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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4524
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dc.contributor.authorBhattacharjee, P-
dc.date.accessioned2009-06-08T15:00:23Z-
dc.date.available2009-06-08T15:00:23Z-
dc.date.issued1995-
dc.identifier.citationCowsik, R. ed., Non-accelerator particle physics., Proceedings of Intlernational Conference on Non-accelerator particle physics., Indian Institute of Astrophysics., Bangalore, 2 - 9 Jan, 1994, India, pp. 329 - 340en
dc.identifier.isbn981-02-1811-7-
dc.identifier.urihttp://hdl.handle.net/2248/4524-
dc.description.abstractThe model of origin of ultrahigh energy (UHE) (i.e., energy E~> 10sup/8 eV) cosmic rays from cosmic topological defects such as cosmic strings, magnetic monopoles, etc., is discussed. We discuss the general nature of the predicted spectra of protons, gamma rays and neutrinos resulting from TD-induced processes and discuss he predicted magnitude of contribution of some specific processes involving specific kinds of TDs to the UHE cosmic ray flux.en
dc.language.isoenen
dc.publisherWorld Scientificen
dc.rightsRestricted Access-
dc.subjectCosmic Raysen
dc.subjectCosmic Stringsen
dc.subjectTopological Defectsen
dc.subjectUHEen
dc.subjectUltrahigh Energyen
dc.subjectCosmic Topological Defectsen
dc.subjectMagnetic Monopolesen
dc.subjectSpectra of Protonsen
dc.subjectCosmic Ray Fluxen
dc.subjectGamma Raysen
dc.titleCosmic rays from cosmic strings and other topological defectsen
dc.typeArticleen
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