SISSA Open Science

On the Onset of Inflation in Loop Quantum Cosmology

Show simple item record Germani, Cristiano en_US Nelson, William en_US Sakellariadou, Mairi en_US 2007-02-02T09:12:35Z en_US 2011-09-07T20:27:03Z 2007-02-02T09:12:35Z en_US 2011-09-07T20:27:03Z 2007-02-02T09:12:35Z en_US
dc.identifier.citation Phys. Rev. D 76 (2007) 043529 en_US
dc.identifier.uri en_US
dc.description.abstract Using a Liouville measure, similar to the one proposed recently by Gibbons and Turok, we investigate the probability that single-field inflation with a polynomial potential can last long enough to solve the shortcomings of the standard hot big bang model, within the semiclassical regime of loop quantum cosmology. We conclude that, for such a class of inflationary models and for natural values of the loop quantum cosmology parameters, a successful inflationary scenario is highly improbable. en_US
dc.format.extent 281772 bytes en_US
dc.format.mimetype application/pdf en_US
dc.language.iso en_US en_US
dc.relation.ispartofseries SISSA;85/2006/EP en_US
dc.relation.ispartofseries;gr-qc/0701172 en_US
dc.relation.uri 10.1103/PhysRevD.76.043529 en_US
dc.title On the Onset of Inflation in Loop Quantum Cosmology en_US
dc.title.alternative Onset of inflation in loop quantum cosmology en_US
dc.type Preprint en_US
dc.contributor.department Elementary Particle Theory en_US
dc.contributor.area Physics en_US

Files in this item

This item appears in the following Collection(s)

Show simple item record

Search SISSA Open Science


My Account