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2007

Linear effects of perturbed recombination

Lewis, Antony

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Perturbations in the ionization fraction after recombination affect the Compton cooling of density perturbations.

Once the gas temperature starts to decouple from the CMB temperature, ionization fraction perturbations can have a significant influence on the subsequent gas temperature perturbation evolution.
This directly affects the 21cm spin temperature of the gas, and also modifies the small-scale baryon perturbation evolution via the difference in baryon pressure.
The effect on the gas temperature perturbations can be significant on all scales, and galactic-scale baryon perturbations are modified at the percent level at redshifts z >~ 100 where numerical simulations are typically started.

Linear effects of perturbed recombination · Around

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2000
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