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Title: Onset of inflation in loop quantum cosmology

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.

Authors:
; ;  [1]
  1. SISSA and INFN, via Beirut 4, 34014 Trieste (Italy)
Publication Date:
OSTI Identifier:
21027594
Resource Type:
Journal Article
Journal Name:
Physical Review. D, Particles Fields
Additional Journal Information:
Journal Volume: 76; Journal Issue: 4; Other Information: DOI: 10.1103/PhysRevD.76.043529; (c) 2007 The American Physical Society; Country of input: International Atomic Energy Agency (IAEA); Journal ID: ISSN 0556-2821
Country of Publication:
United States
Language:
English
Subject:
72 PHYSICS OF ELEMENTARY PARTICLES AND FIELDS; COSMOLOGY; INFLATIONARY UNIVERSE; POLYNOMIALS; POTENTIALS; PROBABILITY; QUANTUM FIELD THEORY; SEMICLASSICAL APPROXIMATION

Citation Formats

Germani, Cristiano, Nelson, William, Sakellariadou, Mairi, and Department of Physics, King's College London, London WC2R 2LS. Onset of inflation in loop quantum cosmology. United States: N. p., 2007. Web. doi:10.1103/PHYSREVD.76.043529.
Germani, Cristiano, Nelson, William, Sakellariadou, Mairi, & Department of Physics, King's College London, London WC2R 2LS. Onset of inflation in loop quantum cosmology. United States. https://doi.org/10.1103/PHYSREVD.76.043529
Germani, Cristiano, Nelson, William, Sakellariadou, Mairi, and Department of Physics, King's College London, London WC2R 2LS. 2007. "Onset of inflation in loop quantum cosmology". United States. https://doi.org/10.1103/PHYSREVD.76.043529.
@article{osti_21027594,
title = {Onset of inflation in loop quantum cosmology},
author = {Germani, Cristiano and Nelson, William and Sakellariadou, Mairi and Department of Physics, King's College London, London WC2R 2LS},
abstractNote = {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.},
doi = {10.1103/PHYSREVD.76.043529},
url = {https://www.osti.gov/biblio/21027594}, journal = {Physical Review. D, Particles Fields},
issn = {0556-2821},
number = 4,
volume = 76,
place = {United States},
year = {Wed Aug 15 00:00:00 EDT 2007},
month = {Wed Aug 15 00:00:00 EDT 2007}
}