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Distribution of Shower Particles as Obtained in the Analysis of a 10 + 13p Shower Event
Author(s) -
Bandyopadhyay B. K.,
Daftari I. K.,
Roy T.
Publication year - 1974
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.19744860203
Subject(s) - shower , event (particle physics) , physics , cluster (spacecraft) , nuclear physics , pion , diagram , meteor shower , nuclear emulsion , distribution (mathematics) , resonance (particle physics) , particle physics , air shower , astrophysics , statistics , meteorology , mathematics , mathematical analysis , meteor (satellite) , computer science , nozzle , thermodynamics , programming language , cosmic ray
We present here the analysis of an accelerator produced 10 + 13 p shower event observed in nuclear emulsion. The D ULLER ‐W ALKER method is applied to obtain the distribution of secondary shower particles, and the particles having the closest log 10 tan θ L values are taken to form a cluster. This cluster formation is also confirmed by the target diagram method. If this cluster is conceived to be a high spin resonance and the secondary pions to be the decay products of this resonance, then the azimuthal integral distribution curve fits fairly well with our experimental data.