Flat Spectrum Gamma Ray Burst Afterglows

dc.contributor.author	Bhattacharya, D
dc.date.accessioned	2008-04-11T12:10:47Z
dc.date.available	2008-04-11T12:10:47Z
dc.date.issued	2001
dc.identifier.citation	BASI, Vol. 29, No. 2, pp. 107 - 114	en
dc.identifier.uri	http://hdl.handle.net/2248/2223
dc.description.abstract	Temporal 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.extent	619098 bytes
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Astronomical Society of India	en
dc.relation.uri	http://adsabs.harvard.edu/abs/2001BASI...29..107B	en
dc.subject	Gamma Ray Bursts	en
dc.subject	Afterglow	en
dc.subject	Radiation mechanism	en
dc.subject	Theory	en
dc.title	Flat Spectrum Gamma Ray Burst Afterglows	en
dc.type	Article	en