Astrophys. Space Sci. Trans., 7, 483-486, 2011
www.astrophys-space-sci-trans.net/7/483/2011/
doi:10.5194/astra-7-483-2011
© Author(s) 2011. This work is distributed
under the Creative Commons Attribution 3.0 License.
 
28 Oct 2011
On the energy spectrum of cosmic ray muons in 100 TeV region
Yu. F. Novoseltsev1, A. G. Bogdanov2, R. P. Kokoulin2, R. V. Novoseltseva1, V. B. Petkov1, and A. A. Petrukhin2
1Institute for Nuclear Research of RAS, 361609 Neutrino, KBR, Russia
2National Research Nuclear University MEPhI, 115409 Moscow, Russia

Abstract. The energy spectrum of cosmic ray muons in the energy range from several TeV to ~1 PeV obtained by means of the analysis of multiple interactions of muons (pair meter technique) in the Baksan underground scintillation telescope is presented. Some evidence for the additional muon flux (to the conventional one from pion and kaon decays) has been obtained at energies ~100 TeV.

Citation: Novoseltsev, Yu. F., Bogdanov, A. G., Kokoulin, R. P., Novoseltseva, R. V., Petkov, V. B., and Petrukhin, A. A.: On the energy spectrum of cosmic ray muons in 100 TeV region, Astrophys. Space Sci. Trans., 7, 483-486, doi:10.5194/astra-7-483-2011, 2011.
 
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