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Please use this identifier to cite or link to this item: http://hdl.handle.net/2248/2223
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dc.contributor.authorBhattacharya, D-
dc.date.accessioned2008-04-11T12:10:47Z-
dc.date.available2008-04-11T12:10:47Z-
dc.date.issued2001-
dc.identifier.citationBASI, Vol. 29, No. 2, pp. 107 - 114en
dc.identifier.urihttp://hdl.handle.net/2248/2223-
dc.description.abstractTemporal behaviour of GRB afterglow light curve is derived for the case where the electron energy distribution is relatively hard, with the power-law index p lying between 1.0 and 2.0. It is shown that the expected behaviour will be the same as that for p > 2.0 if the upper cutoff in the electron energy distribution evolves in direct proportion to the bulk Lorentz factor of the blast wave.en
dc.format.extent619098 bytes-
dc.format.mimetypeapplication/pdf-
dc.language.isoenen
dc.publisherAstronomical Society of Indiaen
dc.relation.urihttp://adsabs.harvard.edu/abs/2001BASI...29..107Ben
dc.subjectGamma Ray Burstsen
dc.subjectAfterglowen
dc.subjectRadiation mechanismen
dc.subjectTheoryen
dc.titleFlat Spectrum Gamma Ray Burst Afterglowsen
dc.typeArticleen
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