Cosmological reionization in LCDM models with and without a scalar field

Details Cosmological reionization in LCDM models with and without a scalar field Cosmological reionization in LCDM models with and without a scalar field

Mar 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006newar..50..191c&link_type=abstract

New Astronomy Reviews, Volume 50, Issue 1-3, p. 191-198.

Astronomy and Astrophysics

Astronomy

2

Scientific paper

One would not have expected just a few years ago that we could observationally start probing the reionization process in the redshift range 6 30. This is indeed extremely exciting, because we are in a completely uncharted water. I will review some of the latest developments on cosmological reionization and suggest, in a somewhat more personal way, that the universe may be reionized twice in order to paint a picture that is consistent with all observations, including SDSS quasar observations, WMAP CMB experiment and Lyα forest observations. Further suggestion is made in the context of the LCDM model with a scalar field to promote early structure formation.

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