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<rss version="2.0" xmlns:atom="http://www.w3.org/2005/Atom"><channel><title>The Kerr spacetime: A brief introduction · HackerPapers discussions</title><link>https://hackerpaper.kaipfister.de/p/0706.0622/</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/0706.0622/feed.xml" rel="self" type="application/rss+xml" /><item><title>The Kerr spacetime: A brief introduction — mentioned by itishappy</title><link>https://news.ycombinator.com/item?id=44565698</link><guid isPermaLink="false">urn:hackerpapers:mention:0706.0622:44565698</guid><pubDate>Mon, 14 Jul 2025 21:44:47 GMT</pubDate><description>&lt;p&gt;It&amp;#x27;s only spherical in a Schwarzschild (non-rotating) black hole. A rotating black hole is called a Kerr black hole, and stuff gets weird, such as there being an oblate event horizon, a weird outer horizon called an ergosphere where spacetime gets dragged along such that it&amp;#x27;s impossible to stand still and you can accelerate objects using the black hole, a weirder inner horizon called the Cauchy horizon where time travel is possible, and a singularity in the shape of a ring. Your intuition is correct that during a merger it would be weirder still. https://en.wikipedia.org/wiki/Kerr_metric…&lt;/p&gt;&lt;p&gt;&lt;a href="https://hackerpaper.kaipfister.de/p/0706.0622/"&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>
