| Autor: |
Galper, A. M., Aptekar, R. L., Arkhangelskaya, I. V., Boezio, M., Bonvicini, V., Dolgoshein, B. A., Farber, M. O., Fradkin, M. I., Gecha, V. Ya., Kachanov, V. A., Kaplin, V. A., Mazets, E. P., Menshenin, A. L., Picozza, P., Prilutskii, O. F., Rodin, V. G., Runtso, M. F., Spillantini, P., Suchkov, S. I., Topchiev, N. P. |
| Předmět: |
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| Zdroj: |
Astrophysics & Space Sciences Transactions (ASTRA); 2011, Vol. 7 Issue 1, p75-78, 4p, 1 Diagram, 1 Chart |
| Abstrakt: |
The GAMMA-400 space observatory will provide precise measurements of gamma rays, electrons, and positrons in the energy range 0.1-3000 GeV. The good angular and energy resolutions, as well as identification capabilities (angular resolution ∼ 0.01°, energy resolution ∼ 1%, and proton rejection factor ∼ 106) will allow us to study the main galactic and extragalactic sources, diffuse gamma-ray background, gamma-ray bursts, and to measure electron and positron fluxes. The peculiar characteristics of the experiment is simultaneous detection of gamma rays and cosmic-ray electrons and positrons, which can be connected with annihilation or decay of dark matter particles. [ABSTRACT FROM AUTHOR] |
| Databáze: |
Complementary Index |
| Externí odkaz: |
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