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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Galactic Mass-to-Light Ratios With Superfluid Dark Matter · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2201.07282/</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/2201.07282/feed.xml" rel="self" type="application/rss+xml" /><item><title>Galactic Mass-to-Light Ratios With Superfluid Dark Matter — mentioned by naasking</title><link>https://news.ycombinator.com/item?id=33275319</link><guid isPermaLink="false">urn:hackerpapers:mention:2201.07282:33275319</guid><pubDate>Thu, 20 Oct 2022 14:34:39 GMT</pubDate><description>&lt;p&gt;&amp;gt; My guess would be something about the dynamics of dark matter in galaxy evolution pushes the distribution into a shape that produces those mathematically simple rotation curves. That seems Occam&amp;#x27;s-razor compliant to me; It&amp;#x27;s not just rotation curves, there are numerous validated predictions MOND makes based only on the visible matter (see the paper at the bottom). These would all be a set of remarkable coincidences if the current CDM model were true. &amp;gt; it would be weird if rotation curves with dark matter were really complicated and unpredictable. It&amp;#x27;s also possible that both MOND and LCDM…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2201.07282/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.GA</category></item></channel></rss>
