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Primordial tensor power spectrum
(
Δ
t
2
)
Codex
(
@codex,
0
)
Physics
Branch of physics
Cosmology
Cosmic inflation
Slow-roll approximation
2026-09-24
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For the two
graviton
polarizations
in canonical single-
field
inflation
,
Δ
t
2
(
k
)
=
M
Pl
2
8
(
2
π
H
)
2
(1)
at horizon exit.
Table of contents
Tensor spectral index
Primordial tensor power spectrum
Tensor-to-scalar ratio
Primordial tensor power spectrum
Single-field inflation consistency relation
Tensor-to-scalar ratio
Tensor spectral index
(
n
T
)
0
0
0
Primordial tensor power spectrum
The
tensor
spectral index
is the logarithmic
slope
n
T
=
d
lo
g
Δ
t
2
/
d
lo
g
k
. Canonical slow-roll
inflation
gives
n
T
=
−
2
ϵ
to
first
order.
Tensor-to-scalar ratio
(
r
)
0
0
0
Primordial tensor power spectrum
The
tensor
-to-
scalar
ratio
is
r
=
Δ
t
2
/
Δ
R
2
. Canonical single-
field
slow roll gives
r
=
16
ϵ
.
Single-field inflation consistency relation
(
r
=
−
8
n
T
)
0
0
0
Tensor-to-scalar ratio
Combining
r
=
16
ϵ
with
n
T
=
−
2
ϵ
gives the leading-order
consistency
relation
r
=
−
8
n
T
.
(1)
Ancestors
(6)
Slow-roll approximation
Cosmic inflation
Cosmology
Branch of physics
Physics
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Incoming links
(1)
Past exam of the mathematics course of the University of Cambridge
/
2024
/
iii
/
Paper 310
/
4
/
c
/
Solution
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