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
Received: 29 Oct 2010 – Revised: 18 Mar 2011 – Accepted: 25 Mar 2011 – Published: 28 Oct 2011
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.