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The influence of inverse Compton scattering on GRB afterglows: one possible way to flatten and steepen the light curves
Wei, DM; Lu, T
2000-08-10
Source PublicationASTRONOMY & ASTROPHYSICS
Volume360Issue:2Pages:L13-L16
AbstractThe fireball model of gamma-ray bursts predicted that when the energetic blast wave encountered the surrounding medium, there will be afterglow emission, and the subsequent afterglow observations appeared to confirm this prediction. In this simplest fireball model, the electrons have been accelerated to a power law energy distribution in a relativistic blast wave, then they give afterglow emission through synchrotron radiation. Up to now synchrotron radiation is believed to be the main mechanism of GRB emission, however, here we will show that under some circumstances, the inverse Compton scattering (ICS) may play an important role, and can change the light curves of GRB afterglows. Here we investigate the effects of ICS in the relativistic case (the surrounding medium density rho proportional to r(-2)) and in the non-relativistic case (for both rho = constant and rho proportional to r(-2)). We find that in the relativistic case the effect of ICS is usually important, while in the non-relativistic case, this effect is usually unimportant, unless the surrounding medium density is very high. We show that if ICS is important, then it can flatten and steepen the light curves of GRB afterglows, and this may provide the explanation for some afterglow observations.
KeywordGamma Rays : Bursts Shock Waves Ism : Jets And Outflows
Subject AreaAstronomy & Astrophysics
WOS HeadingsScience & Technology ; Physical Sciences
WOS KeywordGAMMA-RAY-BURST ; COSMOLOGICAL FIREBALL MODEL ; 23 JANUARY 1999 ; GRB-990123 ; EVOLUTION ; REMNANTS
Indexed BySCI
Language英语
WOS Research AreaAstronomy & Astrophysics
WOS SubjectAstronomy & Astrophysics
WOS IDWOS:000089331400002
Citation statistics
Cited Times:27[WOS]   [WOS Record]     [Related Records in WOS]
Document Type期刊论文
Identifierhttp://libir.pmo.ac.cn/handle/332002/11106
Collection院士文集_陆埮
Affiliation1.Purple Mt Observ, Chinese Acad Sci, Nanjing, Peoples R China
2.Nanjing Univ, Dept Astron, Nanjing 210093, Peoples R China
3.Chinese Acad Sci, Inst High Energy Phys, Lab Cosm Ray & High Energy Astrophys, Beijing 100039, Peoples R China
Recommended Citation
GB/T 7714
Wei, DM,Lu, T. The influence of inverse Compton scattering on GRB afterglows: one possible way to flatten and steepen the light curves[J]. ASTRONOMY & ASTROPHYSICS,2000,360(2):L13-L16.
APA Wei, DM,&Lu, T.(2000).The influence of inverse Compton scattering on GRB afterglows: one possible way to flatten and steepen the light curves.ASTRONOMY & ASTROPHYSICS,360(2),L13-L16.
MLA Wei, DM,et al."The influence of inverse Compton scattering on GRB afterglows: one possible way to flatten and steepen the light curves".ASTRONOMY & ASTROPHYSICS 360.2(2000):L13-L16.
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