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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>On the numerical simulation of propagation of micro-level inherent uncertainty for chaotic dynamic systems · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1109.0130/</link><description>Collected HN comments and submissions linking this paper.</description><language>en</language><lastBuildDate>Mon, 02 Nov 2026 11:16:22 GMT</lastBuildDate><atom:link href="https://hackerpaper.kaipfister.de/p/1109.0130/feed.xml" rel="self" type="application/rss+xml" /><item><title>On the numerical simulation of propagation of micro-level inherent uncertainty for chaotic dynamic systems — mentioned by fdej</title><link>https://news.ycombinator.com/item?id=15462177</link><guid isPermaLink="false">urn:hackerpapers:mention:1109.0130:15462177</guid><pubDate>Thu, 12 Oct 2017 23:25:25 GMT</pubDate><description>&lt;p&gt;In fact the more general N-body problem is perhaps one of the most classical uses of high order Taylor methods, in particular for studying the long term stability of the solar system. Here is a paper from 1993: http://adsabs.harvard.edu/full/1993A%26A...272..687L. Rigorous error analysis of Taylor methods for ODEs goes all the way back to Moore&amp;#x27;s original work on interval arithmetic in the 1960s; in the early 2000s Makino and Berz developed so-called Taylor models which combine rigorous error bounds with accurate long-term propagation of changes due to perturbations in the initial values (see…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1109.0130/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>nlin.CD</category></item></channel></rss>
