Ultrahigh energy cosmic rays from gamma ray bursts: implications of the recent observational results by Milagro

Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/4464

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DC Field	Value	Language
dc.contributor.author	Gupta, Nayantara	-
dc.date.accessioned	2012-05-08T04:44:33Z	-
dc.date.available	2012-05-08T04:44:33Z	-
dc.date.issued	2005-03	-
dc.identifier.citation	Astroparticle Physics, 2005, Vol.23, p227	en
dc.identifier.issn	0927-6505	-
dc.identifier.uri	http://hdl.handle.net/2289/4464	-
dc.description	Restricted Access. An open-access version is available at arXiv.org (one of the alternative locations)	en
dc.description.abstract	It has been speculated earlier that gamma ray bursts are sources of ultrahigh energy cosmic rays. Recently, the search for high energy photons from Gamma Ray Bursts by Milagro group has put limits on the isotropic luminosity of these transient sources in very high energy photons. The implications of the results obtained by Milagro to our understanding of the ultrahigh energy cosmic ray spectrum from these sources have been discussed in the present work.	en
dc.language.iso	en	en
dc.publisher	Elsevier B.V.	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2005APh....23..227G	en
dc.relation.uri	http://arxiv.org/abs/astro-ph/0406087	en
dc.relation.uri	http://dx.doi.org/10.1016/j.astropartphys.2004.12.005	en
dc.rights	2005 Elsevier B.V.	en
dc.subject	gamma-ray sources	en
dc.subject	gamma-ray bursts	en
dc.subject	gamma-ray	en
dc.title	Ultrahigh energy cosmic rays from gamma ray bursts: implications of the recent observational results by Milagro	en
dc.type	Article	en
Appears in Collections:	Research Papers (A&A)

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