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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Entropy of the Gravitational Field · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/gr-qc_9208009/</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_9208009/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Entropy of the Gravitational Field — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=36181174</link><guid isPermaLink="false">urn:hackerpapers:mention:gr-qc_9208009:36181174</guid><pubDate>Sat, 03 Jun 2023 22:36:23 GMT</pubDate><description>&lt;p&gt;Sorry, assume I&amp;#x27;ve read standard textbooks and Ellis-Maartens-Mccallum, and explain to me how inflation controls the spatially flat FLRW chart density of low-entropy fluctuations in the quasi de Sitter +CC phase (ideally beginning with the &amp;quot;dark era&amp;quot;, or even the earlier black hole era if you want to deal in nonequilibrium entropy explicitly, rather than just assuming heat death). (I don&amp;#x27;t know where you got &amp;quot;14b.y.&amp;quot; from; we still have the local group (including Milkdromeda) making new stars that soon from now; it&amp;#x27;s a cosmological eyeblink). &amp;gt; This is barely anything beyond inflation, it…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/gr-qc_9208009/"&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>
