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- Publisher Website: 10.1103/PhysRevLett.77.1436
- Scopus: eid_2-s2.0-0009200746
- PMID: 10063078
- WOS: WOS:A1996VC33600007
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Article: High energy processes in clusters of galaxies and the origin of cosmic rays
Title | High energy processes in clusters of galaxies and the origin of cosmic rays |
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Authors | |
Keywords | Physics |
Issue Date | 1996 |
Publisher | American 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? |
Abstract | We 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 Identifier | http://hdl.handle.net/10722/146673 |
ISSN | 2023 Impact Factor: 8.1 2023 SCImago Journal Rankings: 3.040 |
ISI Accession Number ID |
DC Field | Value | Language |
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dc.contributor.author | Chi, X | - |
dc.contributor.author | Young, ECM | - |
dc.contributor.author | Yu, PKN | - |
dc.contributor.author | Zhang, L | - |
dc.contributor.author | Zhu, QQ | - |
dc.date.accessioned | 2012-05-09T03:55:52Z | - |
dc.date.available | 2012-05-09T03:55:52Z | - |
dc.date.issued | 1996 | - |
dc.identifier.citation | Physical Review Letters, 1996, v. 77 n. 8, p. 1436-1438 | - |
dc.identifier.issn | 0031-9007 | - |
dc.identifier.uri | http://hdl.handle.net/10722/146673 | - |
dc.description.abstract | We 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.language | eng | - |
dc.publisher | American Physical Society. The Journal's web site is located at http://prl.aps.org | - |
dc.relation.ispartof | Physical Review Letters | - |
dc.rights | Copyright 1996 by The American Physical Society. This article is available online at https://doi.org/10.1103/PhysRevLett.77.1436 | - |
dc.subject | Physics | - |
dc.title | High energy processes in clusters of galaxies and the origin of cosmic rays | en_US |
dc.type | Article | en_US |
dc.description.nature | published_or_final_version | - |
dc.identifier.doi | 10.1103/PhysRevLett.77.1436 | - |
dc.identifier.pmid | 10063078 | - |
dc.identifier.scopus | eid_2-s2.0-0009200746 | - |
dc.identifier.hkuros | 22667 | - |
dc.identifier.volume | 77 | - |
dc.identifier.issue | 8 | - |
dc.identifier.spage | 1436 | - |
dc.identifier.epage | 1438 | - |
dc.identifier.isi | WOS:A1996VC33600007 | - |
dc.publisher.place | New York | - |
dc.identifier.issnl | 0031-9007 | - |