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arXiv · 1701.02703

Detailed investigation of the duration of inflation in loop quantum cosmology for a Bianchi-I universe with different inflaton potentials and initial conditions

Killian Martineau·Aurélien Barrau·Susanne Schander
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Abstract

There is a wide consensus on the correct dynamics of the background in loop quantum cosmology. In this article we make a systematic investigation of the duration of inflation by varying what we think to be the most important "unknowns" of the model: the way to set initial conditions, the amount of shear at the bounce and the shape of the inflaton potential.

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Killian Martineau, Aurélien Barrau, Susanne Schander. 2017-01-10. Detailed investigation of the duration of inflation in loop quantum cosmology for a Bianchi-I universe with different inflaton potentials and initial conditions. https://doi.org/10.1103/physrevd.95.083507

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