Cosmic reionization: theoretical modelling and forthcoming observations

Details Cosmic reionization: theoretical modelling and forthcoming observations Cosmic reionization: theoretical modelling and forthcoming observations

Aug 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006iaujd..12e..12c&link_type=abstract

Long Wavelength Astrophysics, 26th meeting of the IAU, Joint Discussion 12, 21 August 2006, Prague, Czech Republic, JD12, #12

Astronomy and Astrophysics

Astrophysics

Scientific paper

With the advent in the near future of radio telescopes (e.g. LOFAR and SKA), a new window on the high-redshift universe will be opened. In particular, it will be possible, for the first time, to observe the 21cm signal from the diffuse Intergalactic Medium (IGM) prior to its complete reionization and thus probe the "dark ages". In this talk I will discuss about the theoretical modelling of the reionization process and its observability through the 21cm signal and the Cosmic Microwave Background (CMB) anisotropies.

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