| Issue |
A&A
Volume 399, Number 1, February III 2003
|
|
|---|---|---|
| Page(s) | 19 - 21 | |
| Section | Cosmology (including clusters of galaxies) | |
| DOI | https://doi.org/10.1051/0004-6361:20021763 | |
| Published online | 05 February 2003 | |
Growth rate of cosmological perturbations in standard model: Explicit analytical solution
1
Sternberg Astronomical Institute, Moscow University, Moscow, 119899, Russia e-mail: chernin@sai.msu.ru
2
Tuorla Observatory, University of Turku, Piikkiö, 21500, Finland
3
Astronomy Division, Oulu University, Oulu, 90014, Finland
4
Sobolev Astronomical Institute, St.-Petersburg State University, Univ. pr. 28, Staryi Peterhoff, St.-Petersburg 198504, Russia e-mail: dinmax@dn1756.spb.edu
5
Isaac Newton Institute of Chile, St. Petersburg Branch
Corresponding author: A. D. Chernin, chernin@sai.msu.ru
Received:
6
September
2002
Accepted:
14
November
2002
An explicit analytical solution is reported for the growth rate of cosmological perturbations in a flat model with non-zero vacuum energy density.
Key words: cosmology: theory / cosmology: large-scale structure of Universe
© ESO, 2003
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