TY - JOUR
T1 - Peering into the dark (ages) with low-frequency space interferometers
T2 - Using the 21-cm signal of neutral hydrogen from the infant universe to probe fundamental (Astro)physics
AU - Koopmans, Léon V.E.
AU - Barkana, Rennan
AU - Bentum, Mark
AU - Bernardi, Gianni
AU - Boonstra, Albert Jan
AU - Bowman, Judd
AU - Burns, Jack
AU - Chen, Xuelei
AU - Datta, Abhirup
AU - Falcke, Heino
AU - Fialkov, Anastasia
AU - Gehlot, Bharat
AU - Gurvits, Leonid
AU - Jelić, Vibor
AU - Klein-Wolt, Marc
AU - Lazio, Joseph
AU - Meerburg, Daan
AU - Mellema, Garrelt
AU - Mertens, Florent
AU - Mesinger, Andrei
AU - Offringa, André
AU - Pritchard, Jonathan
AU - Semelin, Benoit
AU - Subrahmanyan, Ravi
AU - Silk, Joseph
AU - Trott, Cathryn
AU - Vedantham, Harish
AU - Verde, Licia
AU - Zaroubi, Saleem
AU - Zarka, Philippe
N1 - Publisher Copyright:
© 2021, The Author(s).
PY - 2021/6
Y1 - 2021/6
N2 - The Dark Ages and Cosmic Dawn are largely unexplored windows on the infant Universe (z ~ 200–10). Observations of the redshifted 21-cm line of neutral hydrogen can provide valuable new insight into fundamental physics and astrophysics during these eras that no other probe can provide, and drives the design of many future ground-based instruments such as the Square Kilometre Array (SKA) and the Hydrogen Epoch of Reionization Array (HERA). We review progress in the field of high-redshift 21-cm Cosmology, in particular focussing on what questions can be addressed by probing the Dark Ages at z > 30. We conclude that only a space- or lunar-based radio telescope, shielded from the Earth’s radio-frequency interference (RFI) signals and its ionosphere, enable the 21-cm signal from the Dark Ages to be detected. We suggest a generic mission design concept, CoDEX, that will enable this in the coming decades.
AB - The Dark Ages and Cosmic Dawn are largely unexplored windows on the infant Universe (z ~ 200–10). Observations of the redshifted 21-cm line of neutral hydrogen can provide valuable new insight into fundamental physics and astrophysics during these eras that no other probe can provide, and drives the design of many future ground-based instruments such as the Square Kilometre Array (SKA) and the Hydrogen Epoch of Reionization Array (HERA). We review progress in the field of high-redshift 21-cm Cosmology, in particular focussing on what questions can be addressed by probing the Dark Ages at z > 30. We conclude that only a space- or lunar-based radio telescope, shielded from the Earth’s radio-frequency interference (RFI) signals and its ionosphere, enable the 21-cm signal from the Dark Ages to be detected. We suggest a generic mission design concept, CoDEX, that will enable this in the coming decades.
KW - 21-cm cosmology
KW - Cosmic dawn
KW - Dark ages
KW - Epoch of reionization
KW - Space or lunar-based radio telescopes
UR - http://www.scopus.com/inward/record.url?scp=85114175274&partnerID=8YFLogxK
U2 - 10.1007/s10686-021-09743-7
DO - 10.1007/s10686-021-09743-7
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C2 - 34511720
AN - SCOPUS:85114175274
SN - 0922-6435
VL - 51
SP - 1641
EP - 1676
JO - Experimental Astronomy
JF - Experimental Astronomy
IS - 3
ER -