We present a study of the correlations in the arrival times of about 10(6) single and multiple muons detected by the first two MACRO supermodules. The time correlations, from milliseconds to several hundreds of seconds, have been analyzed in terms of the random distribution, with which they are consistent. An analysis of the arrival times (up to 180 ns) of the muons from the same multimuon event is also given.

Ahlen, S.p., Ambrosio, M., Auriemma, G., Baldini, A., Barbarino, G.c., Barish, B., et al. (1992). ARRIVAL TIME DISTRIBUTIONS OF VERY-HIGH-ENERGY COSMIC-RAY MUONS IN MACRO. NUCLEAR PHYSICS. B, 370(2), 432-444 [10.1016/0550-3213(92)90292-J].

ARRIVAL TIME DISTRIBUTIONS OF VERY-HIGH-ENERGY COSMIC-RAY MUONS IN MACRO

BUSSINO, Severino Angelo Maria;
1992

Abstract

We present a study of the correlations in the arrival times of about 10(6) single and multiple muons detected by the first two MACRO supermodules. The time correlations, from milliseconds to several hundreds of seconds, have been analyzed in terms of the random distribution, with which they are consistent. An analysis of the arrival times (up to 180 ns) of the muons from the same multimuon event is also given.
Ahlen, S.p., Ambrosio, M., Auriemma, G., Baldini, A., Barbarino, G.c., Barish, B., et al. (1992). ARRIVAL TIME DISTRIBUTIONS OF VERY-HIGH-ENERGY COSMIC-RAY MUONS IN MACRO. NUCLEAR PHYSICS. B, 370(2), 432-444 [10.1016/0550-3213(92)90292-J].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/124672
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