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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/1711.07597/</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/1711.07597/feed.xml" rel="self" type="application/rss+xml" /><item><title>Global Nonlinear Stability of Schwarzschild Spacetime under Polarized Perturbations — mentioned by raattgift</title><link>https://news.ycombinator.com/item?id=16592511</link><guid isPermaLink="false">urn:hackerpapers:mention:1711.07597:16592511</guid><pubDate>Thu, 15 Mar 2018 13:16:44 GMT</pubDate><description>&lt;p&gt;&amp;gt; where do we get a black hole to poke As qubex suggests, this is really about confirming that asymptotically Schwarzschild spacetime (and its close relatives) is mathematically robust [1]. Asymptotically here means that if we perturb (gravitationally or electromagnetically) a Schwarzschild black hole the resulting radiation from &amp;quot;balding&amp;quot; will decay exponentially fast and die off to ground state well before spatial infinity. This is also a useful check on practices like (in cosmology) taking a boundary at some reasonable radius from a galaxy as if it were asymptotically Schwarzschild space…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/1711.07597/"&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>
