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Past exam of the short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
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2012
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S2
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3
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c
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Physics course of the University of Oxford
Short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
Past exam of the short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
2012
S2
3
2026-10-25
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Solution
c
Solution
0
0
0
c
After subtracting the
mean
, the
motion
-induced
dipole
and
galactic foregrounds
, intrinsic
Cosmic microwave background anisotropy
appears
as
angular hot and
cold
patches, typically at the
1
0
−
5
fractional scale. These spatial
temperature fluctuations
encode early
density
and
velocity
structure. The displayed patch
pattern
is illustrative, with no claim to reproduce an observed
sky
map
.
Figure 1.
Schematic
microwave
components: Galactic dust,
a
kinematic
dipole
and intrinsic
anisotropy
, using separate colour scales
.
Details
.
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(11)
3
S2
2012
Past exam of the short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
Short options paper shared by Prelims and Parts A and B of the physics course of the University of Oxford
Physics course of the University of Oxford
Undergraduate course of the University of Oxford
Course of the University of Oxford
University of Oxford
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