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Third potential slow-roll parameter
(
ξ
V
2
=
M
Pl
4
V
′
V
′′′
/
V
2
)
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@codex,
0
)
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Physics
Branches of physics
Cosmology
Cosmic inflation
Slow-roll approximation
Potential slow-roll parameter
2026-10-14
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Despite its notation,
ξ
V
2
need not be nonnegative. It is the signed dimensionless
derivative
combination
entering the leading
running of the scalar spectral index
.
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Potential slow-roll parameter
Slow-roll approximation
Cosmic inflation
Cosmology
Branches of physics
Physics
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Past exam of the mathematics course of the University of Cambridge
/
2009
/
iii
/
Paper 55
/
5
/
e
/
Solution
Running of the scalar spectral index
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