On the Nuclear Interaction of Non‐lonizing N‐Component of Cosmic‐Rays in Lead at Sea Level (12°N) | Zendy

Bhattacharyya D. P. | Zendy; Das N. C. | Zendy

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On the Nuclear Interaction of Non‐lonizing N‐Component of Cosmic‐Rays in Lead at Sea Level (12°N)

Author(s) -

Bhattacharyya D. P.,

Das N. C.

Publication year - 1971

Publication title -

annalen der physik

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 1.009

H-Index - 68

eISSN - 1521-3889

pISSN - 0003-3804

DOI - 10.1002/andp.19714820213

Subject(s) - cosmic ray , physics , pion , nuclear physics , collision , nucleon , mean free path , coincidence , ionizing radiation , component (thermodynamics) , cross section (physics) , lead (geology) , irradiation , astronomy , medicine , alternative medicine , computer security , pathology , computer science , thermodynamics , electron , geomorphology , geology

The production rate of nuclear interactions by neutral N ‐component of cosmic‐rays of mean energy 15 GeV at sea level was studied as function of absorber thickness by means of a cloud chamber operated by coincidence and anticoincidence technique. The value of collision free path of non‐ionizing N ‐rays in lead was found to be 232 ± 29 g/cm 2 and the collision cross‐section 1.50 ± 0.19 bn. The estimated nucleon inelasticity for pion production in these interactions was 0.4.

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