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20022015
most citedSpacelike spherically symmetric CMC foliation in the extended Schwarzschild spacetime

8 citations · 29 across the 11 of their papers we have counts for

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math.DG2015★ 8 cited

Spacelike spherically symmetric CMC foliation in the extended Schwarzschild spacetime

Kuo-Wei Lee, Yng-Ing Lee

We first summarize the characterization of smooth spacelike spherically symmetric constant mean curvature (SS-CMC) hypersurfaces in the Schwarzschild spacetime and Kruskal extensio…

math.DG2012★ 4 cited

The Stability of Self-Shrinkers of Mean Curvature Flow in Higher Codimension

Yng-Ing Lee, Yang-Kai Lue

In this paper, we generalize Colding and Minicozzi's work \cite{CM} on the stability of self-shrinkers in the hypersurface case to higher co-dimensional cases. The first and second…

math.DG2011★ 5 cited

Spacelike spherically symmetric CMC hypersurfaces in Schwarzschild spacetimes (I): Construction

Kuo-Wei Lee, Yng-Ing Lee

We solve spacelike spherically symmetric constant mean curvature (SS-CMC) hypersurfaces in Schwarzschild spacetimes and analyze their asymptotic behavior near the coordinate singul…

math.DG2010★ 7 cited

Generalized -harmonic Equation and The Inverse Mean Curvature Flow

Yng-Ing Lee, Ai-Nung Wang, Shihshu Walter Wei

We introduce and study generalized -harmonic equations (1.1). Using some ideas and techniques in studying -harmonic functions from [W1] (2007), and in studying nonhomogeneous…

math.DG2010

The existence of Hamiltonian stationary Lagrangian tori in Kahler manifolds of any dimension

Yng-Ing Lee

Hamiltonian stationary Lagrangians are Lagrangian submanifolds that are critical points of the volume functional under Hamiltonian deformations. They can be considered as a general…

math.DG2009★ 1 cited

On the existence of Hamiltonian stationary Lagrangian submanifolds in symplectic manifolds

Dominic Joyce, Yng-Ing Lee, Richard Schoen

Let (M,w) be a compact symplectic 2n-manifold, and g a Riemannian metric on M compatible with w. For instance, g could be Kahler, with Kahler form w. Consider compact Lagrangian su…