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/2289/5578

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DC Field	Value	Language
dc.contributor.author	Bhattacharjee, Pijushpani	-
dc.contributor.author	Gupta, Nayantara	-
dc.date.accessioned	2013-05-15T08:51:01Z	-
dc.date.available	2013-05-15T08:51:01Z	-
dc.date.issued	2004-03	-
dc.identifier.citation	Pramana, 2004, Vol.62, p789	en
dc.identifier.issn	0304-4289	-
dc.identifier.issn	0973-7111(Online)	-
dc.identifier.uri	http://hdl.handle.net/2289/5578	-
dc.description	Open Access.	en
dc.description.abstract	Gamma ray bursts (GRBs) have been proposed as one possible class of sources of the ultrahigh energy cosmic ray (UHECR) events observed up to energies gtrsim 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-synchrotron origin in GRBs in the up-coming ICECUBE muon detector in the south pole.	en
dc.language.iso	en	en
dc.publisher	Springer Verlag	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2004Prama..62..789B	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0305185	en
dc.relation.uri	http://dx.doi.org/10.1007/BF02705371	en
dc.rights	2004 Springer Verlag	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:	Research Papers (A&A)

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