Abstract

We show that quantum-induced marginal deformations of the Starobinsky gravitational action of the form R2(1−α)R^{2(1 -α)}, with RR the Ricci scalar and αα a positive parameter, smaller than one half, can account for the recent experimental observations by BICEP2 of primordial tensor modes. We also suggest natural microscopic (non) gravitational sources of these corrections and demonstrate that they lead generally to a nonzero and positive αα. Furthermore we argue, that within this framework, the tensor modes probe theories of grand unification with a large scalar field content.

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