Ultra-high energy cosmic rays and prompt TeV gamma rays from gamma ray bursts

Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/3605

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DC Field	Value	Language
dc.contributor.author	Bhattacharjee, P	-
dc.contributor.author	Gupta, N	-
dc.date.accessioned	2008-09-15T10:32:34Z	-
dc.date.available	2008-09-15T10:32:34Z	-
dc.date.issued	2004-03	-
dc.identifier.citation	Pramana Journal of Physics, Vol. 62, No. 3, pp. 789 - 792	en
dc.identifier.issn	0304-4289	-
dc.identifier.uri	http://hdl.handle.net/2248/3605	-
dc.description.abstract	Gamma ray bursts (CRBs) have been proposed as one possible class of sources of the ultrahigh energy cosmic ray (UHECR) events observed up to energies greater than or similar to 10(20) eV. The synchrotron radiation of the highest energy protons accelerated within the GRB source should produce gamma rays up to TeV energies. Here we briefly discuss the implications on the energetics of the GRB From the point of view of the detectability of the prompt TeV gamma-rays of proton-sychrotron origin in GRBs in the up-coming ICE CUBE muon detector in the south pole.	en
dc.language.iso	en	en
dc.publisher	Indian Academy of Sciences	en
dc.relation.uri	http://www.ias.ac.in/pramana/v62/v62no3.htm	en
dc.subject	Gamma ray bursts	en
dc.subject	Ulta-high energy cosmic rays	en
dc.subject	TeV gamma rays	en
dc.title	Ultra-high energy cosmic rays and prompt TeV gamma rays from gamma ray bursts	en
dc.type	Article	en
Appears in Collections:	IIAP Publications

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