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关于构建近轴对称和三轴星系模型的经验方法

On an empirical method to build near-equilibrium axisymmetric and triaxial galaxy models

Pierfrancesco Di Cintio, Alessandro Alberto Trani, Valentina Cesare

arXiv 2608.00277首次发表:更新:

AI 中文总结

该研究提出改进的绝热压缩数值技术,可从球对称自洽模型生成可控椭率的近轴对称和三轴位力化系统,用于N体模拟的非球形初始条件,经数值稳定性测试验证可行。

AI 中文摘要

我们引入一种数值技术,用于从已知相空间分布的球对称自洽模型出发,实现轴对称和三轴自引力系统的N体实现。该方法是对所谓绝热压缩技术的改进,能更好地控制粒子分布的有效椭率,生成可作为N体模拟非球形初始条件的位力化系统,文中还给出并讨论了一些数值稳定性测试。

英文摘要

We introduce a numerical technique to implement $N-$body realizations of axisymmetric and triaxial self-gravitating system starting from a spherical self-consistent models for which a phase-space distribution is known. The method is an improvement of the so-called adiabatic squeezing technique and allows one to have a better control of the effective ellipticities of the particle distribution and produces virialized systems that can be used as non-spherical initial conditions for $N-$body simulations. Some numerical stability tests are presented and discussed.

Comments16 pages, 7 figures, submitted. Comments welcome

论文原文

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