Cosmic ray pion-nucleon flux ratio in the atmosphere
- 21 October 1975
- journal article
- Published by IOP Publishing in Journal of Physics G: Nuclear Physics
- Vol. 1 (8) , L63-L65
- https://doi.org/10.1088/0305-4616/1/8/001
Abstract
Using the Bose-type distribution of the form E(d3 sigma /d3p)=Ax square root s/(exp( epsilon ( lambda )/T)-1) for p+p to pi -+x reactions in ISR experiments at centre of mass energy square root s=53 GeV, the cosmic ray pion-nucleon flux ratio in the atmosphere is estimated. The invariant pion-nucleon flux ratio yields the temperature dependence on energy square root s in the following way: T=0.129( sigma in/ square root s)14.6/.Keywords
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