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The dark matter problem. A historical perspective. (English) Zbl 1204.85004

Cambridge: Cambridge University Press (ISBN 978-0-521-11301-4/hbk). viii, 205 p. (2010).
This book describes how astronomers came to believe that the matter content of the Universe is dominated by dark matter: hypothetical particles which interact with normal matter primarily through the force of gravity. Mathematics is kept to a minimum, but many elucidating figures and tables help understanding the text.
The first chapters of this book present the main arguments why dark matter should exist: otherwise the stability of galaxies cannot be explained, and the calculated velocity of stars in their motion around the center of the galaxy would contradict the observed velocity of them.
Beginning from chapter 6, dark matter and dark energy within cosmology are discussed. Both theoretical and observational topics are worked out in detail. In chapter 10 the idea is presented, that instead of introducing dark matter, it might be possible change the theory of gravity such as to reach coincidence with the observed facts.
Chapter 12 shortly discusses philosophical questions like Kuhn’s change of paradigms. The appendix explains many notions from the text and deduces some essential formulas, e.g. for luminosity, redshift, and the Friedmann equation for cosmology. A reference list and subject index close this interesting overview about the detection of dark matter in the universe.

MSC:

85-03 History of astronomy and astrophysics
01A60 History of mathematics in the 20th century
01A61 History of mathematics in the 21st century
83F05 Relativistic cosmology
83C55 Macroscopic interaction of the gravitational field with matter (hydrodynamics, etc.)
85A25 Radiative transfer in astronomy and astrophysics
85A30 Hydrodynamic and hydromagnetic problems in astronomy and astrophysics
76W05 Magnetohydrodynamics and electrohydrodynamics
00A79 Physics
00A30 Philosophy of mathematics
85A40 Astrophysical cosmology

Keywords:

dark energy