Flat Spectrum Gamma Ray Burst Afterglows

Details Flat Spectrum Gamma Ray Burst Afterglows Flat Spectrum Gamma Ray Burst Afterglows

2001-04-15

arxiv.org/abs/astro-ph/0104250v2

Bull. Astr. Soc. India, vol. 29, pp. 107-114 (2001)

Astronomy and Astrophysics

Astrophysics

8 pages, uses basi.sty (included). Revised according to referees' comments. Added discussion on Dai & Cheng (2001) astro-ph/01

Scientific paper

Temporal behaviour of GRB afterglow light curve is derived for the case where
the electron energy distribution is relatively flat, 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.

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