2010
DOI: 10.1007/s00208-010-0550-2
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Foliations of asymptotically flat manifolds by surfaces of Willmore type

Abstract: The goal of this paper is to establish the existence of a foliation of the asymptotic region of an asymptotically flat manifold with nonzero mass by surfaces which are critical points of the Willmore functional subject to an area constraint. Equivalently these surfaces are critical points of the Geroch-Hawking mass. Thus our result has applications in the theory of General Relativity

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Cited by 49 publications
(82 citation statements)
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“…Such manifolds were called asymptotically Schwarzschild in [LMS11] and we will adopt this terminology from now on. The Schwarzschild manifold (M S , g S ) = (R 3 \ {0}, g S ) is the model space for the problem studied in this paper.…”
Section: Preliminariesmentioning
confidence: 99%
See 1 more Smart Citation
“…Such manifolds were called asymptotically Schwarzschild in [LMS11] and we will adopt this terminology from now on. The Schwarzschild manifold (M S , g S ) = (R 3 \ {0}, g S ) is the model space for the problem studied in this paper.…”
Section: Preliminariesmentioning
confidence: 99%
“…Hence, the problem of maximizing the Hawking mass even with fixed area seems particularly challenging from a variational point of view. In this work we make partial progress in understanding the role of the centred spheres in the Schwarzschild space or more generally of the leaves Σ λ in the foliation constructed in [LMS11] in asymptotically Schwarzschild spaces regarding the maximization of the Hawking mass. In fact, we show the following: Theorem 1.2.…”
Section: Introductionmentioning
confidence: 99%
“…We have then the following formulas, see Section 3 in . Proposition With the above notation we have the formulas Wfalse(i(Σ)false)false[φfalse]=normalΣLH+12H3φdσand truerightW(ifalse(normalΣfalse))[φ,φ]=left2Σ[](Lφ)2+12H2|φ|22A˚false(φ,φfalse)dσleft+0.16em2Σφ2false(false|Hfalse|g2+2ϖ(H)+HH+2g(2H,A˚)+2H2false|trueA˚false|g2left+0.16em2Hg(A˚,T)Hg(n Ric )(n,n)12H2false|Afalse|g212H2 Ric (n,n)false)dσleft+0.16emΣ()LH+12H3()φ…”
Section: Preliminariesmentioning
confidence: 99%
“…Let us recall that area‐constrained Willmore surfaces satisfy the equation normalΔtrueg¯H+H|A˚|2+H Ric false(n,nfalse)=λH,for some λR playing the role of Lagrange multiplier. These immersions are naturally linked to the Hawking mass mHfalse(ifalse):=Areafalse(ifalse)64π3/216πWfalse(ifalse),since, clearly, the critical points of the Hawking mass under area constraint are exactly the area‐constrained Willmore immersions (see and the references therein for more material about the Hawking mass).…”
Section: Introductionmentioning
confidence: 99%
“…In more generality, it is interesting to study the minimization problems associated to integral functionals depending on the curvatures of the type introduced by Willmore (see [33]) and studied in the euclidean space (see for instance the works of Simon [27], Kuwert and Schätzle [12], Rivière [30]) or in Riemannian manifolds (see, for example, [13], [21] and [22]). …”
Section: Introductionmentioning
confidence: 99%