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arXiv 1503.03869physics.comp-phastro-ph.COastro-ph.IMphysics.flu-dyn
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非线性薛定谔方程的光滑粒子流体力学数值解

Numerical solution of the non-linear Schrodinger equation using smoothed-particle hydrodynamics

Philip Mocz, Sauro Succi

摘要:

我们制定了一个光滑粒子流体动力学数值方法,传统上用于欧拉方程的流体动力学在天体物理模拟的背景下,解决非线性薛定谔方程的马德隆制定。波函数的概率密度被离散为运动粒子,其性质通过核函数平滑。传统的流体压力被取代的量子压力张量,一个新的,强大的离散found. We展示了我们的数值方法上的各种数值测试问题,涉及简谐振子,玻色-爱因斯坦凝聚体,坍缩奇点,和暗物质晕由Gross-Pitaevskii-Poisson方程。我们的方法是保守的,适用于无界域,并自动适应其分辨率,使其非常适合研究问题的崩溃解决方案。

英文摘要:

We formulate a smoothed-particle hydrodynamics numerical method, traditionally used for the Euler equations for fluid dynamics in the context of astrophysical simulations, to solve the non-linear Schrodinger equation in the Madelung formulation. The probability density of the wavefunction is discretized into moving particles, whose properties are smoothed by a kernel function. The traditional fluid pressure is replaced by a quantum pressure tensor, for which a novel, robust discretization is found. We demonstrate our numerical method on a variety of numerical test problems involving the simple harmonic oscillator, Bose-Einstein condensates, collapsing singularities, and dark matter halos governed by the Gross-Pitaevskii-Poisson equation. Our method is conservative, applicable to unbounded domains, and is automatically adaptive in its resolution, making it well suited to study problems with collapsing solutions.

机构、总结、中文摘要均由AI分析而来,可能存在错误,请以论文正文为准。

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