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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2406.09685/</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/2406.09685/feed.xml" rel="self" type="application/rss+xml" /><item><title>Indefinitely Flat Circular Velocities and the Baryonic Tully-Fisher Relation from Weak Lensing — mentioned by naasking</title><link>https://news.ycombinator.com/item?id=43741444</link><guid isPermaLink="false">urn:hackerpapers:mention:2406.09685:43741444</guid><pubDate>Sun, 20 Apr 2025 04:02:05 GMT</pubDate><description>&lt;p&gt;&amp;gt; Right now, this is the simplest solution we have that fits all observations well. It doesn&amp;#x27;t though. For instance, the latest in a litany of such failures is that rotation curves are flat past a million light years [1]. There is no plausible DM distribution that could reproduce such rotation curves while being consistent with other observations. [1] https://arxiv.org/abs/2406.09685&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2406.09685/"&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>
