Abstract
We consider the cosine Natural inflation model that is a good candidate to explain the initial accelerating phase of the universe. By computing the inflationary parameters in Einstein frame, we construct a consistency relation between the scalar spectral index, tensor-to-scalar ratio, as well as the running of the scalar spectral index and compare the results with recently released Planck 2015 observational data. Our results show that a Natural Inflation model in Einstein frame has a good agreement with the observational data.
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Nozari, K., Kahvaee, H. & Rashidi, N. Consistency relation for natural inflation with Planck 2015 data. Astrophys Space Sci 359, 63 (2015). https://doi.org/10.1007/s10509-015-2514-1
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DOI: https://doi.org/10.1007/s10509-015-2514-1