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The Willmore flow of Hopf-tori in the 33-sphere

Abstract

In this article the author investigates flow lines of the classical Willmore flow, which start moving in a parametrization of a Hopf-torus in S3\mathbb{S}^3. We prove that any such flow line of the Willmore flow exists globally, in particular does not develop any singularities, and subconverges to some smooth Willmore-Hopf-torus in every CmC^{m}-norm. Moreover, if in addition the Willmore-energy of the initial immersion F0F_0 is required to be smaller than the threshold 8 π338 \, \sqrt{\frac{\pi^3}{3}}, then the unique flow line of the Willmore flow, starting to move in F0F_0, converges fully to a conformal image of the standard Clifford-torus in every CmC^{m}-norm, up to time dependent, smooth reparametrizations. Key instruments for the proofs are the equivariance of the Hopf-fibration Ο€:S3β†’S2\pi:\mathbb{S}^3 \to \mathbb{S}^2 w.r.t. the effect of the L2L^2-gradient of the Willmore energy applied to smooth Hopf-tori in S3\mathbb{S}^3 and to smooth closed regular curves in S2\mathbb{S}^2, a particular version of the Lojasiewicz-Simon gradient inequality, and a certain mathematical bridge between the Euler-Lagrange equation of the elastic energy functional and a particular class of elliptic curves over C\mathbb{C}

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