Dark energy and large-scale structure of the Universe

The evolution of matter density perturbations in the two-component model of the Universe filled with dark energy (DE) and dust-like matter (M) is considered. We have analysed it for two kinds of DE with ω ≠ −1: a) an unperturbed energy density and b) a perturbed one (uncoupled with the matter). For...

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Бібліографічні деталі
Опубліковано в: :Кинематика и физика небесных тел
Дата:2005
Автори: Kulinich, Yu., Novosyadlyj, B.
Формат: Стаття
Мова:Англійська
Опубліковано: Головна астрономічна обсерваторія НАН України 2005
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Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/79655
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Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Dark energy and large-scale structure of the Universe / Yu. Kulinich, B. Novosyadlyj // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 266-269. — Бібліогр.: 11 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
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author Kulinich, Yu.
Novosyadlyj, B.
author_facet Kulinich, Yu.
Novosyadlyj, B.
citation_txt Dark energy and large-scale structure of the Universe / Yu. Kulinich, B. Novosyadlyj // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 266-269. — Бібліогр.: 11 назв. — англ.
collection DSpace DC
container_title Кинематика и физика небесных тел
description The evolution of matter density perturbations in the two-component model of the Universe filled with dark energy (DE) and dust-like matter (M) is considered. We have analysed it for two kinds of DE with ω ≠ −1: a) an unperturbed energy density and b) a perturbed one (uncoupled with the matter). For these cases, the linear equations for the evolution of the gauge-invariant amplitudes of matter density perturbations are presented. It is shown that, in the case of the unperturbed energy density of DE, the amplitude of matter density perturbations increases slightly faster than in the second case.
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publisher Головна астрономічна обсерваторія НАН України
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spelling Kulinich, Yu.
Novosyadlyj, B.
2015-04-03T17:40:08Z
2015-04-03T17:40:08Z
2005
Dark energy and large-scale structure of the Universe / Yu. Kulinich, B. Novosyadlyj // Кинематика и физика небесных тел. — 2005. — Т. 21, № 5-додаток. — С. 266-269. — Бібліогр.: 11 назв. — англ.
0233-7665
https://nasplib.isofts.kiev.ua/handle/123456789/79655
The evolution of matter density perturbations in the two-component model of the Universe filled with dark energy (DE) and dust-like matter (M) is considered. We have analysed it for two kinds of DE with ω ≠ −1: a) an unperturbed energy density and b) a perturbed one (uncoupled with the matter). For these cases, the linear equations for the evolution of the gauge-invariant amplitudes of matter density perturbations are presented. It is shown that, in the case of the unperturbed energy density of DE, the amplitude of matter density perturbations increases slightly faster than in the second case.
en
Головна астрономічна обсерваторія НАН України
Кинематика и физика небесных тел
MS3: Physics of Stars and Galaxies
Dark energy and large-scale structure of the Universe
Article
published earlier
spellingShingle Dark energy and large-scale structure of the Universe
Kulinich, Yu.
Novosyadlyj, B.
MS3: Physics of Stars and Galaxies
title Dark energy and large-scale structure of the Universe
title_full Dark energy and large-scale structure of the Universe
title_fullStr Dark energy and large-scale structure of the Universe
title_full_unstemmed Dark energy and large-scale structure of the Universe
title_short Dark energy and large-scale structure of the Universe
title_sort dark energy and large-scale structure of the universe
topic MS3: Physics of Stars and Galaxies
topic_facet MS3: Physics of Stars and Galaxies
url https://nasplib.isofts.kiev.ua/handle/123456789/79655
work_keys_str_mv AT kulinichyu darkenergyandlargescalestructureoftheuniverse
AT novosyadlyjb darkenergyandlargescalestructureoftheuniverse