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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Anomalous contribution to galactic rotation curves due to stochastic spacetime · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2402.19459/</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/2402.19459/feed.xml" rel="self" type="application/rss+xml" /><item><title>Anomalous contribution to galactic rotation curves due to stochastic spacetime — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=39725974</link><guid isPermaLink="false">urn:hackerpapers:mention:2402.19459:39725974</guid><pubDate>Sat, 16 Mar 2024 13:58:34 GMT</pubDate><description>&lt;p&gt;Sure, but the origin of this preprint is in the stochastic-classical/uncertain-quantum &amp;quot;postquantum-classical&amp;quot; theory the Oppenheim group is working on. Their theory is premised on a weakening of the gravitational interaction at short distances (it&amp;#x27;s &amp;quot;asymptotically free&amp;quot; and thus renormalizable) compared to perturbative quantum gravity (which is non-renormalizable by power counting). However, they discovered that the gravitational interaction in their theory can be too strong. More technically, in their diffusion limit they extract a different scalar potential than from GR&amp;#x27;s weak field…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2402.19459/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>gr-qc</category></item><item><title>Anomalous contribution to galactic rotation curves due to stochastic spacetime — mentioned by podiki</title><link>https://news.ycombinator.com/item?id=39723519</link><guid isPermaLink="false">urn:hackerpapers:mention:2402.19459:39723519</guid><pubDate>Sat, 16 Mar 2024 05:03:59 GMT</pubDate><description>&lt;p&gt;The article in question here is a followup to that, as a preprint and linked in this submission: &amp;quot;In a recent paper [0], which has not been peer-reviewed&amp;quot; [0] https://arxiv.org/abs/2402.19459&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2402.19459/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>gr-qc</category></item><item><title>Anomalous contribution to galactic rotation curves due to stochastic spacetime — mentioned by mdturnerphys</title><link>https://news.ycombinator.com/item?id=39723343</link><guid isPermaLink="false">urn:hackerpapers:mention:2402.19459:39723343</guid><pubDate>Sat, 16 Mar 2024 04:15:37 GMT</pubDate><description>&lt;p&gt;That&amp;#x27;s an older paper that was initially uploaded in 2018 and revised last year. The preprint under discussion is at https://arxiv.org/abs/2402.19459&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2402.19459/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>gr-qc</category></item><item><title>Anomalous contribution to galactic rotation curves due to stochastic spacetime — mentioned by willis936</title><link>https://news.ycombinator.com/item?id=39685593</link><guid isPermaLink="false">urn:hackerpapers:mention:2402.19459:39685593</guid><pubDate>Tue, 12 Mar 2024 22:15:06 GMT</pubDate><description>&lt;p&gt;Why should I? I am dedicating my life to my biggest passion, which is not cosmology. If one does commit themselves to their passion they should strive to push the field further forward, not stagnate it. It can be done. https://arxiv.org/abs/2402.19459&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2402.19459/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>gr-qc</category></item><item><title>Anomalous contribution to galactic rotation curves due to stochastic spacetime — HN submission</title><link>https://news.ycombinator.com/item?id=39650489</link><guid isPermaLink="false">urn:hackerpapers:submission:2402.19459:39650489</guid><pubDate>Sat, 09 Mar 2024 09:13:03 GMT</pubDate><description>&lt;p&gt;Anomalous contribution to galactic rotation curves due to stochastic spacetime&lt;/p&gt;&lt;p&gt;&lt;/p&gt;&lt;p&gt;143 points; 77 discussion replies on HN. &lt;a href="https://hackerpaper.kaipfister.de/p/2402.19459/"&gt;Paper and source history&lt;/a&gt;. A submission is not an endorsement.&lt;/p&gt;</description><category>gr-qc</category></item></channel></rss>
