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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Three Dimensional Evolution to Core Collapse of a Massive Star · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1503.02199/</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/1503.02199/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Three Dimensional Evolution to Core Collapse of a Massive Star — mentioned by magicalhippo</title><link>https://news.ycombinator.com/item?id=25929402</link><guid isPermaLink="false">urn:hackerpapers:mention:1503.02199:25929402</guid><pubDate>Wed, 27 Jan 2021 15:32:20 GMT</pubDate><description>&lt;p&gt;As far as I can determine, this[1] is an older video from the paper[2] linked in the article, showing the first hundred milliseconds. Also found this[3] presentation by Adam Burrows, also mentioned in the article, giving an overview on the 3D simulations compared to the older 1D and 2D simulations. [1]: https://www.youtube.com/watch?v=oxGajNoPz8c [2]: https://arxiv.org/abs/1503.02199 [3]: https://www.youtube.com/watch?v=ZDk5AzmNCCk&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1503.02199/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.HE</category></item></channel></rss>
