On the non-acceleration origin of the highest energy cosmic rays

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/4230

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DC Field	Value	Language
dc.contributor.author	Sivaram, C	-
dc.date.accessioned	2009-01-02T11:15:41Z	-
dc.date.available	2009-01-02T11:15:41Z	-
dc.date.issued	1993	-
dc.identifier.citation	D. A. Leahy, R. B. Hickws, and D. Venkatesan., eds., 23rd International Cosmic Ray Conference, Vol. 2, held 19 - 30 July, 1993 at University of Calgary, Alberta, Canada.	en
dc.identifier.uri	http://hdl.handle.net/2248/4230	-
dc.description.abstract	The Hawking radiation from primordial black holes in their near terminal stages of evaporation can produce ultra high energy (UHE) particles spontaneously. The contribution from such objects to the highest energy cosmic rays observed is estimated. Comparison is made with the UHE particle production from cosmic topological defects such as strings and monopoles.	en
dc.language.iso	en	en
dc.publisher	University of Calgary	en
dc.relation.ispartofseries	International Cosmic Ray Conference; Vol. 2	-
dc.relation.uri	http://adsabs.harvard.edu/abs/1993ICRC....2..326S	en
dc.title	On the non-acceleration origin of the highest energy cosmic rays	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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