21 cm cosmology in the 21st century
Imaging the Universe during the first hundreds of millions of years remains one of the
exciting challenges facing modern cosmology. Observations of the redshifted 21 cm line of …
exciting challenges facing modern cosmology. Observations of the redshifted 21 cm line of …
The epoch of reionization
S Zaroubi - The first galaxies: theoretical predictions and …, 2012 - Springer
The Universe's dark ages end with the formation of the first generation of galaxies. These
objects start emitting ultraviolet radiation that carves out ionized regions around them. After a …
objects start emitting ultraviolet radiation that carves out ionized regions around them. After a …
Fundamental physics with the square kilometre array
The Square Kilometre Array (SKA) is a planned large radio interferometer designed to
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
operate over a wide range of frequencies, and with an order of magnitude greater sensitivity …
A small amount of mini-charged dark matter could cool the baryons in the early Universe
The dynamics of our Universe is strongly influenced by pervasive—albeit elusive—dark
matter, with a total mass about five times the mass of all the baryons,. Despite this, its origin …
matter, with a total mass about five times the mass of all the baryons,. Despite this, its origin …
HERA phase I limits on the cosmic 21 cm signal: constraints on astrophysics and cosmology during the epoch of reionization
Abstract Recently, the Hydrogen Epoch of Reionization Array (HERA) has produced the
experiment's first upper limits on the power spectrum of 21 cm fluctuations at z∼ 8 and 10 …
experiment's first upper limits on the power spectrum of 21 cm fluctuations at z∼ 8 and 10 …
Upper limits on the 21 cm epoch of reionization power spectrum from one night with LOFAR
We present the first limits on the Epoch of Reionization 21 cm H i power spectra, in the
redshift range z= 7.9–10.6, using the Low-Frequency Array (LOFAR) High-Band Antenna …
redshift range z= 7.9–10.6, using the Low-Frequency Array (LOFAR) High-Band Antenna …
Dark energy
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Late-time cosmology with 21 cm intensity map** experiments
We present a framework for forecasting cosmological constraints from future neutral
hydrogen intensity map** experiments at low to intermediate redshifts. In the process, we …
hydrogen intensity map** experiments at low to intermediate redshifts. In the process, we …
64 constraints on reionization: the 21 cm power spectrum at z= 8.4
In this paper, we report new limits on 21 cm emission from cosmic reionization based on a
135 day observing campaign with a 64-element deployment of the Donald C. Backer …
135 day observing campaign with a 64-element deployment of the Donald C. Backer …
Reionization and the cosmic dawn with the square kilometre array
Abstract The Square Kilometre Array (SKA) will have a low frequency component (SKA-low)
which has as one of its main science goals the study of the redshifted 21 cm line from the …
which has as one of its main science goals the study of the redshifted 21 cm line from the …