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Matter-era transfer of a horizon-crossing amplitude
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Linear cosmological density perturbation
Cosmological horizon crossing
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Words: 24
A mode crossing during matter domination acquires the growth factor
(
τ
0
/
τ
H
)
2
. An initial amplitude proportional to
τ
H
2
k
1/2
therefore becomes proportional to
k
1/2
today.
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Cosmological horizon crossing
Linear cosmological density perturbation
Cosmology
Branch of physics
Physics
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