Your browser doesn't support javascript.
loading
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.
Koopmans, Léon V E; Barkana, Rennan; Bentum, Mark; Bernardi, Gianni; Boonstra, Albert-Jan; Bowman, Judd; Burns, Jack; Chen, Xuelei; Datta, Abhirup; Falcke, Heino; Fialkov, Anastasia; Gehlot, Bharat; Gurvits, Leonid; Jelic, Vibor; Klein-Wolt, Marc; Lazio, Joseph; Meerburg, Daan; Mellema, Garrelt; Mertens, Florent; Mesinger, Andrei; Offringa, André; Pritchard, Jonathan; Semelin, Benoit; Subrahmanyan, Ravi; Silk, Joseph; Trott, Cathryn; Vedantham, Harish; Verde, Licia; Zaroubi, Saleem; Zarka, Philippe.
  • Koopmans LVE; Kapteyn Astronomical Institute, University of Groningen, Groningen, Netherlands.
  • Barkana R; Tel-Aviv University, Tel Aviv, Israel.
  • Bentum M; Eindhoven University of Technology, Eindhoven, Netherlands.
  • Bernardi G; ASTRON, Dwingeloo, Netherlands.
  • Boonstra AJ; INAF, Bologna, Italy.
  • Bowman J; SKAO-SA, Cape Town, South Africa.
  • Burns J; ASTRON, Dwingeloo, Netherlands.
  • Chen X; Arizona State University, Tempe, AZ USA.
  • Datta A; University of Colorado Boulder, Boulder, CO USA.
  • Falcke H; NAOC, Beijing, China.
  • Fialkov A; IIT Indore, Indore, India.
  • Gehlot B; Radboud University, Nijmegen, Netherlands.
  • Gurvits L; IoA, University of Cambridge, Cambridge, UK.
  • Jelic V; Arizona State University, Tempe, AZ USA.
  • Klein-Wolt M; JIVE and Delft University of Technology, Delft, Netherlands.
  • Lazio J; Institut Ruder Boskovic, Zagreb, Croatia.
  • Meerburg D; Radboud University, Nijmegen, Netherlands.
  • Mellema G; JPL, Caltech, Pasadena, CA USA.
  • Mertens F; VSI, University of Groningen, Groningen, Netherlands.
  • Mesinger A; Stockholm University, Stockholm, Sweden.
  • Offringa A; Kapteyn Astronomical Institute, University of Groningen, Groningen, Netherlands.
  • Pritchard J; Observatoire de Paris, Paris, France.
  • Semelin B; Scuola Normale Superiore, Pisa, Italy.
  • Subrahmanyan R; ASTRON, Dwingeloo, Netherlands.
  • Silk J; Imperial College, London, UK.
  • Trott C; Observatoire de Paris, Paris, France.
  • Vedantham H; Raman Research Institute, Bengaluru, India.
  • Verde L; Institut d'astrophysique de Paris, Paris, France.
  • Zaroubi S; University of Oxford, Oxford, UK.
  • Zarka P; Curtin University, Perth, Australia.
Exp Astron (Dordr) ; 51(3): 1641-1676, 2021.
Article en En | MEDLINE | ID: mdl-34511720
ABSTRACT
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.
Palabras clave