中文

High-resolution numerical simulations for galaxy formation

天体物理学 2007-05-23 v1

摘要

Understanding of the structure evolution in the Universe has been greatly advanced with a rapid progress in high-resolution cosmological simulations. In this contribution, we report a new set of cosmological simulations with 5123512^3 (1.4×108\sim 1.4\times 10^8) particles in a simulation box of 100\mpc100\mpc. With this unprecedented resolution, we have successfully overcomed the over-merging problem while retaining a cosmological volume size that is crucial for the statistical analysis. The simulations are being applied to studying important astrophysical problems that are sensitive to the simulation resolution.

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引用

@article{arxiv.astro-ph/0201147,
  title  = {High-resolution numerical simulations for galaxy formation},
  author = {Y. P. Jing and Yasushi Suto},
  journal= {arXiv preprint arXiv:astro-ph/0201147},
  year   = {2007}
}

备注

4 pages, observe.sty files, talk at the 5th RESCEU International Symp. on New Trends in Theoretical and Observational Cosmology (13-16 November, 2001: Tokyo, Japan)