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Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures
We present an analytical fit to the growth function of the dark matter perturbations when dark energy perturbations are present. The growth index depends upon the dark energy equation of state w, the speed of sound of the dark energy fluctuations, the dark matter abundance and the observed comoving...
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Lenguaje: | eng |
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2008
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Acceso en línea: | https://dx.doi.org/10.1016/j.physletb.2008.08.035 http://cds.cern.ch/record/1116651 |
_version_ | 1780914428567355392 |
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author | Ballesteros, Guillermo Riotto, Antonio |
author_facet | Ballesteros, Guillermo Riotto, Antonio |
author_sort | Ballesteros, Guillermo |
collection | CERN |
description | We present an analytical fit to the growth function of the dark matter perturbations when dark energy perturbations are present. The growth index depends upon the dark energy equation of state w, the speed of sound of the dark energy fluctuations, the dark matter abundance and the observed comoving scale. The growth index changes by ~5% for small speed of sound and large deviations of w from -1 with respect to its value in the limit of no dark energy perturbations. |
id | cern-1116651 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2008 |
record_format | invenio |
spelling | cern-11166512023-03-15T19:11:22Zdoi:10.1016/j.physletb.2008.08.035http://cds.cern.ch/record/1116651engBallesteros, GuillermoRiotto, AntonioParameterizing the Effect of Dark Energy Perturbations on the Growth of StructuresAstrophysics and AstronomyWe present an analytical fit to the growth function of the dark matter perturbations when dark energy perturbations are present. The growth index depends upon the dark energy equation of state w, the speed of sound of the dark energy fluctuations, the dark matter abundance and the observed comoving scale. The growth index changes by ~5% for small speed of sound and large deviations of w from -1 with respect to its value in the limit of no dark energy perturbations.We present an analytical fit to the growth function of the dark matter perturbations when dark energy perturbations are present. The growth index γ depends upon the dark energy equation of state w , the speed of sound of the dark energy fluctuations, the dark matter abundance and the observed comoving scale. The growth index changes by O(5%) for small speed of sound and large deviations of w from −1 with respect to its value in the limit of no dark energy perturbations.We present an analytical fit to the growth function of the dark matter perturbations when dark energy perturbations are present. The growth index depends upon the dark energy equation of state w, the speed of sound of the dark energy fluctuations, the dark matter abundance and the observed comoving scale. The growth index changes by ~5% for small speed of sound and large deviations of w from -1 with respect to its value in the limit of no dark energy perturbations.arXiv:0807.3343CERN-PH-TH-2008-160IFT-UAM-CSIC-08-46CERN-PH-TH-2008-160IFT-UAM-CSIC-08-46oai:cds.cern.ch:11166512008-07-23 |
spellingShingle | Astrophysics and Astronomy Ballesteros, Guillermo Riotto, Antonio Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures |
title | Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures |
title_full | Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures |
title_fullStr | Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures |
title_full_unstemmed | Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures |
title_short | Parameterizing the Effect of Dark Energy Perturbations on the Growth of Structures |
title_sort | parameterizing the effect of dark energy perturbations on the growth of structures |
topic | Astrophysics and Astronomy |
url | https://dx.doi.org/10.1016/j.physletb.2008.08.035 http://cds.cern.ch/record/1116651 |
work_keys_str_mv | AT ballesterosguillermo parameterizingtheeffectofdarkenergyperturbationsonthegrowthofstructures AT riottoantonio parameterizingtheeffectofdarkenergyperturbationsonthegrowthofstructures |