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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Galactic Dynamics via General Relativity: A Compilation and New Developments · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/astro-ph_0610370/</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_0610370/feed.xml" rel="self" type="application/rss+xml" /><item><title>Galactic Dynamics via General Relativity: A Compilation and New Developments — mentioned by cygx</title><link>https://news.ycombinator.com/item?id=26442790</link><guid isPermaLink="false">urn:hackerpapers:mention:astro-ph_0610370:26442790</guid><pubDate>Sat, 13 Mar 2021 00:45:40 GMT</pubDate><description>&lt;p&gt;That&amp;#x27;s the wrong paragraph to cite. The parts relevant to Cooperstock&amp;#x27;s (and similar) work is this: &amp;gt; Although filled with controversy, the studies of the galactic rotation via general relativity [16,17,18] reach the same basic conclusion of the present paper. Namely, the dragging effect of a gravitomagnetic component (time-space component of the metric) explains the flat rotation curve at large distances, without the recourse to dark matter. The main problem with the general relativistic models is the very limited number of exact solutions of the Einstein field equations [...] &amp;gt; The…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/astro-ph_0610370/"&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>
