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Article: High energy processes in clusters of galaxies and the origin of cosmic rays

TitleHigh energy processes in clusters of galaxies and the origin of cosmic rays
Authors
KeywordsPhysics
Issue Date1996
PublisherAmerican Physical Society. The Journal's web site is located at http://prl.aps.org
Citation
Physical Review Letters, 1996, v. 77 n. 8, p. 1436-1438 How to Cite?
AbstractWe test the hypothesis of a universal cosmic ray intensity by calculating the secondary electron or positron production in the hadronic interactions of cosmic ray nuclei with intergalactic gas within clusters of galaxies. We find that the spectral characteristics of the radio synchrotron emission by these secondary electrons is not consistent with observations of the Coma cluster. Thus the hypothesis can be ruled out on cluster scales.
Persistent Identifierhttp://hdl.handle.net/10722/146673
ISSN
2020 Impact Factor: 9.161
2020 SCImago Journal Rankings: 3.688
ISI Accession Number ID

 

DC FieldValueLanguage
dc.contributor.authorChi, X-
dc.contributor.authorYoung, ECM-
dc.contributor.authorYu, PKN-
dc.contributor.authorZhang, L-
dc.contributor.authorZhu, QQ-
dc.date.accessioned2012-05-09T03:55:52Z-
dc.date.available2012-05-09T03:55:52Z-
dc.date.issued1996-
dc.identifier.citationPhysical Review Letters, 1996, v. 77 n. 8, p. 1436-1438-
dc.identifier.issn0031-9007-
dc.identifier.urihttp://hdl.handle.net/10722/146673-
dc.description.abstractWe test the hypothesis of a universal cosmic ray intensity by calculating the secondary electron or positron production in the hadronic interactions of cosmic ray nuclei with intergalactic gas within clusters of galaxies. We find that the spectral characteristics of the radio synchrotron emission by these secondary electrons is not consistent with observations of the Coma cluster. Thus the hypothesis can be ruled out on cluster scales.-
dc.languageeng-
dc.publisherAmerican Physical Society. The Journal's web site is located at http://prl.aps.org-
dc.relation.ispartofPhysical Review Letters-
dc.rightsCopyright 1996 by The American Physical Society. This article is available online at https://doi.org/10.1103/PhysRevLett.77.1436-
dc.subjectPhysics-
dc.titleHigh energy processes in clusters of galaxies and the origin of cosmic raysen_US
dc.typeArticleen_US
dc.description.naturepublished_or_final_version-
dc.identifier.doi10.1103/PhysRevLett.77.1436-
dc.identifier.pmid10063078-
dc.identifier.scopuseid_2-s2.0-0009200746-
dc.identifier.hkuros22667-
dc.identifier.volume77-
dc.identifier.issue8-
dc.identifier.spage1436-
dc.identifier.epage1438-
dc.identifier.isiWOS:A1996VC33600007-
dc.publisher.placeNew York-
dc.identifier.issnl0031-9007-

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