<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Numerical Method |</title><link>https://example.com/tags/numerical-method/</link><atom:link href="https://example.com/tags/numerical-method/index.xml" rel="self" type="application/rss+xml"/><description>Numerical Method</description><generator>HugoBlox Kit (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Sun, 01 Mar 2026 00:00:00 +0000</lastBuildDate><image><url>https://example.com/media/icon_hu_4757ff0cb9b1c124.png</url><title>Numerical Method</title><link>https://example.com/tags/numerical-method/</link></image><item><title>Smoothed particle hydrodynamics</title><link>https://example.com/research/sph-method/</link><pubDate>Sun, 01 Mar 2026 00:00:00 +0000</pubDate><guid>https://example.com/research/sph-method/</guid><description>&lt;span style="font-size:0.85em; text-align: justify;"&gt;
&lt;p&gt;Smoothed particle hydrodynamics (SPH) is a mesh-free Lagrangian particle method that represents physical quantities using a smoothing kernel and solves the hydrodynamic conservation equations for mass, momentum, and energy.
The SPH method has been widely used to model hypervelocity impacts and tidal responses of planetary bodies.
Our SPH code is publicly available at
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&lt;p&gt;&lt;strong&gt;Y. Jiao&lt;/strong&gt;, X. Yan, B. Cheng, et al. &lt;a href="https://doi.org/10.1093/mnras/stad3888" target="_blank"&gt;&lt;em&gt;SPH-DEM modeling of hypervelocity impacts on rubble-pile asteroids&lt;/em&gt;.&lt;/a&gt; Monthly Notices of the Royal Astronomical Society (2023)&lt;/p&gt;
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