Kavli Affiliate: George Efstathiou
| First 5 Authors: Sudipta Sikder, Sudipta Sikder, , ,
| Summary:
The 21-cm line of hydrogen is the most promising probe of the Dark Ages and
Cosmic Dawn. We combine hydrodynamical simulations with a large-scale grid in
order to calculate the effect of non-linear structure formation on the
large-scale 21-cm power spectrum, focusing on redshifts $z=20-40$. As the
clumping effect arises from small-scale density fluctuations, it offers a
unique opportunity to probe the standard cold dark matter model in a new regime
and thus potentially investigate the properties of dark matter. To this end, we
also study a warm dark matter $-$ like model with a Gaussian cutoff on a scale
of 50 kpc. We find that clumping has a significant impact on the large-scale
21-cm power spectrum. For example, for the Dark Ages case at $z=30$ and
wavenumber $k=0.05$ Mpc$^-1$, small-scale clustering enhances the 21-cm power
spectrum by $13%$. Once Lyman-$alpha$ coupling kicks in due to the first
stars, the 21-cm signal strengthens, and the effect of clumping grows; it
suppresses the observable power spectrum at $z=20$ by a factor of two, while
the cutoff model has less than half the clumping impact. The clumping effect is
significantly higher than the sensitivity of the planned Square Kilometre Array
(SKA) AA$^star$ configuration, by up to a factor of 20 for standard cold dark
matter, though detection will require separation from foregrounds and from
astrophysical contributions to the 21-cm power spectrum.
| Search Query: ArXiv Query: search_query=au:”Anastasia Fialkov”&id_list=&start=0&max_results=3