High-resolution numerical simulations for galaxy formation
| dc.creator | Jing, Y. P. | |
| dc.creator | Suto, Yasushi | |
| dc.date | 2002-01-10 | |
| dc.date.accessioned | 2026-07-07T02:02:12Z | |
| dc.date.available | 2026-07-07T02:02:12Z | |
| dc.description | 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 $512^3$ ($\sim 1.4\times 10^8$) particles in a simulation box of $100\mpc$. 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. | |
| dc.description | 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) | |
| dc.identifier | https://arxiv.org/abs/astro-ph/0201147 | |
| dc.identifier | http://arxiv.org/abs/astro-ph/0201147 | |
| dc.identifier.uri | http://salesiana.dossiersoluciones.com/handle/123456789/4005 | |
| dc.subject | Astrophysics | |
| dc.title | High-resolution numerical simulations for galaxy formation | |
| dc.type | text |