Download Affine Bernstein Problems and Monge-Ampère Equations by An-Min Li, Ruiwei Xu, Udo Simon, Fang Jia PDF

By An-Min Li, Ruiwei Xu, Udo Simon, Fang Jia

During this monograph, the interaction among geometry and partial differential equations (PDEs) is of specific curiosity. It offers a selfcontained advent to investigate within the final decade bearing on worldwide difficulties within the thought of submanifolds, resulting in a few forms of Monge-Ampère equations. From the methodical standpoint, it introduces the answer of definite Monge-Ampère equations through geometric modeling thoughts. the following geometric modeling capability the best collection of a normalization and its caused geometry on a hypersurface outlined through an area strongly convex worldwide graph. For a greater knowing of the modeling ideas, the authors provide a selfcontained precis of relative hypersurface concept, they derive vital PDEs (e.g. affine spheres, affine maximal surfaces, and the affine consistent suggest curvature equation). relating modeling concepts, emphasis is on conscientiously based proofs and exemplary comparisons among assorted modelings.

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Example text

4) states the Weingarten equation for Y . 2 Affine shape operator and affine extrinsic curvature For a hypersurface in Euclidean space the Weingarten equation for the unit normal implicitly defines the Euclidean shape or Weingarten operator; from this we get the extrinsic curvature functions. 4) states that dY (v) is tangential to x(M ) for any v ∈ Tp M . This situation suggests to search for an affine analogue of the Euclidean Weingarten operator. Let x; e1 , ···, en , en+1 be an equiaffine frame on M .

4) We will frequently need condition (c) in the apolarity condition above for explicit calculations. Equiaffine frames. From now on we shall choose an adapted frame field {x; e1 , ···, en , en+1 } such that en+1 is parallel to Y . We call such a frame an equiaffine frame; so an equiaffine frame has the three properties: (i) it is unimodular, (ii) e1 , · · ·, en are tangential, (iii) en+1 is parallel to the affine normal vector Y . This choice implies the apolarity condition and 1 Y = |H| n+2 en+1 .

We define the relative Tchebychev form T as the trace of a linear mapping by nT (v) := tr{w → A(w, v)} and the associated relative Tchebychev vector field T by h(T, v) := T (v) for all tangent fields v. One can easily show that the one-form T is closed and thus T is the gradient of a potential function. Relative structure equations in covariant local notation. We rewrite the structure equations in terms of h-covariant differentiation and with affinely invariant coefficients as follows: Gauß equation for x : Akij xk + hij Y.

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