On the interaction of cosmic rays with matter under 50 metres water equivalent View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1952-10

AUTHORS

E. Amaldi, C. Castagnoli, A. Gigli, S. Sciuti

ABSTRACT

The production of penetrating secondaries by cosmic rays at 50 m w.e. has been investigated by means of a counter hodoscope. The cross section (in lead) for events which can be interpreted as pairs of associated penetrating particles (a.p.p.) is not larger than (13±3)·10−30 cm2/nucleon. Such a value is deduced from measurements of the corresponding differential cross section as a function of the penetration of the secondary particles produced (section 4·3 table V). A value of the same order of magnitude is found for the production ofa.p.p. in rock (section 4·5). Furthermore it is shown that the events that can be interpreted as showers penetrating 15 cm Pb, have a frequency that can be explained, at least in part, as due to purely electromagnetic interaction. Therefore one can establish an upper limit of a few units in 10−30 cm2/nucleon for the cross section for production in Pb of penetrating showers by μ-mesons. Finally we discuss those events which appear to be due to a few penetrating particles coming from the rock and it is shown that they can be accounted for, by considering besides the production of penetrating showers in rock the penetrating particles present in the vicinity of the core of extensive air showers. More... »

PAGES

969-1003

Identifiers

URI

http://scigraph.springernature.com/pub.10.1007/bf02786163

DOI

http://dx.doi.org/10.1007/bf02786163

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1052002616


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