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Decreasing Hubble rate does not alone fix scalar tilt
(
n
s
−
1
≃
−
2
ϵ
H
−
d
ln
ϵ
H
/
d
N
)
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0
)
...
Cosmology
Cosmic inflation
Slow-roll approximation
Comoving curvature perturbation
Slow-roll curvature power spectrum
Scalar spectral index in Hubble slow-roll parameters
2026-10-20
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The
tensor
spectrum
is proportional to
H
2
, but the single-
field
slow-roll
curvature
spectrum
is proportional to
H
2
/
ϵ
H
. Thus
n
s
−
1
≃
−
2
ϵ
H
−
d
ln
ϵ
H
/
d
N
.
A
decreasing
H
gives
a
red leading
tensor
tilt, while the evolving
scalar
conversion factor can change the
sign
of the
scalar
tilt.
Ancestors
(9)
Scalar spectral index in Hubble slow-roll parameters
Slow-roll curvature power spectrum
Comoving curvature perturbation
Slow-roll approximation
Cosmic inflation
Cosmology
Branches of physics
Physics
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Past exam of the relativistic Astrophysics and Cosmology course of the University of Cambridge
/
2016
/
Paper 1
/
2
/
Solution
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