Cosmic re-onization: theoretical modelling and forthcoming observations

Details Cosmic re-onization: theoretical modelling and forthcoming observations Cosmic re-onization: theoretical modelling and forthcoming observations

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007hia....14..380c&link_type=abstract

Highlights of Astronomy, Volume 14, p. 380-381

Astronomy and Astrophysics

Astronomy

Atomic Processes, Line Formation, Cosmology: Observations, Cosmology: Theory

Scientific paper

With the advent in the near future of radio telescopes such as LOFAR and the 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 21-cm signal from the diffuse IGM prior to its complete re-ionization and thus probe the ‘dark ages’. I discuss the theoretical modelling of the re-ionization process and its observability through the 21-cm signal and the CMB anisotropies.

Affiliated with

Also associated with

No associations

Rating

Cosmic re-onization: theoretical modelling and forthcoming observations does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Cosmic re-onization: theoretical modelling and forthcoming observations, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Cosmic re-onization: theoretical modelling and forthcoming observations will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-974804