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Matter-era linear growth factor
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Linear cosmological density perturbation
Matter-era growing and decaying density modes
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After neglecting the decaying mode, the linear growth between conformal times
τ
1
and
τ
2
is
D
(
τ
2
,
τ
1
)
=
a
(
τ
1
)
a
(
τ
2
)
=
(
τ
1
τ
2
)
2
.
(31)
Ancestors
(6)
Matter-era growing and decaying density modes
Linear cosmological density perturbation
Cosmology
Branch of physics
Physics
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