This up-to-date and concise account of a critical period of the
early universe directly links the latest theories and experiments.
Targeted at cosmological problems rather than specific methods, it
begins with an introduction reviewing the early universe and looks
at why reionization is important. The process of reionization
analyzes simple analytical considerations and compares existing
observations, while a further chapter describes some of the issues
regarding the transition from Population III to Population II
stars, as well as the constraints that can be derived from WMAP.
Further chapters survey the latest numerical modeling and future
perspectives for studying the dark ages using galaxies as
probes.
Written by a scientist with much experience in both research and
writing, this account is equally suitable for young researchers as
well as master and PhD students.
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