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

K. Martineau 1 A. Barrau 1 S. Schander
1 LPSC - Laboratoire de Physique Subatomique et de Cosmologie
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.
Type de document :
Article dans une revue
Physical Review D, American Physical Society, 2017, 95 (8), pp.083507. 〈10.1103/PhysRevD.95.083507〉
Liste complète des métadonnées
http://hal.in2p3.fr/in2p3-01505077
Contributeur : Emmanuelle Vernay <>
Soumis le : mardi 11 avril 2017 - 08:34:42
Dernière modification le : mardi 22 mai 2018 - 21:48:11

Lien texte intégral

arxiv

Identifiants

Collections

IN2P3 | LPSC | UGA

Citation

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〉

Exporter

BibTeX TEI DC DCterms EndNote

Partager

Métriques

Consultations de la notice

232

Contact

support.ccsd.cnrs.fr
hal.support@ccsd.cnrs.fr
Logo CCSD