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Please use this identifier to cite or link to this item: http://hdl.handle.net/2289/1346

Title: Flat spectrum gamma ray burst afterglows
Authors: Bhattacharya, D.
Keywords: Gamma Ray Burst
Afterglow
Radiation Mechanism
Theory
Issue Date: Jun-2001
Publisher: The Astronomical Society of India
Citation: Bulletin of the Astronomical Society of India, 2001, Vol.29, p107-114
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.
URI: http://hdl.handle.net/2289/1346
ISSN: 0304-9523
Alternative Location: http://adsabs.harvard.edu/cgi-bin/bib_query?2001BASI...29..107B
Copyright: (2001) by the Astronomical Society of India. Scanned images provided by the NASA ADS Data System.
Appears in Collections:Research Papers (A&A)

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