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Relaxing the TCC bound on inflationary cosmology?
We demonstrate that the strict upper bounds on the energy scale of inflation and on the tensor-to-scalar ratio can be somewhat relaxed if we assume that – after an initial period of slow rolling when scales probed today in CMB experiments exit the Hubble radius – the equation of state of the backgro...
Autores principales: | , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
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Springer Berlin Heidelberg
2020
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7319298/ https://www.ncbi.nlm.nih.gov/pubmed/32624682 http://dx.doi.org/10.1140/epjc/s10052-020-7908-8 |
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author | Kamali, Vahid Brandenberger, Robert |
author_facet | Kamali, Vahid Brandenberger, Robert |
author_sort | Kamali, Vahid |
collection | PubMed |
description | We demonstrate that the strict upper bounds on the energy scale of inflation and on the tensor-to-scalar ratio can be somewhat relaxed if we assume that – after an initial period of slow rolling when scales probed today in CMB experiments exit the Hubble radius – the equation of state of the background changes to correspond to an almost marginally accelerating universe. Constructing an actual model in which this happens appears, however, to be unnatural. |
format | Online Article Text |
id | pubmed-7319298 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2020 |
publisher | Springer Berlin Heidelberg |
record_format | MEDLINE/PubMed |
spelling | pubmed-73192982020-07-01 Relaxing the TCC bound on inflationary cosmology? Kamali, Vahid Brandenberger, Robert Eur Phys J C Part Fields Letter We demonstrate that the strict upper bounds on the energy scale of inflation and on the tensor-to-scalar ratio can be somewhat relaxed if we assume that – after an initial period of slow rolling when scales probed today in CMB experiments exit the Hubble radius – the equation of state of the background changes to correspond to an almost marginally accelerating universe. Constructing an actual model in which this happens appears, however, to be unnatural. Springer Berlin Heidelberg 2020-04-25 2020 /pmc/articles/PMC7319298/ /pubmed/32624682 http://dx.doi.org/10.1140/epjc/s10052-020-7908-8 Text en © The Author(s) 2020 Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/. Funded by SCOAP3 |
spellingShingle | Letter Kamali, Vahid Brandenberger, Robert Relaxing the TCC bound on inflationary cosmology? |
title | Relaxing the TCC bound on inflationary cosmology? |
title_full | Relaxing the TCC bound on inflationary cosmology? |
title_fullStr | Relaxing the TCC bound on inflationary cosmology? |
title_full_unstemmed | Relaxing the TCC bound on inflationary cosmology? |
title_short | Relaxing the TCC bound on inflationary cosmology? |
title_sort | relaxing the tcc bound on inflationary cosmology? |
topic | Letter |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7319298/ https://www.ncbi.nlm.nih.gov/pubmed/32624682 http://dx.doi.org/10.1140/epjc/s10052-020-7908-8 |
work_keys_str_mv | AT kamalivahid relaxingthetccboundoninflationarycosmology AT brandenbergerrobert relaxingthetccboundoninflationarycosmology |