Abstract
Some basic physical properties of the cosmological many-body problem are discussed and the successes and limitations of its applicability to galaxy clustering are reviewed, especially regarding recent observations of high redshift clustering.
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© 2001 Springer Science+Business Media Dordrecht
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Saslaw, W.C. (2001). The Cosmological Many-Body Problem and Some of Its Observational Implications. In: Sánchez, N.G. (eds) Current Topics in Astrofundamental Physics: The Cosmic Microwave Background. NATO Science Series, vol 562. Springer, Dordrecht. https://doi.org/10.1007/978-94-010-0748-1_20
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DOI: https://doi.org/10.1007/978-94-010-0748-1_20
Publisher Name: Springer, Dordrecht
Print ISBN: 978-0-7923-6856-4
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