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dc.contributor.authorBhattacharya, D.-
dc.identifier.citationBulletin of the Astronomical Society of India, 2001, Vol.29, p107-114en
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.extent619131 bytes-
dc.publisherThe Astronomical Society of Indiaen
dc.rights(2001) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System.en
dc.subjectGamma Ray Bursten
dc.subjectRadiation Mechanismen
dc.titleFlat spectrum gamma ray burst afterglowsen
Appears in Collections:Research Papers (A&A)

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