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N体模拟

N体模拟是一种计算方法,用于模拟粒子系统在相互引力作用下的动力学行为。该方法源于牛顿的运动定律和万有引力定律,用于求解天体力学的基本方程。这项技术对于理解行星轨道、星团演化和宇宙结构形成至关重要。

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来源

  1. Poincaré, H. (1892). Les méthodes nouvelles de la mécanique céleste. Gauthier-Villars. link
  2. Newton, I. (1687). Philosophiæ Naturalis Principia Mathematica. Royal Society. link
  3. Aarseth, S. J. (1985). Direct methods for N-body simulations. In Multiple Time Scales (pp. 377-418). Springer. DOI: 10.1016/b978-0-12-123420-1.50017-3

如何引用本页

ScholarGate. (2026, June 3). N-Body Simulation. ScholarGate. https://scholargate.app/zh/applied-physics/n-body-simulation

Which method?

Set this method beside its closest kin and read them side by side — the library lays the books on the table; the choice is yours.

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被引用于

ScholarGateN-Body Simulation (N-Body Simulation). 于 2026-06-15 检索自 https://scholargate.app/zh/applied-physics/n-body-simulation · 数据集: https://doi.org/10.5281/zenodo.20539026