Simulations of large-scale structure in the new millennium

被引：0
|
作者：
Suto, Y [1 ]
机构：
[1] Univ Tokyo, Dept Phys, Sch Sci, Tokyo 1130033, Japan
来源：
MAPS OF THE COSMOS | 2005年 / 216期
关键词：
D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
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页码：105 / 119
页数：15
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