Detailed analysis of observed antiprotons in cosmic rays

In the present work, the origin of antiprotons observed in cosmic rays (above the atmosphere) is analyzed in details. We have considered the origin of the primaries, (which their interactions with the interstellar medium is one of the most important sources of antiprotons) is a supernova type II the...

Full description

Bibliographic Details
Main Authors: P Davoudifar, SJ Fatemi
Format: Article
Language:English
Published: Isfahan University of Technology 2009-12-01
Series:Iranian Journal of Physics Research
Subjects:
Online Access:http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-428&slc_lang=en&sid=1
_version_ 1819155731976290304
author P Davoudifar
SJ Fatemi
author_facet P Davoudifar
SJ Fatemi
author_sort P Davoudifar
collection DOAJ
description In the present work, the origin of antiprotons observed in cosmic rays (above the atmosphere) is analyzed in details. We have considered the origin of the primaries, (which their interactions with the interstellar medium is one of the most important sources of antiprotons) is a supernova type II then used a diffusion model for their propagation. We have used the latest parameterization for antiproton production cross section in pp collisions (instead of well known parameterization introduced by Tan et al.) as well as our calculated residence time for primaries. The resulted intensity shows the secondary antiprotons produced in pp collisions in the galaxy, have a high population as one can not consider an excess for extragalactic antiprotons. Also there is a high degree of uncertainty in different parameters.
first_indexed 2024-12-22T15:41:39Z
format Article
id doaj.art-7a87bb5d2aff4bd89042537e0d6bf6c6
institution Directory Open Access Journal
issn 1682-6957
language English
last_indexed 2024-12-22T15:41:39Z
publishDate 2009-12-01
publisher Isfahan University of Technology
record_format Article
series Iranian Journal of Physics Research
spelling doaj.art-7a87bb5d2aff4bd89042537e0d6bf6c62022-12-21T18:21:07ZengIsfahan University of TechnologyIranian Journal of Physics Research1682-69572009-12-0193291291Detailed analysis of observed antiprotons in cosmic raysP DavoudifarSJ FatemiIn the present work, the origin of antiprotons observed in cosmic rays (above the atmosphere) is analyzed in details. We have considered the origin of the primaries, (which their interactions with the interstellar medium is one of the most important sources of antiprotons) is a supernova type II then used a diffusion model for their propagation. We have used the latest parameterization for antiproton production cross section in pp collisions (instead of well known parameterization introduced by Tan et al.) as well as our calculated residence time for primaries. The resulted intensity shows the secondary antiprotons produced in pp collisions in the galaxy, have a high population as one can not consider an excess for extragalactic antiprotons. Also there is a high degree of uncertainty in different parameters.http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-428&slc_lang=en&sid=1cosmic raysinterstellar mediumcosmic rays (origin)
spellingShingle P Davoudifar
SJ Fatemi
Detailed analysis of observed antiprotons in cosmic rays
Iranian Journal of Physics Research
cosmic rays
interstellar medium
cosmic rays (origin)
title Detailed analysis of observed antiprotons in cosmic rays
title_full Detailed analysis of observed antiprotons in cosmic rays
title_fullStr Detailed analysis of observed antiprotons in cosmic rays
title_full_unstemmed Detailed analysis of observed antiprotons in cosmic rays
title_short Detailed analysis of observed antiprotons in cosmic rays
title_sort detailed analysis of observed antiprotons in cosmic rays
topic cosmic rays
interstellar medium
cosmic rays (origin)
url http://ijpr.iut.ac.ir/browse.php?a_code=A-10-1-428&slc_lang=en&sid=1
work_keys_str_mv AT pdavoudifar detailedanalysisofobservedantiprotonsincosmicrays
AT sjfatemi detailedanalysisofobservedantiprotonsincosmicrays