On the Onset of Inflation in Loop Quantum Cosmology

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dc.contributor.areaPhysicsen_US
dc.contributor.authorGermani, Cristianoen_US
dc.contributor.authorNelson, Williamen_US
dc.contributor.authorSakellariadou, Mairien_US
dc.contributor.departmentElementary Particle Theoryen_US
dc.date.accessioned2007-02-02T09:12:35Zen_US
dc.date.accessioned2011-09-07T20:27:03Z
dc.date.available2007-02-02T09:12:35Zen_US
dc.date.available2011-09-07T20:27:03Z
dc.date.issued2007-02-02T09:12:35Zen_US
dc.description.abstractUsing 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.extent281772 bytesen_US
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationPhys. Rev. D 76 (2007) 043529en_US
dc.identifier.urihttps://openscience.sissa.it/handle/1963/1911en_US
dc.language.isoen_USen_US
dc.relation.ispartofseriesSISSA;85/2006/EPen_US
dc.relation.ispartofseriesarXiv.org;gr-qc/0701172en_US
dc.relation.uri10.1103/PhysRevD.76.043529en_US
dc.titleOn the Onset of Inflation in Loop Quantum Cosmologyen_US
dc.title.alternativeOnset of inflation in loop quantum cosmologyen_US
dc.typePreprinten_US
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