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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Thermonuclear explosions on neutron stars reveal the speed of their jets · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/2403.18135/</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/2403.18135/feed.xml" rel="self" type="application/rss+xml" /><item><title>Thermonuclear explosions on neutron stars reveal the speed of their jets — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=39888511</link><guid isPermaLink="false">urn:hackerpapers:mention:2403.18135:39888511</guid><pubDate>Sun, 31 Mar 2024 22:08:03 GMT</pubDate><description>&lt;p&gt;That seems a bit excessively nitpicky. Neither you nor the comment you corrected somewhat is really wrong. I&amp;#x27;m not sure you&amp;#x27;re much more right, though. Thomas-Fermi screening and the Coulomb crystal lattice of the outer crust isn&amp;#x27;t very plasma-like (and differs from the astrophysical plasma in the accretion disc). Perhaps it&amp;#x27;s better to say that it&amp;#x27;s a phase of matter unlike the &amp;quot;classical four&amp;quot;, and more like one of the dozens and dozens of known condensed matter states. Chamel 2007 is pretty interesting on that front: &amp;lt;https://arxiv.org/abs/0709.3798&amp;gt;. I would agree with you about the inner…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/2403.18135/"&gt;Paper and discussion history&lt;/a&gt;. A mention is not an endorsement.&lt;/p&gt;</description><category>astro-ph.HE</category></item></channel></rss>
