Figures 4-6


Figure 4

Forced oscillations. Inside the horizon, the regulatory effects of photon-baryon self-gravity become ineffective. A source that peaks at $x=k\eta\gg 1$ can produce complicated forced oscillations in the fluid. The intrinsic temperature fluctuation $\RF\approx\Theta_0$ suffers a large unobservable offset $-\Psi_s$ (bottom panel) which is removed by the redshift in the effective temperature $\Theta_0+\Psi$ (top panel). Notice that the fundamental period $kr_s = 2\pi$ or $x\simeq 10.9$ is still clearly apparent for this slowly-varying source.

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Figure 5

Baryon drag and relative peak heights. Baryons displace the zero point of the oscillation by $- R\Psi$. For a near BBN baryon content (center panel), the displacement is smaller than the oscillation itself leading to alternating peak heights in the rms. For a much larger baryon content, the photons oscillate around a strongly displaced zero point.

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Figure 6
Diffusion damping. Although adiabatic and isocurvature models predict acoustic oscillations in different positions, they both suffer diffusion damping in the same way. The damping length is fixed by background assumptions, here $\Omega_0=1$, $h=0.5$, $\Omega_b=0.05$ and standard recombination. These calculations were performed using a full numerical integration of the Boltzmann equation with the code of Sugiyama (1995) as were results in Figs.~7,8,10,11.

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