<oai_dc:dc xmlns:oai_dc="http://www.openarchives.org/OAI/2.0/oai_dc/" xmlns:dc="http://purl.org/dc/elements/1.1/" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xsi:schemaLocation="http://www.openarchives.org/OAI/2.0/oai_dc/ http://www.openarchives.org/OAI/2.0/oai_dc.xsd">
<dc:title>Volume preserving mean curvature flow in the hyperbolic space</dc:title>
<dc:creator>Esther Cabezas-Rivas</dc:creator><dc:creator>Vicente Miquel</dc:creator>
<dc:subject>53C44</dc:subject><dc:subject>53C21</dc:subject><dc:subject>52A55</dc:subject><dc:subject>52A20</dc:subject><dc:subject>volume preserving mean curvature flow</dc:subject><dc:subject>hyperbolic space</dc:subject><dc:subject>convex by horospheres</dc:subject>
<dc:description>We prove: &quot;If $M$ is a compact hypersurface of the hyperbolic space, convex by horospheres and evolving by the volume preserving mean curvature flow, then it flows for all time, convexity by horospheres is preserved and the flow converges, exponentially, to a geodesic sphere&quot;. In addition, we show that the same conclusions about long time existence and convergence hold if $M$ is not convex by horospheres but it is close enough to a geodesic sphere.</dc:description>
<dc:publisher>Indiana University Mathematics Journal</dc:publisher>
<dc:date>2007</dc:date>
<dc:type>text</dc:type>
<dc:format>pdf</dc:format>
<dc:identifier>10.1512/iumj.2007.56.3060</dc:identifier>
<dc:source>10.1512/iumj.2007.56.3060</dc:source>
<dc:language>en</dc:language>
<dc:relation>Indiana Univ. Math. J. 56 (2007) 2061 - 2086</dc:relation>
<dc:coverage>state-of-the-art mathematics</dc:coverage>
<dc:rights>http://iumj.org/access/</dc:rights>
</oai_dc:dc>