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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Cosmological Difficulties with Modified Newtonian Dynamics (or: La Fin du MOND?) · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/astro-ph_0104435/</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_0104435/feed.xml" rel="self" type="application/rss+xml" /><item><title>Cosmological Difficulties with Modified Newtonian Dynamics (or: La Fin du MOND?) — mentioned by XorNot</title><link>https://news.ycombinator.com/item?id=40740287</link><guid isPermaLink="false">urn:hackerpapers:mention:astro-ph_0104435:40740287</guid><pubDate>Thu, 20 Jun 2024 16:07:55 GMT</pubDate><description>&lt;p&gt;For one thing MOND doesn&amp;#x27;t actually appear to eliminate the need for dark matter[1]. It gets rid of ~80% of the missing mass requirement, but not all of it. Whereas pure DM can just eliminate MOND. Then you&amp;#x27;ve got the &amp;quot;Bullet Cluster&amp;quot;[2] - where two colliding galaxies have had their observable and dark matter masses apparently separated. MOND can&amp;#x27;t explain this one without a lot of tweaking, but it&amp;#x27;s pretty trivial for DM: electromagnetically interacting matter is &amp;quot;sticky&amp;quot; where as gravity only matter isn&amp;#x27;t. The Bullet Cluster shows a galaxy shaped blob of gravitational lensing exactly where…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/astro-ph_0104435/"&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>
