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arxiv: 1307.2345 · v1 · submitted 2013-07-09 · 🌌 astro-ph.IM · astro-ph.HE

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Dark Matter Search Perspectives with GAMMA-400

A.A. Moiseev , A.M. Galper , O. Adriani , R.L. Aptekar , I.V. Arkhangelskaja , A.I. Arkhangelskiy , G.A.Avanesov , L.Bergstrom
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M.Boezio V.Bonvicini K.A.Boyarchuk V.A.Dogiel Yu.V. Gusakov M.I. Fradkin Ch. Fuglesang B.I. Hnatyk V.A. Kachanov V.A. Kaplin M.D. Kheymits V. Korepanov J. Larsson A.A. Leonov F. Longo P. Maestro P. Marrocchesi E.P. Mazets V.V. Mikhailov E. Mocchiutti N. Mori I. Moskalenko P.Yu. Naumov P. Papini M. Pearce P. Picozza M.F. Runtso F. Ryde R. Sparvoli P. Spillantini S.I. Suchkov M. Tavani N.P. Topchiev A. Vacchi E. Vannuccini Yu.T. Yurkin N. Zampa V.N. Zarikashvili V.G. Zverev
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classification 🌌 astro-ph.IM astro-ph.HE
keywords gamma-400gamma-raydarkenergymatteremissiongamma-raysmeasure
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GAMMA-400 is a future high-energy gamma-ray telescope, designed to measure the fluxes of gamma-rays and cosmic-ray electrons + positrons, which can be produced by annihilation or decay of dark matter particles, and to survey the celestial sphere in order to study point and extended sources of gamma-rays, measure energy spectra of Galactic and extragalactic diffuse gamma-ray emission, gamma-ray bursts, and gamma-ray emission from the Sun. GAMMA-400 covers the energy range from 100 MeV to ~3000 GeV. Its angular resolution is ~0.01 deg(Eg > 100 GeV), and the energy resolution ~1% (Eg > 10 GeV). GAMMA-400 is planned to be launched on the Russian space platform Navigator in 2019. The GAMMA-400 perspectives in the search for dark matter in various scenarios are presented in this paper

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