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A Short Introduction to Reionization Physics
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The epoch of reionization probes the state of our universe when the very first stars formed and ionized the hydrogen atoms in the surrounding medium. Since the epoch has not yet been probed observationally, it is often called the "final frontier" of observational cosmology. This final frontier is attracting a lot of attention because of the availability of a large number of telescopes in a wide variety of wavebands. This review article summarizes some of the concepts required to understand the interesting physics of reionization and how to analyze the high-redshift universe using related observations.
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Impact of CMB low-$\ell$ EE polarization data on dark energy parameterizations
Removing Planck's low-ℓ EE polarization data shifts A_s and τ_reio upward and makes three dark-energy parameterizations look more quintessence-like, with model-selection evidence depending on the dataset and prior.
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