New ekpyrotic quantum cosmology

Ekpyrotic instantons describe the emergence of classical contracting universes out of the no-boundary quantum state. However, up to now these instantons ended in a big crunch singularity. We remedy this by adding a higher-derivative term, allowing a ghost condensate to form. This causes a smooth, no...

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Main Author: Jean-Luc Lehners
Format: Article
Language:English
Published: Elsevier 2015-11-01
Series:Physics Letters B
Online Access:http://www.sciencedirect.com/science/article/pii/S0370269315007078
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author Jean-Luc Lehners
author_facet Jean-Luc Lehners
author_sort Jean-Luc Lehners
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description Ekpyrotic instantons describe the emergence of classical contracting universes out of the no-boundary quantum state. However, up to now these instantons ended in a big crunch singularity. We remedy this by adding a higher-derivative term, allowing a ghost condensate to form. This causes a smooth, non-singular bounce from the contracting phase into an expanding, kinetic-dominated phase. Remarkably, and although there is a non-trivial evolution during the bounce, the wavefunction of the universe is “classical” in a WKB sense just as much after the bounce as before. These new non-singular instantons can thus form the basis for a fully non-singular and calculable ekpyrotic history of the universe, from creation until now.
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spelling doaj.art-5a5825e659c347a3a2c585f34445013f2022-12-22T03:21:32ZengElsevierPhysics Letters B0370-26931873-24452015-11-01750C24224610.1016/j.physletb.2015.09.032New ekpyrotic quantum cosmologyJean-Luc LehnersEkpyrotic instantons describe the emergence of classical contracting universes out of the no-boundary quantum state. However, up to now these instantons ended in a big crunch singularity. We remedy this by adding a higher-derivative term, allowing a ghost condensate to form. This causes a smooth, non-singular bounce from the contracting phase into an expanding, kinetic-dominated phase. Remarkably, and although there is a non-trivial evolution during the bounce, the wavefunction of the universe is “classical” in a WKB sense just as much after the bounce as before. These new non-singular instantons can thus form the basis for a fully non-singular and calculable ekpyrotic history of the universe, from creation until now.http://www.sciencedirect.com/science/article/pii/S0370269315007078
spellingShingle Jean-Luc Lehners
New ekpyrotic quantum cosmology
Physics Letters B
title New ekpyrotic quantum cosmology
title_full New ekpyrotic quantum cosmology
title_fullStr New ekpyrotic quantum cosmology
title_full_unstemmed New ekpyrotic quantum cosmology
title_short New ekpyrotic quantum cosmology
title_sort new ekpyrotic quantum cosmology
url http://www.sciencedirect.com/science/article/pii/S0370269315007078
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