A Mini-course on EllipticâHyperbolic Equations - ICMS

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The isometric embedding problem: When can a 2-dimensionalRiemannian manifold be “seen” via a local realization in R 3 ? Thisproblem is associated with the existence of a local solution to thefully nonlinear Darboux equation. But that equation has beensuccessfully approached via Nash–Moser methods involving thelinearization(aKu x ) x+ bu yy + cKu x + du y ,where a, b > 0 and K is the Gaussian curvature of the surface.[Han, Commun. Pure Appl. Math. 58 (2005); Han and Khuri,Commun. Anal. Geom. 18 (2010)]
Given a function K (x, y) defined in a neighborhood of the origin,does there exist a graph z (x, y) having Gaussian curvature K?Because every surface may be expressed locally as a graph, this isthe problem of locally prescribing the curvature of a surface. As inthe preceding geometric problem, this problem can be reduced tothe local solvability of a Monge–Ampère equation, and in this caseas well implicit-function methods lead one to consider the linearequationu yy + ( x 2 − y 2) u xx = f .[Q. Han and M. Khuri, Calc. Var. Partial Diff. Eqs. (2012)]
Page 1 and 2: A Mini-cou
Page 3 and 4: Part I. Orientation◮ Why study th
Page 5 and 6: But, for example:◮ Separating var
Page 7 and 8: ◮ the governing equations for ide
Page 9 and 10: ◮ the Laplace-Beltrami equation o
Page 11 and 12: ◮ In certain models for plasma fl
Page 13 and 14: ◮ The relevant equation for the e
Page 15 and 16: Adopting the “differential polyno
Page 17 and 18: Example of a first-order elliptic-h
Page 19 and 20: We obtain from the first-order syst
Page 21 and 22: Geometric approach: replace the cla
Page 23 and 24: Four features of the geometric appr
Page 25 and 26: 1. Elliptic-hyperbolic continuity e
Page 27: Denote by Ω a domain of R n and co
Page 31 and 32: For most of the past century, the s
Page 33 and 34: Tricomi’s assistant Cinquini-Cibr
Page 35 and 36: M.V. Keldysh had nothing to do with
Page 37 and 38: Equations of Keldysh type can be ch
Page 39 and 40: Why do equations of Keldysh type ha
Page 41 and 42: Let ξ = K (x, y) and η = λ (x, y
Page 43 and 44: Moreover the Implicit Function Theo
Page 45 and 46: If a system of equations has the fo
Page 47 and 48: The coordinate systems (p, q) and (
Page 49 and 50: Making the substitutions p = θ x ,
Page 51 and 52: The partial hodograph transformatio
Page 53 and 54: Example for an elliptic-hyperbolic
Page 55 and 56: Because the nonlinear Lavrent’ev-
Page 57 and 58: In order to fix the boundary, we no
Page 59 and 60: Example 2: Find an L 2 solution to
Page 61 and 62: Open boundary conditions: Data are
Page 63 and 64: Geometries of canonical domains:Geo
Page 65 and 66: Ingredients:1. A one-parameter fami
Page 67 and 68: Moreover, whenever a domain is star
Page 69 and 70: Example: the cold plasma model(x
Page 71 and 72: TheoremLet Ω be star-shaped with r
Page 73 and 74: Idea of the proof: Integral variant
Page 75 and 76: If we find such a, b, and c, then w
Page 77 and 78: Suppose instead that we prove the f
Page 79:
Instead of the L 2 solution which r
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A Mini-course on EllipticâHyperbolic Equations - ICMS