GRB prompt high-energy emission from internal shocks:a time-dependent model
We compute the GRB prompt high energy gamma-ray emission in the framework of the internal shock scenario.Our numerical model combines a code developed to follow the dynamics of the internal shocks phase with a code calculatingthe high-energy radiative processes.We discuss the resulting synthetic light curves and spectra.
Gamma-ray bursts-gammarays theory-radiation mechanisms nonthermal
Zeljka Bosnjak Frederic Daigne Guillatume Dubus
Institut dAstrophysique de Paris,UMR 7095 CNRS,Universite Pierre&Marie Curie-Paris 6,98bis boulevar Institut dAstrophysique de Paris,UMR 7095 CNRS,Universite Pierre&Marie Curie-Paris 6,98bis boulevar Laboratoire dAstrophysique de Grenoble,UMR 5571 CNRS,Universite J.Fourier,8P 53,38041 Grenoble,Fran
国际会议
2008 NanJing Gamma-Ray Burst Conference(2008年伽马暴国际研讨会)
南京
英文
207-210
2008-06-23(万方平台首次上网日期,不代表论文的发表时间)