Will quantum cosmology resurrect chaotic inflation model?

Sang Pyo Kim; Won Kim (Kunsan Natl U.)

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Will quantum cosmology resurrect chaotic inflation model?

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arxiv 1603.08087 v1 pith:URXGJCXC submitted 2016-03-26 gr-qc

Sang Pyo Kim , Won Kim (Kunsan Natl U.) This is my paper

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keywords modelquantumcosmologychaoticinflationcurvaturefluctuationshigher

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The single field chaotic inflation model with a monomial power greater than one seems to be ruled out by the recent Planck and WMAP CMB data while Starobinsky model with a higher curvature term seems to be a viable model. Higher curvature terms being originated from quantum fluctuations, we revisit the quantum cosmology of the Wheeler-DeWitt equation for the chaotic inflation model. The semiclassical cosmology emerges from quantum cosmology with fluctuations of spacetimes and matter when the wave function is peaked around the semiclassical trajectory with quantum corrections a la the de Broglie-Bohm pilot theory.

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