Abstract
This paper discusses the form of energy called the brane tension λ that can effect in the reheating phase after inflation. In this regard, we study an inflationary model with a tree level potential in the framework of braneworld Randall-Sundrum type II model to investigate the reheating epoch. We have computed and discussed the reheating temperature of the universe following inflation for several choices parameters of the scalar potential parameters. And we have found that the reheating temperature an upper limit that lies in the range 109–1010 GeV.
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