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Chinese Physics, 2005, Vol. 14(11): 2276-2286    DOI: 10.1088/1009-1963/14/11/023
CONDENSED MATTER: STRUCTURAL, MECHANICAL, AND THERMAL PROPERTIES Prev   Next  

Relationship between width of pulses and Lorentz factor expected from the light curve of fireball sources

Zhang Fu-Wen (张富文)abc, Qin Yi-Ping (覃一平)ab 
a National Astronomical Observatories/Yunnan Observatory, Chinese Academy of Sciences, Kunming 650011, Chinab Physics Department, Guangxi University, Nanning 530004, China; c Graduate School of The Chinese Academy of Sciences, Beijing 100049, China
Abstract  Time profiles of many gamma-ray bursts consist of distinct pulses, which provides a possibility of characterizing the temporal structure of these bursts. We employ a simple model of highly symmetric fireballs to analyse the effect of the expansion speed on the light curve arising from different forms of local pulses. The relationship between the ratio r of the FWHM width of the rising phase of the light curve to that of the decaying phase and the Lorentz factor is investigated. The analysis shows that, when the rest frame radiation form is ignored, temporal profiles of the light curve arising from pulses of fireballs will not be affected by the expansion speed (that is, r is almost a constant) as long as the fireball expands relativistically. When the rest frame radiation form is taken into account, there will be a break in the curves of r$-$log$\varGamma$. The location of the break depends mainly on the adopted value of the rest frame peak frequency $\nu _{\rm 0,p}$. One would reach almost the same result when a jet is considered. In addition, we utilize a sample of 48 individual GRB pulses to check the relationship between the ratio r and the expansion speed $\varGamma$. We find no significant correlation between them, and this is consistent with the theoretical analysis.
Keywords:  gamma-ray bursts      gamma-rays      relativity  
Received:  23 December 2004      Revised:  31 January 2005      Accepted manuscript online: 
PACS:  98.70.Rz (γ-ray sources; γ-ray bursts)  
  95.30.Sf (Relativity and gravitation)  
Fund: Project partly supported by the Special Funds for Major State Basic Research Projects (973 Program) and the National Natural Science Foundation of China (Grant No 10273019).

Cite this article: 

Zhang Fu-Wen (张富文), Qin Yi-Ping (覃一平) Relationship between width of pulses and Lorentz factor expected from the light curve of fireball sources 2005 Chinese Physics 14 2276

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