Cosmic microwave background diffusion damping is the suppression of small-angular-scale anisotropy as photons random-walk out of overdense regions during the finite-width recombination epoch. It produces an approximately exponential damping tail in the Cosmic microwave background power spectrum at multipoles .
Past exam of the mathematics course of the University of Cambridge 2023 iii Paper 310 2 e Solution 2026-09-28
A large neutrino degeneracy parameter raises the relativistic energy density and therefore the expansion rate. Big Bang nucleosynthesis tests this through primordial light-element abundances; an electron-neutrino chemical potential also shifts neutron--proton chemical equilibrium directly. The Cosmic microwave background power spectrum tests the changed expansion rate, matter-radiation equality, sound horizon, damping scale, and neutrino anisotropic stress. Finally, large-scale structure of the universe and the matter power spectrum test the altered equality scale and neutrino free streaming. These observables distinguish a degenerate-neutrino cosmology from the standard thermal relic scenario in complementary epochs.
Past exam of the mathematics course of the University of Cambridge 2023 iii Paper 310 3 b Solution 2026-09-28
After a spatial Fourier transform, the preceding equation isThe constant particular solution is . Hence the Sachs-Wolfe combinationcontains only the homogeneous harmonic oscillator modes and satisfiesFor adiabatic initial conditions on large scales, and at the start of matter domination. Up to an irrelevant choice of the phase origin,Thus the radiation acoustic transfer function is flat at as and oscillates on smaller scales. Projection onto the sky produces a large-angle Sachs-Wolfe plateau and, after the full photon-baryon physics is included, the acoustic structure of the Cosmic microwave background power spectrum.
The baryon transfer function should also oscillate soon after cosmological recombination: before decoupling, Thomson scattering forced baryons to share the acoustic motion of the photon-baryon fluid, and recombination does not instantly erase the resulting density pattern.