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Inflationary solution of the flatness problem
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Physics
Branch of physics
Cosmology
Critical density
Cosmological density parameter
Flatness problem
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Words: 21
The continuity equation gives
d
t
d
(
ρ
a
2
)
=
−
H
a
2
(
ρ
+
3
P
)
.
(5)
During expansion with
ρ
+
3
P
<
0
, the product
ρ
a
2
grows and
∣
Ω
−
1
−
1∣
∝
(
ρ
a
2
)
−
1
decreases.
Ancestors
(7)
Flatness problem
Cosmological density parameter
Critical density
Cosmology
Branch of physics
Physics
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