捕捉冲击和接触不连续性的新型流体力学方案以及与现有方法的比较研究

IF 1.9 4区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Takuhiro Yuasa , Masao Mori
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引用次数: 0

摘要

我们提出了一种名为 "戈杜诺夫密度无关平滑粒子流体力学(GDISPH)"的新流体力学方案,无需手动调整参数即可准确处理冲击波和接触不连续性。这与标准的平滑粒子流体力学(SSPH)形成了鲜明对比,后者需要人工粘度项参数来处理冲击波,并且由于非物理排斥力导致的表面张力破坏了压力平衡并抑制了流体不稳定性,因而难以准确处理接触不连续性。虽然戈杜诺夫 SPH(GSPH)可以通过使用黎曼求解器的解来处理无参数冲击,但仍无法完全处理接触不连续性。与密度无关的平滑粒子流体力学(DISPH)是为比 SSPH 更有效地处理接触不连续性而提出的几种方案之一,它在我们涉及强冲击和接触不连续性的测试中表现出更优越的性能。然而,DISPH 仍然需要人工粘度项。我们通过几种方法将黎曼求解器集成到 DISPH 中,得到了 GDISPH 的一些模式。一维黎曼问题、压力平衡、Sedov-Taylor 和 Kelvin-Helmholtz 等标准测试的结果均有利于 GDISPH 案例 1 和 GDISPH 案例 2 以及 DISPH。我们的结论是,GDISPH 案例 1 比 GDISPH 案例 2 更好地处理了冲击和接触不连续性问题,而无需特定参数或引入任何额外的数值扩散。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Novel hydrodynamic schemes capturing shocks and contact discontinuities and comparison study with existing methods

We present a new hydrodynamic scheme named Godunov Density-Independent Smoothed Particle Hydrodynamics (GDISPH), that can accurately handle shock waves and contact discontinuities without any manually tuned parameters. This is in contrast to the standard formulation of smoothed particle hydrodynamics (SSPH), which requires the parameters for an artificial viscosity term to handle the shocks and struggles to accurately handle the contact discontinuities due to unphysical repulsive forces, resulting in surface tension that disrupts pressure equilibrium and suppresses fluid instabilities. While Godunov SPH (GSPH) can handle the shocks without the parameters by using solutions from a Riemann solver, it still cannot fully handle the contact discontinuities. Density-Independent Smoothed Particle Hydrodynamics (DISPH), one of several schemes proposed to handle contact discontinuities more effectively than SSPH, demonstrates superior performance in our tests involving strong shocks and contact discontinuities. However, DISPH still requires the artificial viscosity term. We integrate the Riemann solver into DISPH in several ways, yielding some patterns of GDISPH. The results of standard tests such as the one-dimensional Riemann problem, pressure equilibrium, Sedov–Taylor, and Kelvin–Helmholtz tests are favourable to GDISPH Case 1 and GDISPH Case 2, as well as DISPH. We conclude that GDISPH Case 1 has an advantage over GDISPH Case 2effectively handling shocks and contact discontinuities without the need for specific parameters or introducing any additional numerical diffusion.

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来源期刊
New Astronomy
New Astronomy 地学天文-天文与天体物理
CiteScore
4.00
自引率
10.00%
发文量
109
审稿时长
13.6 weeks
期刊介绍: New Astronomy publishes articles in all fields of astronomy and astrophysics, with a particular focus on computational astronomy: mathematical and astronomy techniques and methodology, simulations, modelling and numerical results and computational techniques in instrumentation. New Astronomy includes full length research articles and review articles. The journal covers solar, stellar, galactic and extragalactic astronomy and astrophysics. It reports on original research in all wavelength bands, ranging from radio to gamma-ray.
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