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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>General relativistic hydrodynamics with viscosity: contraction, catastrophic collapse, and disk formation in hypermassive neutron stars · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/astro-ph_0402502/</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/astro-ph_0402502/feed.xml" rel="self" type="application/rss+xml" /><item><title>General relativistic hydrodynamics with viscosity: contraction, catastrophic collapse, and disk formation in hypermassive neutron stars — mentioned by qubex</title><link>https://news.ycombinator.com/item?id=15987867</link><guid isPermaLink="false">urn:hackerpapers:mention:astro-ph_0402502:15987867</guid><pubDate>Fri, 22 Dec 2017 15:00:36 GMT</pubDate><description>&lt;p&gt;It wasn’t my code to link to and I probably last saw it in 1996, back in the era of dot-matrix printouts on green-and-white continuous paper (on a Windows NT 3.5 machine running FORTRAN PowerStation, if you care to commiserate). I think I can dig up the paper where the equation was published, though. EDIT: This isn&amp;#x27;t the paper I had in mind, and the equation presented is ‘merely’ relativistic, but it gives you a feel for the beast: https://arxiv.org/pdf/astro-ph/0402502.pdf (see section C).&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/astro-ph_0402502/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph</category></item></channel></rss>
