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Scale-invariant inflationary power spectrum
...
Cosmic inflation
Inflaton
Inflaton action in an expanding universe
Inflationary scalar Fourier mode
Canonically rescaled de Sitter scalar mode
Bunch-Davies vacuum
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A Fourier-space variance
P
k
in three dimensions is scale invariant when the dimensionless power per logarithmic wavenumber interval,
Δ
2
(
k
)
=
2
π
2
k
3
P
k
,
(12)
is independent of
k
. For a massless inflaton mode at late times,
P
k
⟶
2
c
3
k
3
ℏ
H
inf
2
,
(13)
so
Δ
2
(
k
)
is constant.
Ancestors
(10)
Bunch-Davies vacuum
Canonically rescaled de Sitter scalar mode
Inflationary scalar Fourier mode
Inflaton action in an expanding universe
Inflaton
Cosmic inflation
Cosmology
Branch of physics
Physics
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