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Simulations of Large-Scale Structure in the New Millennium

Published online by Cambridge University Press:  23 September 2016

Yasushi Suto
Yasushi Suto*
Affiliation:
Department of Physics, School of Science, The University of Tokyo, Tokyo 113-0033, Japan

Abstract

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Simulations of large-scale structure in the universe have played a vital role in observational cosmology since the 1980's in particular. Their important role will definitely continue to be true in the 21st century; indeed the requirements for simulations in the precision cosmology era will become more progressively demanding as they are supposed to fill the missing link in an accurate and reliable manner between the “initial” condition at z=1000 revealed by WMAP and the galaxy/quasar distribution at z=0 − 6 surveyed by 2dF and SDSS. In this review, I will summarize what we have learned so far from the previous cosmological simulations, and discuss several remaining problems for the new millennium.

Type
Session II: Formation of Large-Scale Structure 75
Information
Symposium - International Astronomical Union , Volume 216: Maps of the Cosmos , 2005 , pp. 105 - 119
Copyright
Copyright © Astronomical Society of the Pacific 2005 

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