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Abstract
The GAMMA-400 gamma-ray telescope with excellent angular and energy resolutions is designed to search for signatures of dark matter in the fluxes of gamma-ray emission and electrons + positrons. Precision investigations of gamma-ray emission from Galactic Center, Crab, Vela, Cygnus, Geminga, and other regions will be performed, as well as diffuse gamma-ray emission, along with measurements of high-energy electron + positron and nuclei fluxes. Furthermore, it will study gamma-ray bursts and gamma-ray emission from the Sun during periods of solar activity. The GAMMA-400 energy range is expected to be from ∼20 MeV up to TeV energies for gamma rays, up to 10 TeV for electrons + positrons, and up to 1015 eV for cosmic-ray nuclei. For 100-GeV gamma rays, the GAMMA-400 angular resolution is ∼0.01° and energy resolution is ∼1%; the proton rejection factor is ∼5x105. GAMMA-400 will be installed onboard the Russian space observatory.
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Details
1 Lebedev Physical Institute, RU-119991 Moscow, Russia
2 Lebedev Physical Institute, RU-119991 Moscow, Russia; National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Kashirskoe highway 31, Moscow, 115409, Russia
3 Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34149 Trieste, Italy
4 Istituto Nazionale di Fisica Nucleare, Sezione di Florence, I-50019 Sesto Fiorentino, Florence, Italy
5 Ioffe Physical Technical Institute, RU-194021 St. Petersburg, Russia
6 National Research Nuclear University MEPhI (Moscow Engineering Physics Institute), Kashirskoe highway 31, Moscow, 115409, Russia
7 The Oskar Klein Centre, Department of Physics, Stockholm University, AlbaNova University Center, SE-106 91, Stockholm, Sweden
8 Department of Physical Sciences, Earth and Environment, University of Siena and Istituto Nazionale di Fisica Nucleare, Sezione di Pisa, Italy
9 Scientific Research Institute for System Analysis, RU-117218, Moscow, Russia
10 Istituto di Fisica Applicata Nello Carrara, I-50019, Sesto Fiorentino, Florence, Italy
11 Istituto Nazionale di Fisica Nucleare, Sezione di Pavia, I-27100, Pavia, Italy
12 Istituto Nazionale di Fisica Nucleare, Sezione di Trieste, I-34149 Trieste, Italy; Institut de Fisica d'Altes Energies, Bellaterra, Spain
13 Istituto Nazionale di Fisica Nucleare, Sezione di Rome “Tor Vergata”, I-00133, Rome, Italy
14 Departament d'Astronomia i Meteorologia, Institut de Ciències del Cosmos, Universitat de Barcelona, Spain
15 Taras Shevchenko National University, Kyiv, 01601, Ukraine
16 Lviv Center of Institute of Space Research, Lviv, 79060, Ukraine
17 KTH Royal Institute of Technology, Department of Physics and the Oskar Klein Centre, AlbaNova University Center, SE-10691, Stockholm, Sweden
18 Institut de Fisica d'Altes Energies, Bellaterra, Spain
19 Research Institute for Electromechanics, RU-143502 Istra, Moscow region, Russia
20 NASA Goddard Space Flight Center and CRESST/University of Maryland, Greenbelt, Maryland 20771, USA
21 Hansen Experimental Physics Laboratory and Kavli Institute for Particle Astrophysics and Cosmology, Stanford University, Stanford, CA, 94305, USA
22 Istituto Nazionale di Astrofisica IASF and Physics Department of University of Rome Tor Vergata, I-00133, Roma, Italy
23 Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation, Troitsk, Moscow region, Russia