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We show that S-dual inflationary potentials solve the unlikeliness problem manifested in Planck data and explain the excess B-mode power observed by the BICEP2 experiment as arising from primordial tensor fluctuations.
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H. Liu, P. Mertsch and S. Sarkar, arXiv:1404.1899 [astro-ph.CO]
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We note that inflationary potentials can be characterized by a scale M > M Pl M>M_{\rm Pl} provided the energy density ≪ M Pl 4 \ll M_{\rm Pl}^{4}
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A. Ijjas, P. J. Steinhardt and A. Loeb, Phys. Lett. B 723
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