The underground muon intensity induced by the primaries producing the air shower signal from Cygnus X-3 has been calculated, in both hypothesis of their hadronic or photonic nature. The muon flux measured in NUSEX and SOUDAN experiments is found to be considerably higher than that expected from conventional interactions of the primaries. It is, therefore, impossible to explain both air shower and underground muon fluxes in the frame of conventional interactions.

The high-energy muon flux in air showers from Cygnus X-3 / A. Castellina, B. D’Ettorre Piazzoli, G. Mannocchi, P. Picchi, S. Vernetto, H. Bilokon, E. Meroni. - In: LETTERE AL NUOVO CIMENTO DELLA SOCIETÀ ITALIANA DI FISICA. - ISSN 0375-930X. - 44:7(1985), pp. 491-496. [10.1007/BF02746747]

The high-energy muon flux in air showers from Cygnus X-3

E. Meroni
Ultimo
1985

Abstract

The underground muon intensity induced by the primaries producing the air shower signal from Cygnus X-3 has been calculated, in both hypothesis of their hadronic or photonic nature. The muon flux measured in NUSEX and SOUDAN experiments is found to be considerably higher than that expected from conventional interactions of the primaries. It is, therefore, impossible to explain both air shower and underground muon fluxes in the frame of conventional interactions.
cosmic-rays
Settore FIS/01 - Fisica Sperimentale
Settore FIS/04 - Fisica Nucleare e Subnucleare
1985
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2434/191920
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