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Influence of the pulsar parameters on γ-ray burst afterglows
Authors:Xu Yun  Yang Pi-bo  Wu Shao-ping  Zheng Xiao-ping
Institution:

a Department of Physics, Hua Zhong Normal University, Wuhan 430079, China

b Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 20030, China

Abstract:By applying the fireball model of γ-ray burst with a central pulsar, the radiation fluxes of the afterglows of two γ-ray bursts, GRB970228 and GRB000301c, are calculated. The results of the calculation agree very well with the observations. The differing characters of the light curves with a “break” in the optical waveband R of the afterglows of two bursts are interpreted, in terms of differing pulsar parameter values.
Keywords:γ-ray  burst—γ-ray  observation—γ-ray  theory
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