Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2127
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dc.contributor.authorJain, D-
dc.contributor.authorPanchapakesan, N-
dc.contributor.authorMahajan, S-
dc.contributor.authorBhatia, V. B-
dc.date.accessioned2008-03-05T11:35:11Z-
dc.date.available2008-03-05T11:35:11Z-
dc.date.issued2000-
dc.identifier.citationBASI, Vol. 28, No. 2, pp. 377 - 379en
dc.identifier.urihttp://hdl.handle.net/2248/2127-
dc.description.abstractIdentification of gravitationally lensed Gamma Ray Bursts (GRBs) in the BATSE 4B catalog can be used to constrain the average redshift <z> of the GRBs. Here we calculate an upper limit to <z>, independent of the physical model for GRBs, using a filled beam approximation to compute the lensing rate for GRBs at high z for a variety of cosmologies. The upper limit on <z> depends directly on the cosmological parameters ? and ?. The other factor which can change the <z> of GRBs is the evolution of the lensing galaxies. We find that merging of lensing galaxies puts the GRBs at higher redshift as compare to non evolving model of galaxies.en
dc.format.extent215913 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2000BASI...28..377Jen
dc.subjectGravitational lensingen
dc.subjectGamma ray burstsen
dc.subjectEvolution of galaxiesen
dc.titleLimit on the average redshift of Gamma Ray Bursts from evolving galaxiesen
dc.typeArticleen
Appears in Collections:BASI Publications

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