Volume-preserving mean curvature flow of revolution hypersurfaces in a Rotationally Symmetric Space

Abstract

In an ambient space with rotational symmetry around an axis (which include the Hyperbolic and Euclidean spaces), we study the evolution under the volume-preserving mean curvature flow of a revolution hypersurface M generated by a graph over the axis of revolution and with boundary in two totally geodesic hypersurfaces (tgh for short). Requiring that, for each time t, the evolving hypersurface Mt meets such tgh ortogonally, we prove that: a) the flow exists while Mt does not touch the axis of rotation; b) throughout the time interval of existence, b1) the generating curve of Mt remains a graph, and b2) the averaged mean curvature is double side bounded by positive constants; c) the singularity set (if non-empty) is finite and discrete along the axis; d) under a suitable hypothesis relating the enclosed volume to the n-volume of M, we achieve long time existence and convergence to a revolution hypersurface of constant mean curvature.

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