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...
Main Author: | |
---|---|
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 |
id |
doaj-c40bab8904d043e3807cdbc5961108d8 |
---|---|
record_format |
Article |
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 |
work_keys_str_mv |
AT gabrielleon eternalinflationandthequantumbirthofcosmicstructure |
_version_ |
1724962471592067072 |