Eternal inflation and the quantum birth of cosmic structure

Abstract We consider the eternal inflation scenario of the slow-roll/chaotic type with the additional element of an objective collapse of the wave function. The incorporation of this new agent to the traditional inflationary setting might represent a possible solution to the quantum measurement prob...

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Main Author: Gabriel León
Format: Article
Language:English
Published: SpringerOpen 2017-10-01
Series:European Physical Journal C: Particles and Fields
Online Access:http://link.springer.com/article/10.1140/epjc/s10052-017-5288-5
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spelling doaj-c40bab8904d043e3807cdbc5961108d82020-11-25T02:00:07ZengSpringerOpenEuropean Physical Journal C: Particles and Fields1434-60441434-60522017-10-01771011410.1140/epjc/s10052-017-5288-5Eternal inflation and the quantum birth of cosmic structureGabriel León0Grupo de Astrofísica, Relatividad y Cosmología, Facultad de Ciencias Astronómicas y Geofísicas, Universidad Nacional de La PlataAbstract We consider the eternal inflation scenario of the slow-roll/chaotic type with the additional element of an objective collapse of the wave function. The incorporation of this new agent to the traditional inflationary setting might represent a possible solution to the quantum measurement problem during inflation, a subject that has not reached a consensus among the community. Specifically, it could provide an explanation for the generation of the primordial anisotropies and inhomogeneities, starting from a perfectly symmetric background and invoking symmetric dynamics. We adopt the continuous spontaneous localization model, in the context of inflation, as the dynamical reduction mechanism that generates the primordial inhomogeneities. Furthermore, when enforcing the objective reduction mechanism, the condition for eternal inflation can be bypassed. In particular, the collapse mechanism incites the wave function, corresponding to the inflaton, to localize itself around the zero mode of the field. Then the zero mode will evolve essentially unperturbed, driving inflation to an end in any region of the Universe where inflation occurred. Also, our approach achieves a primordial spectrum with an amplitude and shape consistent with the one that best fits the observational data.http://link.springer.com/article/10.1140/epjc/s10052-017-5288-5
collection DOAJ
language English
format Article
sources DOAJ
author Gabriel León
spellingShingle Gabriel León
Eternal inflation and the quantum birth of cosmic structure
European Physical Journal C: Particles and Fields
author_facet Gabriel León
author_sort Gabriel León
title Eternal inflation and the quantum birth of cosmic structure
title_short Eternal inflation and the quantum birth of cosmic structure
title_full Eternal inflation and the quantum birth of cosmic structure
title_fullStr Eternal inflation and the quantum birth of cosmic structure
title_full_unstemmed Eternal inflation and the quantum birth of cosmic structure
title_sort eternal inflation and the quantum birth of cosmic structure
publisher SpringerOpen
series European Physical Journal C: Particles and Fields
issn 1434-6044
1434-6052
publishDate 2017-10-01
description Abstract We consider the eternal inflation scenario of the slow-roll/chaotic type with the additional element of an objective collapse of the wave function. The incorporation of this new agent to the traditional inflationary setting might represent a possible solution to the quantum measurement problem during inflation, a subject that has not reached a consensus among the community. Specifically, it could provide an explanation for the generation of the primordial anisotropies and inhomogeneities, starting from a perfectly symmetric background and invoking symmetric dynamics. We adopt the continuous spontaneous localization model, in the context of inflation, as the dynamical reduction mechanism that generates the primordial inhomogeneities. Furthermore, when enforcing the objective reduction mechanism, the condition for eternal inflation can be bypassed. In particular, the collapse mechanism incites the wave function, corresponding to the inflaton, to localize itself around the zero mode of the field. Then the zero mode will evolve essentially unperturbed, driving inflation to an end in any region of the Universe where inflation occurred. Also, our approach achieves a primordial spectrum with an amplitude and shape consistent with the one that best fits the observational data.
url http://link.springer.com/article/10.1140/epjc/s10052-017-5288-5
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