| 注册
首页|期刊导航|天文学进展|平滑粒子流体动力学(SPH)数值模拟中的重子物理

平滑粒子流体动力学(SPH)数值模拟中的重子物理

姜春艳

天文学进展2012,Vol.30Issue(3):334-345,12.
天文学进展2012,Vol.30Issue(3):334-345,12.

平滑粒子流体动力学(SPH)数值模拟中的重子物理

Baryonic Physics in Cosmological Smoothed Particle Hydrodynamics Simulations

姜春艳1

作者信息

  • 1. 中国科学院上海天文台星系与宇宙学重点实验室,上海200030
  • 折叠

摘要

Abstract

The smoothed particle hydrodynamics (SPH) simulation is a powerful tool in studying galaxy formation and evolution. In this review, standard formulation of SPH is summarized. And then the implementation of baryonic physics in cosmological SPH simulations are illustrated, including star formation, galactic wind feedback, AGN feedback, and thermal conduction. uring the past years, much progress has been made on improving the physical modeling in hydro dynamical simulations, by nvoking more sophisticated treatments of star formation, supernovae feedback, AGN feedback and so on. The implementation of these baryonic physics in SPH simulations has helped us a lot in understanding how galaxies form and evolve in the universe. However, due to our limited knowledge of these baryonic physics, these models, are still far from being perfect. Many further studies are therefore needed in future to improve these physical modeling in simulations.

关键词

流体数值模拟/重子物理/恒星形成

Key words

SPH simulation/ baryonic physics/ stellar evolution

分类

天文与地球科学

引用本文复制引用

姜春艳..平滑粒子流体动力学(SPH)数值模拟中的重子物理[J].天文学进展,2012,30(3):334-345,12.

基金项目

国家自然科学基金(11003035) (11003035)

天文学进展

OA北大核心CSCDCSTPCD

1000-8349

访问量0
|
下载量0
段落导航相关论文