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In this paper, we focus on general features of quintessential inflation whichis an effort to unify inflation and dark energy using a single scalar field. Wedescribe a class of models of quintessential inflation which can give rise tothe tensor to scalar ratio of perturbations consistent with recent BICEP2measurements. The scale of inflation in the model is around the GUT scale andthere is large parameter space consistent with the recent findings.

A class of quintessential inflation models with parameter space consistent with BICEP2