Spherical Fallback Accretion -the Engine GRB 050502B
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Date
2016-09
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Addis Ababa University
Abstract
Gamma ray bursts are energetic and most luminous objects in the universe. They emit
the most energetic form of electromagnetic radiation with extremely short wavelength and
high frequencies. The gamma ray burst which is detected by swift Burst Alert Telescope
(BAT) with giant and bright
are is GRB 050502B with the energy band (0.3 - 10.0 keV).
In this thesis we have tried to theoretically reconstruct the X-ray after-glow from GRB
050502B as observed by NASA`s Swift satellite based on current GRB model
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Spherical Fallback Accretion