Volume 399, Number 1, February III 2003
|Page(s)||19 - 21|
|Section||Cosmology (including clusters of galaxies)|
|Published online||05 February 2003|
Growth rate of cosmological perturbations in standard model: Explicit analytical solution
Sternberg Astronomical Institute, Moscow University, Moscow, 119899, Russia e-mail: email@example.com
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: firstname.lastname@example.org
5 Isaac Newton Institute of Chile, St. Petersburg Branch
Corresponding author: A. D. Chernin, email@example.com
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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