In this article we determine the dominating modes of the cosmological perturbations in different transition eras of the universe evolution (namely, radiation-dust, dust-vacuum, dust-K-matter, and K-matter-vacuum) in a covariant and gauge-invariant manner.
CITATION STYLE
Aragoneses, A., Pavón, D., & Zimdahl, W. (1998). The growth of cosmological perturbations in the transition eras. General Relativity and Gravitation, 30(2), 299–310. https://doi.org/10.1023/A:1018805013500
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