<?xml version="1.0" encoding="utf-8" standalone="yes"?><rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Few-Body Dynamics | Yihan Wang (王艺涵)</title><link>https://yihanwangastro.github.io/tag/few-body-dynamics/</link><atom:link href="https://yihanwangastro.github.io/tag/few-body-dynamics/index.xml" rel="self" type="application/rss+xml"/><description>Few-Body Dynamics</description><generator>Hugo Blox Builder (https://hugoblox.com)</generator><language>en-us</language><lastBuildDate>Sat, 01 May 2021 00:00:00 +0000</lastBuildDate><image><url>https://yihanwangastro.github.io/media/icon_hu_5f4ae6b6057760e0.png</url><title>Few-Body Dynamics</title><link>https://yihanwangastro.github.io/tag/few-body-dynamics/</link></image><item><title>SpaceHub</title><link>https://yihanwangastro.github.io/project/spacehub/</link><pubDate>Sat, 01 May 2021 00:00:00 +0000</pubDate><guid>https://yihanwangastro.github.io/project/spacehub/</guid><description>&lt;p>SpaceHub is a state-of-the-art few-body gravity integration toolkit built in C++. It implements Algorithmic Regularization (AR) and symplectic integrators to handle scenarios that break conventional codes:&lt;/p>
&lt;div class="highlight">&lt;pre tabindex="0" class="chroma">&lt;code class="language-fallback" data-lang="fallback">&lt;span class="line">&lt;span class="cl">$ spacehub --status
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">┌─────────────────────────────────────────────┐
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">│ SpaceHub v1.0 │
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">│ Extreme mass ratios ✓ │
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">│ High eccentricities ✓ │
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">│ Close encounters ✓ │
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">│ Round-off error control ✓ │
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">│ Long-term integration ✓ │
&lt;/span>&lt;/span>&lt;span class="line">&lt;span class="cl">└─────────────────────────────────────────────┘
&lt;/span>&lt;/span>&lt;/code>&lt;/pre>&lt;/div>&lt;p>&lt;strong>Key Features:&lt;/strong>&lt;/p>
&lt;ul>
&lt;li>Algorithmic Regularization for extreme mass ratios (e.g., SMBH + stellar-mass objects)&lt;/li>
&lt;li>Symplectic integrators ensuring time-reversibility&lt;/li>
&lt;li>Rigorous round-off error control for long-term orbital evolution&lt;/li>
&lt;li>Easy-to-use API designed for community adoption&lt;/li>
&lt;li>Applications: SMBH binaries, planetary system evolution, chaotic star clusters&lt;/li>
&lt;/ul>
&lt;p>&lt;strong>Publication:&lt;/strong> Wang et al. (2021), MNRAS, 505, 1053&lt;/p></description></item></channel></rss>