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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Nuclear Equation of State and Neutron Star Masses · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1305.3510/</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/1305.3510/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Nuclear Equation of State and Neutron Star Masses — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=11181199</link><guid isPermaLink="false">urn:hackerpapers:mention:1305.3510:11181199</guid><pubDate>Fri, 26 Feb 2016 13:23:20 GMT</pubDate><description>&lt;p&gt;It gets a bit more complicated than that. Matt Strassler has a couple relevant articles on his blog site. The first goes deeper than the 3-quark simplification. &amp;quot;What&amp;#x27;s a proton? First and foremost, it’s a mess. A total mess&amp;quot; http://profmattstrassler.com/articles-and-posts/largehadronc... The second digs into both protons and neutrons &amp;quot;So there are reasons to go further and describe things as I have elsewhere on this website: a proton is made from three quarks (two up quarks and a down quark), lots of gluons, and lots of quark-antiquark pairs (mostly up quarks and down quarks, but also even a…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1305.3510/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>nucl-th</category></item></channel></rss>
