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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Para-Sasakian geometry in thermodynamic fluctuation theory · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1408.5443/</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/1408.5443/feed.xml" rel="self" type="application/rss+xml" /><item><title>Para-Sasakian geometry in thermodynamic fluctuation theory — mentioned by Animats</title><link>https://news.ycombinator.com/item?id=42484627</link><guid isPermaLink="false">urn:hackerpapers:mention:1408.5443:42484627</guid><pubDate>Sun, 22 Dec 2024 05:47:13 GMT</pubDate><description>&lt;p&gt;Ambitious title. The key idea seems to come from this 1995 paper.[1] Here&amp;#x27;s a later paper.[2] None of them get far enough to tie this to real world experimental results, It&amp;#x27;s all descriptive math at this point, as the original article points out. But maybe someday someone will make further progress and understand turbulence or something. Anybody understand this? [1] https://ui.adsabs.harvard.edu/abs/1995RvMP...67..605R/abstra... [2] https://arxiv.org/pdf/1408.5443&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1408.5443/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>math-ph</category></item></channel></rss>
