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Structures in the Universe by Exact Methods: Formation, Evolution, Interactions (Cambridge Monographs on Mathematical Physics)

Structures in the Universe by Exact Methods: Formation, Evolution, Interactions (Cambridge Monographs on Mathematical Physics)

Structures in the Universe by Exact Methods: Formation, Evolution, Interactions
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Structures in the Universe by Exact Methods: Formation, Evolution, Interactions (Cambridge Monographs on Mathematical Physics) Hardback - 2009

by Bolejko, Krzysztof

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Cambridge University Press, 2009-11-23. 1. hardcover. Used: Good. 7.00x1.00x10.00. Buy with confidence. Excellent Customer Service & Return policy.
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  • Title Structures in the Universe by Exact Methods: Formation, Evolution, Interactions (Cambridge Monographs on Mathematical Physics)
  • Author Bolejko, Krzysztof
  • Binding Hardback
  • Edition 1
  • Condition Used: Good
  • Pages 256
  • Volumes 1
  • Language ENG
  • Publisher Cambridge University Press, Cambridge
  • Publication date 2009-11-23
  • Features Bibliography, Index
  • Bookseller's Inventory # SONG0521769140
  • ISBN 9780521769143 / 0521769140
  • Weight 1.35 lbs (0.61 kg)
  • Dimensions 9.8 x 6.7 x 0.8 in (24.89 x 17.02 x 2.03 cm)
  • Size 7.00x1.00x10.00
  • Themes
    • Aspects (Academic): Science/Technology Aspects
  • Category Science
  • Library of Congress subjects Inhomogeneous materials, Einstein field equations
  • Library of Congress Catalogue Number 2009020680
  • Dewey Decimal Code 523
  • Quantity available 1

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Reader reviews for Structures in the Universe by Exact Methods: Formation, Evolution, Interactions (Cambridge Monographs on Mathematical Physics)

From the publisher

As the structures in our Universe are mapped out on ever larger scales, and with increasing detail, the use of inhomogeneous models is becoming an essential tool for analyzing and understanding them. This book reviews a number of important developments in the application of inhomogeneous solutions of Einstein's field equations to cosmology. It shows how inhomogeneous models can be employed to study the evolution of structures such as galaxy clusters and galaxies with central black holes, and to account for cosmological observations like supernovae dimming, the cosmic microwave background, baryon acoustic oscillations or the dependence of the Hubble parameter on redshift within classical general relativity. Whatever dark matter' and dark energy' turn out to be, inhomogeneities exist on many scales and need to be investigated with all appropriate methods. This book is of great value to all astrophysicists and researchers working in cosmology, from graduate students to academic researchers.
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