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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| Published in: | Кинематика и физика небесных тел |
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| Date: | 2005 |
| Main Authors: | , |
| Format: | Article |
| Language: | English |
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Головна астрономічна обсерваторія НАН України
2005
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| Online Access: | https://nasplib.isofts.kiev.ua/handle/123456789/79655 |
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| Journal Title: | Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| Cite this: | 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. |
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Digital Library of Periodicals of National Academy of Sciences of Ukraine| id |
nasplib_isofts_kiev_ua-123456789-79655 |
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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 |
| institution |
Digital Library of Periodicals of National Academy of Sciences of Ukraine |
| collection |
DSpace DC |
| title |
Dark energy and large-scale structure of the Universe |
| spellingShingle |
Dark energy and large-scale structure of the Universe Kulinich, Yu. Novosyadlyj, B. MS3: Physics of Stars and Galaxies |
| title_short |
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_sort |
dark energy and large-scale structure of the universe |
| author |
Kulinich, Yu. Novosyadlyj, B. |
| author_facet |
Kulinich, Yu. Novosyadlyj, B. |
| topic |
MS3: Physics of Stars and Galaxies |
| topic_facet |
MS3: Physics of Stars and Galaxies |
| publishDate |
2005 |
| language |
English |
| container_title |
Кинематика и физика небесных тел |
| publisher |
Головна астрономічна обсерваторія НАН України |
| format |
Article |
| 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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| issn |
0233-7665 |
| url |
https://nasplib.isofts.kiev.ua/handle/123456789/79655 |
| 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. |
| work_keys_str_mv |
AT kulinichyu darkenergyandlargescalestructureoftheuniverse AT novosyadlyjb darkenergyandlargescalestructureoftheuniverse |
| first_indexed |
2025-12-07T19:40:25Z |
| last_indexed |
2025-12-07T19:40:25Z |
| _version_ |
1850879692317392896 |