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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Galactic rotation curves in conformal gravity · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1211.0188/</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/1211.0188/feed.xml" rel="self" type="application/rss+xml" /><item><title>Galactic rotation curves in conformal gravity — mentioned by cygx</title><link>https://news.ycombinator.com/item?id=25500268</link><guid isPermaLink="false">urn:hackerpapers:mention:1211.0188:25500268</guid><pubDate>Mon, 21 Dec 2020 22:15:09 GMT</pubDate><description>&lt;p&gt;There&amp;#x27;s conformal gravity, which replaces the Einstein field equations with ones derived from a conformally invariant action. Like MOND, this allows you to fit rotation curves nicely without invoking dark matter, see eg [1][2]. [1] https://arxiv.org/abs/1211.0188 (2012) [2] https://arxiv.org/abs/1812.03152v3 (2018)&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1211.0188/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.CO</category></item></channel></rss>
