma-ray sources, Galactic and extragalactic diffuse emission, gamma-ray bursts, as well as high-precision measurements of the spectra of cosmic-ray electrons + positrons and nuclei. experimental apparatus is designed for simultaneous detection of gamma and cosmic rays in a broad energy range: 100 MeV - 3 TeV for photons, 1 GeV - 20 TeV for electrons and positrons, and up to 1015-1016 eV for p and He. The characteristics of the instrument are optimized to address some of the most impelling science topics, such as search for signatures of dark matter, studies of Galactic and extragalactic gamma-ray sources, Galactic and extragalactic diffuse emission, gamma-ray bursts, as well as high-precision measurements of the spectra of cosmic-ray electrons + positrons and nuclei.
The GAMMA-400 mission / Bonvicini, Valter; Galper, A.M.; Topchiev, N.P.; Adriani, O.; Aptekar, R.L.; Arkhangelskaja, I.V.; Arkhangelskiy, A.I.; Bergstrom, L.; Berti, E.; Bigongiari, G.; Bobkov, S.G.; Boezio, M.; Bogomolov, E.A.; Bonechi, S.; Bongi, M.; Bottai, S.; Boyarchuk, K.A.; Castellini, G.; Cattaneo, P.W.; Cumani, P.; Dedenko, G.L.; De Donato, C.; Dogiel, V.A.; Fuglesang, Ch.; Gorbunov, M.S.; Gusakov, Yu.V.; Hnatyk, B.I.; Kadilin, V.V.; Kaplin, V.A.; Kaplun, A.A.; Kheymits, M.D.; Korepanov, V.E.; Larsson, J.; Leonov, A.A.; Loginov, V.A.; Longo, F.; Maestro, P.; Marrocchesi, P.S.; Mikhailov, V.V.; Mocchiutti, E.; Moiseev, A.A.; Mori, N.; Moskalenko, I.V.; Naumov, P.Yu.; Papini, P.; Pearce, M.; Picozza, P.; Popov, A.V.; Rappoldi, A.; Ricciarini, S.; Runtso, M.F.; Ryde, F.; Sarkar, R.; Serdin, O.V.; Sparvoli, R.; Spillantini, P.; Suchkov, S.I.; Tavani, M.; Taraskin, A.A.; Tiberio, A.; Tyurin, E.M.; Ulanov, M.V.; Vacchi, A.; Vannuccini, E.; Vasilyev, G.I.; Yurkin, Yu.T.; Zampa, N.; Zarikashvili, V.N.; Zverev, V.G.. - ELETTRONICO. - 58:(2014), pp. 300-306. (Intervento presentato al convegno 15th Vulcano Workshop: Frontier Objects in Astrophysics and Particle Physics 2014 tenutosi a Conference Room of the Therasia Resort, ita nel 2014).
The GAMMA-400 mission
ADRIANI, OSCAR;BERTI, EUGENIO;BONGI, MASSIMO;MORI, NICOLA;SPILLANTINI, PIERO;TIBERIO, ALESSIO;
2014
Abstract
GAMMA-400 is a new space mission scheduled to be launched at the end of the current decade on-board the Russian space platform Navigator. Theexperimental apparatus is designed for simultaneous detection of gamma and cosmic rays in a broad energy range: 100 MeV - 3 TeV for photons, 1 GeV - 20 TeV for electrons and positrons, and up to 1015-1016 eV for p and He. The characteristics of the instrument are optimized to address some of the most impelling science topics, such as search for signatures of dark matter, studies of Galactic and extragalactic gamma-ray sources, Galactic and extragalactic diffuse emission, gamma-ray bursts, as well as high-precision measurements of the spectra of cosmic-ray electrons + positrons and nuclei. experimental apparatus is designed for simultaneous detection of gamma and cosmic rays in a broad energy range: 100 MeV - 3 TeV for photons, 1 GeV - 20 TeV for electrons and positrons, and up to 1015-1016 eV for p and He. The characteristics of the instrument are optimized to address some of the most impelling science topics, such as search for signatures of dark matter, studies of Galactic and extragalactic gamma-ray sources, Galactic and extragalactic diffuse emission, gamma-ray bursts, as well as high-precision measurements of the spectra of cosmic-ray electrons + positrons and nuclei.I documenti in FLORE sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.