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    INFLATIONARY COSMOLOGY REVISITED
    An Overview of Contemporary Scientific Cosmology After the Inflationary Proposal

    by Julio A Gonzalo (Universidad Autonoma de Madrid, Spain)

    Table of Contents (27k)
    Prologue (84k)
    Chapter 1: Steady State Versus Big Bang Cosmology (374k)

    Scientific Cosmology is clearly one of the most active physics research fields at present, and likely to remain so in the near future. Shortly after the pioneering cosmological work of Einstein, Georges Lemaitre proposed a model which some years later to be known as the big-bang model. In the early fifties an alternative proposal, the so called steady-state (expansion at constant density) model, became the fashionable model in prominent academic circles. The discovery of the cosmic background microwave radiation (Penzias & Wilson, 1965) made the steady-state model almost untenable. A quarter of a century later the inflationary model was proposed, becoming extraordinarily popular almost immediately. For some it seemed to combine attractive features of both the steady-state and the big-bang models, by postulating a very early violent (constant density) expansion during a very tiny fraction of a second.

    The book makes use of the best and most recent observational data, from the Cosmic Background Explorer (COBE, 1992) to the Microwave Anisotropy Probe (WMAP, 2003), to discuss the merits and demerits of inflationary cosmology for a general readership acquainted with the basic facts of scientific cosmology. A complete Glossary and a detailed Index help the reader to follow controversial topics, such as dark matter, dark energy, cosmic flatness and accelerated expansion.

     
    Contents:
    • Steady State versus Big Bang Cosmologies
    • The Microwave CBR
    • The Birth of Inflationary Cosmology
    • The Cosmic Background Explorer (COBE)
    • Dark Matter, Cosmic Flatness and Accelerated Expansion
    • The Microwave Anisotropy Probe (WMAP)
    • On the Monopole, Flatness and Horizon Problems
    • An Alternative to Inflation?
    • Appendix. How Close are the Cosmic Times at Decoupling and Atom Formation
     
    Readership: Scientists, physicists, astrophysicists and general readers with a good scientific background.
     
    “The author has succeeded where other authors have sometimes failed, namely to explain a topic at the forefront of science and hence far removed from ordinary human experience so that it can be understood by scientists in neighbouring fields and also by non-scientists who are familiar with the basic facts … In under 100 pages, the author summarizes the different models of contemporary scientific cosmology and shows how each model has tried to overcome the shortcomings of the preceding one. Then he presents the observational results that have led to the development of the Inflationary Model, the most recent attempt to understand the initial phases of cosmic evolution. He shows that these results can also be explained without making the implausible assumptions of that approach. He does so with a minimum of mathematical reasoning, employing convincing logical arguments instead whenever possible. Occasional references to the author's own experiences in the search for a valid cosmological model add a personal touch to the book.”
    Professor Emeritus Hans S Plendl

    Florida State University
     
    120pp    Pub. date: Mar 2005  
    ISBN:   978-981-256-151-0
    981-256-151-X
       US$67 / £37

     


    120pp    Pub. date: Mar 2005  
    ISBN:   978-981-270-123-7(ebook)
    981-270-123-0(ebook)
       US$87

     


     

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    Updated on 8 February 2010