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Peering into the dark (ages) with low-frequency space interferometers Using the 21-cm signal of neutral hydrogen from the infant universe to probe fundamental (Astro)physics

Authors :
Harish Vedantham
Daan Meerburg
Joseph Lazio
A. R. Offringa
Jonathan R. Pritchard
Rennan Barkana
Andrei Mesinger
Anastasia Fialkov
Abhirup Datta
Saleem Zaroubi
B. K. Gehlot
Heino Falcke
Léon V. E. Koopmans
Mark J. Bentum
Marc Klein-Wolt
Philippe Zarka
Jack O. Burns
Cathryn M. Trott
Licia Verde
Leonid I. Gurvits
Xuelei Chen
Florent Mertens
Ravi Subrahmanyan
Vibor Jelić
Judd D. Bowman
Gianni Bernardi
Garrelt Mellema
Albert-Jan Boonstra
B. Semelin
Joseph Silk
Observatoire de Paris - Site de Paris (OP)
Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris
Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)
HEP, INSPIRE
Koopmans, Léon VE [0000-0003-1840-0312]
Apollo - University of Cambridge Repository
Koopmans, Léon V E [0000-0003-1840-0312]
Source :
Experimental Astronomy: an international journal on astronomical instrumentation and data analysis, 51(3), Experimental Astronomy, 51, 1641-1676, Experimental Astronomy, 51, pp. 1641-1676
Publication Year :
2021

Abstract

Neutral hydrogen pervades the infant Universe, and its redshifted 21-cm signal allows one to chart the Universe. This signal allows one to probe astrophysical processes such as the formation of the first stars, galaxies, (super)massive black holes and enrichment of the pristine gas from z~6 to z~30, as well as fundamental physics related to gravity, dark matter, dark energy and particle physics at redshifts beyond that. As one enters the Dark Ages (z>30), the Universe becomes pristine. Ground-based low-frequency radio telescopes aim to detect the spatial fluctuations of the 21-cm signal. Complementary, global 21-cm experiments aim to measure the sky-averaged 21-cm signal. Escaping RFI and the ionosphere has motivated space-based missions, such as the Dutch-Chinese NCLE instrument (currently in lunar L2), the proposed US-driven lunar or space-based instruments DAPPER and FARSIDE, the lunar-orbit interferometer DSL (China), and PRATUSH (India). To push beyond the current z~25 frontier, though, and measure both the global and spatial fluctuations (power-spectra/tomography) of the 21-cm signal, low-frequency (1-100MHz; BW~50MHz; z>13) space-based interferometers with vast scalable collecting areas (1-10-100 km2), large filling factors (~1) and large fields-of-view (4pi sr.) are needed over a mission lifetime of >5 years. In this ESA White Paper, we argue for the development of new technologies enabling interferometers to be deployed, in space (e.g. Earth-Sun L2) or in the lunar vicinity (e.g. surface, orbit or Earth-Moon L2), to target this 21-cm signal. This places them in a stable environment beyond the reach of most RFI from Earth and its ionospheric corruptions, enabling them to probe the Dark Ages as well as the Cosmic Dawn, and allowing one to investigate new (astro)physics that is inaccessible in any other way in the coming decades. [Abridged]

Details

ISSN :
09226435 and 16411676
Volume :
51
Database :
OpenAIRE
Journal :
Experimental Astronomy
Accession number :
edsair.doi.dedup.....398bacd29ec9025a00b0199544320458