Title of article
Chemical composition of primary cosmic rays with energies from 10^15 to 10^16.5 eV
Author/Authors
Takeda، M. نويسنده , , Shirasaki، Y. نويسنده , , Kakimoto، F. نويسنده , , Ogio، S. نويسنده , , Gironda، N. نويسنده , , Kaneko، T. نويسنده , , Yoshii، H. نويسنده , , Baba، T. نويسنده , , Sano، S. نويسنده , , Nishi، K. نويسنده , , Tajima، N. نويسنده ,
Issue Information
روزنامه با شماره پیاپی سال 2001
Pages
-356
From page
357
To page
0
Abstract
The study of rapidity gap probability has been carried out with 32S-AgBr interactions at 200 A GeV. The study reveals the scaling behaviour of the void probability in the central rapidity domain which hints towards the outer spaceinner space connection. This also confirms the validity of the linked-pair approximation for the N-particle cumulant correlation functions.
Keywords
Cosmic rays , Extensive air showers , COMPOSITION
Journal title
Astroparticle Physics
Serial Year
2001
Journal title
Astroparticle Physics
Record number
30800
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