有哪些信誉好的足球投注网站- 1、本文档共15页，可阅读全部内容。
- 2、有哪些信誉好的足球投注网站（book118）网站文档一经付费（服务费），不意味着购买了该文档的版权，仅供个人/单位学习、研究之用，不得用于商业用途，未经授权，严禁复制、发行、汇编、翻译或者网络传播等，侵权必究。
- 3、本站所有内容均由合作方或网友上传，本站不对文档的完整性、权威性及其观点立场正确性做任何保证或承诺！文档内容仅供研究参考，付费前请自行鉴别。如您付费，意味着您自己接受本站规则且自行承担风险，本站不退款、不进行额外附加服务；查看《如何避免下载的几个坑》。如果您已付费下载过本站文档，您可以点击 这里二次下载。
- 4、如文档侵犯商业秘密、侵犯著作权、侵犯人身权等，请点击“版权申诉”（推荐），也可以打举报电话：400-050-0827(电话支持时间：9:00-18:30)。
查看更多
Simulations of Large-Scale Structure in the New Millennium
a
r
X
i
v
:
a
s
t
r
o
-
p
h
/
0
3
1
1
5
7
5
v
1
2
5
N
o
v
2
0
0
3
**TITLE**
ASP Conference Series, Vol. **VOLUME***, **YEAR OF PUBLICATION**
**NAMES OF EDITORS**
Simulations of Large-Scale Structure
in the New Millennium
Yasushi Suto
Department of Physics, School of Science, The University of Tokyo,
Tokyo 113-0033, Japan
Abstract. Simulations of large-scale structure in the universe have played
a vital role in observational cosmology since 1980’s in particular. Their
important role will definitely continue to be true in the 21st century.
Rather the requirements for simulations in the precision cosmology era
will become more progressively demanding; they are supposed to fill the
missing link in an accurate and reliable manner between the “initial” con-
dition 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.
1. Introduction: evolution of cosmological simulations
Cosmological N -body simulations started in late 1970’s, and since then have
played an important part in describing and understanding the nonlinear gravi-
tational clustering in the universe. As far as I know, the cosmological N-body
simulation in a comoving periodic cube, which is quite conventional now, was
performed for the first time by Miyoshi Kihara (1975) usingN = 400 particles.
Figure 1 plots the evolution of the number of particles employed in cosmologi-
cal N-body simulations. Here I consider only the “high-resolution” simulations
including Particle-Particle, Particle-Particle–Particle-Mesh, and tree algorithms
which are published in refereed journals (excluding, e.g., conference proceed-
ings). I found that the evolution is well fitted by
N = 400× 100.215(Year?1975), (1)
where the amplitude is normalized to the work of Miyoshi Kihara (1975). Just
for comparison, the total number
您可能关注的文档
- PrimeScript.pdf
- Principle subspace for bosonic vertex operator $phi_{sqrt{2m}}(z)$ and Jack polynomials.pdf
- PRICING AN INSURANCE AGAINST INVESTMENT YIELD DEVIATIONS FOR ARGENTINE PENSION FUNDS BY A Q.pdf
- Printed in Great Britain. GLOBULAR DYNAMICS A CONNECTED PARTICLE SYSTEM FOR ANIMATING VISCO.pdf
- Priority-Based Multiplexing of IP-Streams onto Shared Cellular Links.pdf
- Principles and clinical implications of the brain-gut-enteric.pdf
- Probabilistic Brain Atlases of.pdf
- Pro Face gp4100工业HMI指导书.pdf
- probes in a dry-reagent strip biosensor for protein analysis. Analytical chemistry.pdf
- Probiotic yogurt in the elderly with SIBO.pdf
文档评论（0）