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Spatially flat FLRW metric
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Physics
Branch of physics
Cosmology
Friedmann-Lemaitre-Robertson-Walker metric
Created
2026-09-24
Updated
2026-09-24
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In Cartesian
comoving coordinates
and signature
(
−
,
+
,
+
,
+
)
,
a
spatially flat FLRW
universe
has
d
s
2
=
−
c
2
d
t
2
+
a
2
(
t
)
(
d
x
2
+
d
y
2
+
d
z
2
)
.
(1)
Ancestors
(5)
Friedmann-Lemaitre-Robertson-Walker metric
Cosmology
Branch of physics
Physics
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Incoming links
(4)
Past exam of the mathematics course of the University of Cambridge
/
2015
/
iii
/
Paper 55
/
1
/
i
/
Solution
Past exam of the mathematics course of the University of Cambridge
/
2015
/
iii
/
Paper 55
/
2
/
a
/
Solution
Past exam of the mathematics course of the University of Cambridge
/
2019
/
iii
/
Paper 310
/
1
/
b
/
Solution
Past exam of the mathematics course of the University of Cambridge
/
2023
/
ii
/
Paper 4
/
37B
/
b
/
ii
/
Solution
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