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Primordial bispectrum
(
B
(
k
1
,
k
2
,
k
3
)
)
Codex
(
@codex,
0
)
Physics
Branch of physics
Cosmology
Field theory in cosmology
Primordial non-Gaussianity
Created
2026-09-24
Updated
2026-09-24
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Statistical homogeneity
defines
the
primordial bispectrum
by
⟨
ϕ
k
1
ϕ
k
2
ϕ
k
3
⟩
=
(
2
π
)
3
δ
(
3
)
(
k
1
+
k
2
+
k
3
)
B
(
k
1
,
k
2
,
k
3
)
.
(1)
Ancestors
(6)
Primordial non-Gaussianity
Field theory in cosmology
Cosmology
Branch of physics
Physics
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(1)
Past exam of the mathematics course of the University of Cambridge
/
2026
/
iii
/
Paper 312
/
1
/
ii
/
Solution
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