Justin Corvino, Elene Karangozishvili, Deniz Ozbay
{"title":"On the index of a free-boundary minimal surface in Riemannian Schwarzschild-AdS","authors":"Justin Corvino, Elene Karangozishvili, Deniz Ozbay","doi":"10.1007/s10455-023-09925-w","DOIUrl":null,"url":null,"abstract":"<div><p>We consider the index of a certain non-compact free-boundary minimal surface with boundary on the rotationally symmetric minimal sphere in the Schwarzschild-AdS geometry with <span>\\(m>0\\)</span>. As in the Schwarzschild case, we show that in dimensions <span>\\(n\\ge 4\\)</span>, the surface is stable, whereas in dimension three, the stability depends on the value of the mass <span>\\(m>0\\)</span> and the cosmological constant <span>\\(\\Lambda <0\\)</span> via the parameter <span>\\(\\mu :=m\\sqrt{-\\Lambda /3}\\)</span>. We show that while for <span>\\(\\mu \\ge \\tfrac{5}{27}\\)</span> the surface is stable, there exist positive numbers <span>\\(\\mu _0\\)</span> and <span>\\(\\mu _1\\)</span>, with <span>\\(\\mu _1<\\tfrac{5}{27}\\)</span>, such that for <span>\\(0<\\mu <\\mu _0\\)</span>, the surface is unstable, while for all <span>\\(\\mu \\ge \\mu _1\\)</span>, the index is at most one.</p></div>","PeriodicalId":0,"journal":{"name":"","volume":null,"pages":null},"PeriodicalIF":0.0,"publicationDate":"2023-10-04","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"https://link.springer.com/content/pdf/10.1007/s10455-023-09925-w.pdf","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"","FirstCategoryId":"100","ListUrlMain":"https://link.springer.com/article/10.1007/s10455-023-09925-w","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
Abstract
We consider the index of a certain non-compact free-boundary minimal surface with boundary on the rotationally symmetric minimal sphere in the Schwarzschild-AdS geometry with \(m>0\). As in the Schwarzschild case, we show that in dimensions \(n\ge 4\), the surface is stable, whereas in dimension three, the stability depends on the value of the mass \(m>0\) and the cosmological constant \(\Lambda <0\) via the parameter \(\mu :=m\sqrt{-\Lambda /3}\). We show that while for \(\mu \ge \tfrac{5}{27}\) the surface is stable, there exist positive numbers \(\mu _0\) and \(\mu _1\), with \(\mu _1<\tfrac{5}{27}\), such that for \(0<\mu <\mu _0\), the surface is unstable, while for all \(\mu \ge \mu _1\), the index is at most one.