Talk detail

MG14 - Talk detail

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 Participant

Leonov, Alexey

Institution

P.N. Lebedev Physical Institute of the Russian Academy of Sciences  - 53 Leninskij Prospekt - Moscow - Moscow - Russia

Session

HE4

Accepted

Order

Time

Talk

Oral abstract

Title

The GAMMA-400 Space Mission for Measuring High-Energy Gamma Rays and Cosmic Rays
Coauthors

Abstract

The scientific goals of the GAMMA-400 space mission and the design of the new space-based gamma-ray telescope GAMMA-400 are presented. GAMMA-400 is a dual experiment dedicated to the study of gamma rays and electrons, protons and nuclei. It has aimed to a broad range of scientific topics, such as search for signatures of dark matter, studies of Galactic and extragalactic gamma-ray sources, especially Galactic Center, Galactic and extragalactic diffuse emission, as well as high-precision measurements of cosmic rays spectra. GAMMA-400 will have the best parameters when measuring gamma rays: the angular resolution ~0.01 deg. (at 100 GeV), the energy resolution ~1% (at 100 GeV), and the proton rejection factor ~10^6 and will be able to measure gamma-ray and cosmic-ray electron + positron fluxes in the energy range from 100 MeV to 20 TeV, as well as protons and nuclei up to the knee (10^15-10^16 eV).

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