Abstract
In the timing study, we report the results of extensive analysis of the Long Dark Gamma Ray Bur sts 130528A at various differential Energy range of Soft (low) and Hard (high) bands starting from 5 keV to 100 keV in the steps of 5, which is exhibited by complete sequential merger of two galaxies: halos of galaxies, corona of stars and hot gases in the giant stars. We observed three distinct bursts in the light curve in differential energy range. The results showed the loss of mass on an average 7.5 1019 kg of the system in the form of radiation during the occurrence of dGRB 130528A. This can be attri buting to the mechanism described in a model for the origin of the dGRBs in the space.
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