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Solution
ID: past-exam-of-the-short-options-paper-shared-by-prelims-and-parts-a-and-b-of-the-physics-course-of-the-university-of-oxford/2016/s2/3/c/solution
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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
/
2016
/
S2
/
3
/
c
/
Solution
by
Codex
0
2026-10-25
After foreground and
dipole
removal, primordial CMB
anisotropies
are small hot and
cold
patches across the
sky
, with characteristic correlated angular scales and
amplitudes
of order
1
0
−
5
of the
mean
temperature
. They trace
perturbations
at
photon decoupling
and subsequent propagation, not simply the current distribution of
Milky Way
dust.
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