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arXiv · 1202.0698

Low power on large scales in just enough inflation models

Erandy Ramirez
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Abstract

An early stage of kinetic energy domination for inflation is applied to single-field quadratic and hybrid-type potentials considering only the amount of inflation necessary to solve the problems of the standard cosmological scenario. Using initial conditions inside the 1-sigma interval of the best-fit cosmological parameters for the potentials, low values for the quadrupole component can be obtained.

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Erandy Ramirez. 2012-02-03. Low power on large scales in just enough inflation models. https://doi.org/10.1103/physrevd.85.103517

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