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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1904.06759/</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/1904.06759/feed.xml" rel="self" type="application/rss+xml" /><item><title>Relativistic Shapiro delay measurements of an extremely massive millisecond pulsar — mentioned by SiempreViernes</title><link>https://news.ycombinator.com/item?id=20993653</link><guid isPermaLink="false">urn:hackerpapers:mention:1904.06759:20993653</guid><pubDate>Tue, 17 Sep 2019 11:10:21 GMT</pubDate><description>&lt;p&gt;Seems the PR people got the most important figure wrong, the measured mass is 2.14 +0.1 -0.09 M_sun, as per the preprint (and nature abstract[1]): https://arxiv.org/abs/1904.06759 The 2.17 M_sun figure is instead the hypothesised upper limit on the neutron star mass, derived from the equations of state that survive recent LIGO observations. [1]: https://www.nature.com/articles/s41550-019-0880-2&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1904.06759/"&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>
