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

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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Physical Review D, American Physical Society, 2017, 95 (8), pp.083507. 〈10.1103/PhysRevD.95.083507〉
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Contributeur : Emmanuelle Vernay <>
Soumis le : mardi 11 avril 2017 - 08:34:42
Dernière modification le : mardi 22 mai 2018 - 21:48:11

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K. Martineau, A. Barrau, S. Schander. Detailed investigation of the duration of inflation in loop quantum cosmology for a Bianchi-I universe with different inflaton potentials and initial conditions. Physical Review D, American Physical Society, 2017, 95 (8), pp.083507. 〈10.1103/PhysRevD.95.083507〉. 〈in2p3-01505077〉

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