Emergent universe revisited through the CSL theory
Abstract In this work we analyze how the spectrum of primordial scalar perturbations is modified, within the emergent universe scenario, when a particular version of the Continuous Spontaneous Localization (CSL) model is incorporated as the generating mechanism of initial perturbations, providing al...
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2021
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oai:doaj.org-article:636fed59119044e08181afb88056806d2021-12-05T12:09:18ZEmergent universe revisited through the CSL theory10.1140/epjc/s10052-021-09842-x1434-60441434-6052https://doaj.org/article/636fed59119044e08181afb88056806d2021-12-01T00:00:00Zhttps://doi.org/10.1140/epjc/s10052-021-09842-xhttps://doaj.org/toc/1434-6044https://doaj.org/toc/1434-6052Abstract In this work we analyze how the spectrum of primordial scalar perturbations is modified, within the emergent universe scenario, when a particular version of the Continuous Spontaneous Localization (CSL) model is incorporated as the generating mechanism of initial perturbations, providing also an explanation to the quantum-to-classical transition of such perturbations. On the other hand, a phase of super-inflation, prior to slow-roll inflation, is a characteristic feature of the emergent universe hypothesis. In recent works, it was shown that the super-inflation phase could generically induce a suppression of the temperature anisotropies of the CMB at large angular scales. We study here under what conditions the CSL maintains or modifies these characteristics of the emergent universe and their compatibility with the CMB observations.Gabriel R. BengocheaMaría Pía PiccirilliGabriel LeónSpringerOpenarticleAstrophysicsQB460-466Nuclear and particle physics. Atomic energy. RadioactivityQC770-798ENEuropean Physical Journal C: Particles and Fields, Vol 81, Iss 12, Pp 1-16 (2021) |
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Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 |
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Astrophysics QB460-466 Nuclear and particle physics. Atomic energy. Radioactivity QC770-798 Gabriel R. Bengochea María Pía Piccirilli Gabriel León Emergent universe revisited through the CSL theory |
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Abstract In this work we analyze how the spectrum of primordial scalar perturbations is modified, within the emergent universe scenario, when a particular version of the Continuous Spontaneous Localization (CSL) model is incorporated as the generating mechanism of initial perturbations, providing also an explanation to the quantum-to-classical transition of such perturbations. On the other hand, a phase of super-inflation, prior to slow-roll inflation, is a characteristic feature of the emergent universe hypothesis. In recent works, it was shown that the super-inflation phase could generically induce a suppression of the temperature anisotropies of the CMB at large angular scales. We study here under what conditions the CSL maintains or modifies these characteristics of the emergent universe and their compatibility with the CMB observations. |
format |
article |
author |
Gabriel R. Bengochea María Pía Piccirilli Gabriel León |
author_facet |
Gabriel R. Bengochea María Pía Piccirilli Gabriel León |
author_sort |
Gabriel R. Bengochea |
title |
Emergent universe revisited through the CSL theory |
title_short |
Emergent universe revisited through the CSL theory |
title_full |
Emergent universe revisited through the CSL theory |
title_fullStr |
Emergent universe revisited through the CSL theory |
title_full_unstemmed |
Emergent universe revisited through the CSL theory |
title_sort |
emergent universe revisited through the csl theory |
publisher |
SpringerOpen |
publishDate |
2021 |
url |
https://doaj.org/article/636fed59119044e08181afb88056806d |
work_keys_str_mv |
AT gabrielrbengochea emergentuniverserevisitedthroughthecsltheory AT mariapiapiccirilli emergentuniverserevisitedthroughthecsltheory AT gabrielleon emergentuniverserevisitedthroughthecsltheory |
_version_ |
1718372195127787520 |