What are the current ideas describing the large-scale structure of
the Universe? How do they relate to the observed facts? This book
looks at both the strengths and weaknesses of the current big-bang
model in explaining certain puzzling data. It arises from an
international conference that brought together many of the world's
leading players in cosmology. In addition to presenting individual
talks, the proceedings of the resulting discussions are also
recorded. Giving a comprehensive coverage of the expanding field of
cosmology, this text will be valuable for graduate students and
researchers in cosmology and theoretical astrophysics.
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