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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>High-redshift rotation curves and MOND · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1703.06110/</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/1703.06110/feed.xml" rel="self" type="application/rss+xml" /><item><title>High-redshift rotation curves and MOND — mentioned by zackmorris</title><link>https://news.ycombinator.com/item?id=18151025</link><guid isPermaLink="false">urn:hackerpapers:mention:1703.06110:18151025</guid><pubDate>Fri, 05 Oct 2018 19:30:25 GMT</pubDate><description>&lt;p&gt;From a bit of armchair research this Friday, here are some articles on the connection between MOND and the Hubble constant: https://en.wikipedia.org/wiki/MOND https://arxiv.org/abs/1204.6359 https://arxiv.org/abs/1703.06110 http://file.scirp.org/Html/1-4500356_51478.htm https://ned.ipac.caltech.edu/level5/Sept01/Milgrom2/Milgrom3... https://academic.oup.com/mnras/article/438/2/1805/1016908 Basically what these are saying is that if the universe (and space around galaxies) is expanding, then stars would be dragged along with that expansion and move outward from the center of mass if they…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1703.06110/"&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>
