GAMMA
Appearance
The GAMMA experiment is a study of:
- Primary
- gamma-ray intensity at energies 1014–1015eV[4]
- Extensive scintillation counters
- Hard jets production at energies ~1016eV by the muon multi-core shower events
The GAMMA experiment is deployed on the South side of
GeV
.
The results of GAMMA experiment for 2004–2010 runs are presented in references below .[7]
References
- ^ A.P. Garyaka; R.M. Martirosov; S.V. Ter-Antonyan; A.D. Erlykin; N.M. Nikolskaya; Y.A. Gallant; L.W. Jones; J. Procureur (2008). "All-particle primary energy spectrum in the 3-200 PeV energy range". .
- ^ A.P. Garyaka; R.M. Martirosov; S.V. Ter-Antonyan; N. Nikolskaya; Y.A. Gallant; L. Jones; J. Procureur (2007). "Rigidity-dependent cosmic ray energy spectra in the knee region obtained with the GAMMA experiment". .
- ^ S.V. Ter-Antonyan (2007). "Mutually compensative pseudo solutions of primary energy spectra in the knee region". .
- ^
R.M. Martirosov; S.V. Ter-Antonyan; A.D. Erlykin; A.P. Garyaka; N.M. Nikolskaya; Y.A. Gallant; L.W. Jones (2009). "Galactic diffuse gamma-ray flux at the energy about 175 TeV". arXiv:0905.3593 [astro-ph.GA].
- ^ https://asbarez.com/physicists-at-armenias-cosmic-ray-division-publish-new-discoveries-on-mount-aragats
- ^ http://crd.yerphi.am/Highlights_of_Aragats_Research
- ^ Samvel Ter-Antonyan (2014). "Sharp knee phenomenon of primary cosmic ray energy spectrum". .