Book contents
- Frontmatter
- Contents
- Prologue
- Part I Historical
- Part II Descriptions of Clustering
- Part III Gravity and Correlation Functions
- Part IV Gravity and Distribution Functions
- Part V Computer Experiments for Distribution Functions
- Part VI Observations of Distribution Functions
- Part VII Future Unfoldings
- Bibliography
- Index
Part III - Gravity and Correlation Functions
Published online by Cambridge University Press: 19 January 2010
- Frontmatter
- Contents
- Prologue
- Part I Historical
- Part II Descriptions of Clustering
- Part III Gravity and Correlation Functions
- Part IV Gravity and Distribution Functions
- Part V Computer Experiments for Distribution Functions
- Part VI Observations of Distribution Functions
- Part VII Future Unfoldings
- Bibliography
- Index
Summary
Of all the processes that might produce correlations among galaxies in our Universe, we know only one that definitely exists. It is gravity. Inevitably and inexorably, as Newton told Bentley, gravitational instability causes the galaxies to cluster.
Of all the descriptions of galaxy clustering, the correlation functions are connected most closely to the underlying gravitational dynamics. The next several chapters develop this connection. It resembles a great fugue, starting with simple themes and variations, then combining, developing, and recombining them to obtain a grand theoretical structure whose main insights have formed over the last three decades and which still continues to expand.
- Type
- Chapter
- Information
- The Distribution of the GalaxiesGravitational Clustering in Cosmology, pp. 169 - 170Publisher: Cambridge University PressPrint publication year: 1999