3-11 July 2007
Merida, Mexico
Mexico/General timezone
- icrc2007@icrc2007.unam.mx
Support
Contribution Poster (WITHDRAWN)
OG.1.2
Coma supercluster an origin for the the highest energy protons in observed Cosmic Rays flux.
Speakers
- Mrs. Pantea DAVOUDIFAR
Primary authors
- Mrs. Pantea DAVOUDIFAR (PhD student in Astroparticle Physics/Kerman University)
Co-authors
- Prof. S. Jalil Aldin FATEMI (Professor of physics in Kerman univercity)
- Mr. Hamid ARJOMAND KERMANI (PhD student in Astroparticle Physics/Kerman University)
Abstract content
In the present work, after our work about the extragalactic gamma ray flux in direction of Coma supercluster , with considering the Virgo proton flux and considering a constant gamma to proton ratio for the very high energy cosmic rays in first approximation, the extragalactic proton flux in Coma direction is calculated. we have studied that is it possible that the coma supercluster be an origin for the highest energy protons in cosmic rays flux or not. a detailed analysis has made.