<?xml version="1.0" encoding="UTF-8"?>
<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817 · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1710.05938/</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/1710.05938/feed.xml" rel="self" type="application/rss+xml" /><item><title>Constraining the Maximum Mass of Neutron Stars From Multi-Messenger Observations of GW170817 — mentioned by 4ad</title><link>https://news.ycombinator.com/item?id=16483954</link><guid isPermaLink="false">urn:hackerpapers:mention:1710.05938:16483954</guid><pubDate>Wed, 28 Feb 2018 16:18:13 GMT</pubDate><description>&lt;p&gt;This is not correct, the nature of gravitational waves emitted by the merging of two objects is different in its final stage, depending whether the objects form a black hole or not. Until a black hole is formed, the nature of the emission is the same for all objects (e.g. black holes or neutron stars), but if a black hole forms, the final emission (ringdown) is different. The first LIGO-Virgo events detected black hole mergers which resulted in black holes. The last LIGO-Virgo event detected two neutron star mergers. Unfortunately the sensitivity of the apparatus is not good enough to…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1710.05938/"&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>
