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Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations
We point out a weak side of the commonly used determination of scalar cosmological perturbations lying in the fact that their average values can be nonzero for some matter distributions. It is shown that introduction of the finite-range gravitational potential instead of the infinite-range one resol...
Autores principales: | , , |
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Formato: | Online Artículo Texto |
Lenguaje: | English |
Publicado: |
Springer Berlin Heidelberg
2015
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Materias: | |
Acceso en línea: | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4547628/ https://www.ncbi.nlm.nih.gov/pubmed/26321878 http://dx.doi.org/10.1140/epjc/s10052-015-3598-z |
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author | Eingorn, Maxim Brilenkov, Maxim Vlahovic, Branislav |
author_facet | Eingorn, Maxim Brilenkov, Maxim Vlahovic, Branislav |
author_sort | Eingorn, Maxim |
collection | PubMed |
description | We point out a weak side of the commonly used determination of scalar cosmological perturbations lying in the fact that their average values can be nonzero for some matter distributions. It is shown that introduction of the finite-range gravitational potential instead of the infinite-range one resolves this problem. The concrete illustrative density profile is investigated in detail in this connection. |
format | Online Article Text |
id | pubmed-4547628 |
institution | National Center for Biotechnology Information |
language | English |
publishDate | 2015 |
publisher | Springer Berlin Heidelberg |
record_format | MEDLINE/PubMed |
spelling | pubmed-45476282015-08-26 Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations Eingorn, Maxim Brilenkov, Maxim Vlahovic, Branislav Eur Phys J C Part Fields Regular Article - Theoretical Physics We point out a weak side of the commonly used determination of scalar cosmological perturbations lying in the fact that their average values can be nonzero for some matter distributions. It is shown that introduction of the finite-range gravitational potential instead of the infinite-range one resolves this problem. The concrete illustrative density profile is investigated in detail in this connection. Springer Berlin Heidelberg 2015-08-22 2015 /pmc/articles/PMC4547628/ /pubmed/26321878 http://dx.doi.org/10.1140/epjc/s10052-015-3598-z Text en © The Author(s) 2015 Open AccessThis article is distributed under the terms of the Creative Commons Attribution 4.0 International License (http://creativecommons.org/licenses/by/4.0/), which permits unrestricted use, distribution, and reproduction in any medium, provided you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons license, and indicate if changes were made. Funded by SCOAP3. |
spellingShingle | Regular Article - Theoretical Physics Eingorn, Maxim Brilenkov, Maxim Vlahovic, Branislav Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations |
title | Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations |
title_full | Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations |
title_fullStr | Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations |
title_full_unstemmed | Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations |
title_short | Zero average values of cosmological perturbations as an indispensable condition for the theory and simulations |
title_sort | zero average values of cosmological perturbations as an indispensable condition for the theory and simulations |
topic | Regular Article - Theoretical Physics |
url | https://www.ncbi.nlm.nih.gov/pmc/articles/PMC4547628/ https://www.ncbi.nlm.nih.gov/pubmed/26321878 http://dx.doi.org/10.1140/epjc/s10052-015-3598-z |
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