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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Physical and Geometric Interpretations of the Riemann Tensor, Ricci Tensor, and Scalar Curvature · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/gr-qc_0401099/</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/gr-qc_0401099/feed.xml" rel="self" type="application/rss+xml" /><item><title>Physical and Geometric Interpretations of the Riemann Tensor, Ricci Tensor, and Scalar Curvature — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=41934600</link><guid isPermaLink="false">urn:hackerpapers:mention:gr-qc_0401099:41934600</guid><pubDate>Thu, 24 Oct 2024 11:48:02 GMT</pubDate><description>&lt;p&gt;The area of the Sun and the Earth and every other self-gravitating body in hydrostatic equilibrium is also proportional to the body&amp;#x27;s mass. Volumes are weird though: unlike area, relativistic volume can depend on the body&amp;#x27;s (and the spacetime&amp;#x27;s) history and composition rather than just the body&amp;#x27;s mass. In general the spatial volumes inside massive bodies in curved spacetime are larger than in Euclidean-Newtonian space. The volume deviation is carried in the Ricci tensor https://en.wikipedia.org/wiki/Ricci_curvature#Direct_geometr... http://arxiv.org/pdf/gr-qc/0401099v1 (section 5.2)…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/gr-qc_0401099/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>gr-qc</category></item></channel></rss>
