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Matter-era growing and decaying density modes

In a flat matter-dominated era with

a \propto τ^{2}

, one has

H = 2/ τ

and

δ = A τ^{2} + B τ^{- 3} .

The growing mode is proportional to the scale factor.

Table of contents 65 2
- Cosmic-time matter density modes Matter-era growing and decaying density modes 25
- Matter-era linear growth factor Matter-era growing and decaying density modes 17

 Ancestors (5)