Physical Cosmology From the 21-cm Line

26 Sep 2019 Furlanetto Steven R. UCLA

We describe how the high-redshift 21-cm background can be used to improve both our understanding of the fundamental cosmological parameters of our Universe and exotic processes originating in the dark sector. The 21-cm background emerging during the cosmological Dark Ages, the era between hydrogen recombination and the formation of the first luminous sources (likely at z ~ 30), is difficult to measure but provides several powerful advantages for these purposes: in addition to the lack of astrophysical contamination, it will allow probes of very small scale structure over a very large volume... (read more)

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  • COSMOLOGY AND NONGALACTIC ASTROPHYSICS