Perturbations of singular solutions to Gelfand s problem p.1

Similar documents
On Schrödinger equations with inverse-square singular potentials

Integro-differential equations: Regularity theory and Pohozaev identities

Non-homogeneous semilinear elliptic equations involving critical Sobolev exponent

Regularity of stable solutions of a Lane-Emden type system

Extremal Solutions and Instantaneous Complete Blow-up for Elliptic and Parabolic Problems

Heat equations with singular potentials: Hardy & Carleman inequalities, well-posedness & control

Exact solutions of Bratu and Liouville equations

Blow-up solutions for critical Trudinger-Moser equations in R 2

Liouville theorems for stable Lane-Emden systems and biharmonic problems

Hardy inequalities, heat kernels and wave propagation

A simplified proof of a conjecture for the perturbed Gelfand equation from combustion theory

Ciudad Universitaria C.P., México D.F., México b Departamento de Ingeniería Matemática and CMM, Universidad de Chile, Santiago, Chile

Stationary Kirchhoff equations with powers by Emmanuel Hebey (Université de Cergy-Pontoise)

The Liouville^Bratu^Gelfand Problem for Radial Operators

Partial Differential Equations

Microlocal Methods in X-ray Tomography

Hardy Rellich inequalities with boundary remainder terms and applications

Exit times of diffusions with incompressible drifts

Analysis in weighted spaces : preliminary version

A global solution curve for a class of free boundary value problems arising in plasma physics

arxiv: v1 [math.ap] 16 Jan 2015

A non-local critical problem involving the fractional Laplacian operator

Recent result on porous medium equations with nonlocal pressure

NONLINEAR FREDHOLM ALTERNATIVE FOR THE p-laplacian UNDER NONHOMOGENEOUS NEUMANN BOUNDARY CONDITION

Existence of Positive Solutions to Semilinear Elliptic Systems Involving Concave and Convex Nonlinearities

The critical dimension for a fourth order elliptic problem with singular nonlinearity

Symmetry breaking in Caffarelli-Kohn-Nirenberg inequalities

Rigidity Results for Elliptic PDEs

Global unbounded solutions of the Fujita equation in the intermediate range

A VARIATIONAL INEQUALITY RELATED TO AN ELLIPTIC OPERATOR

On semilinear elliptic equations with measure data

Symmetry and symmetry breaking of extremal functions in some interpolation inequalities: an overview

NONHOMOGENEOUS ELLIPTIC EQUATIONS INVOLVING CRITICAL SOBOLEV EXPONENT AND WEIGHT

Regularity estimates for the solution and the free boundary of the obstacle problem for the fractional Laplacian

NONLOCAL DIFFUSION EQUATIONS

Lecture I.: (Simple) Basic Variational and Topological Methods (an introductory lecture for graduate students and postdocs)

NONLINEAR SCHRÖDINGER ELLIPTIC SYSTEMS INVOLVING EXPONENTIAL CRITICAL GROWTH IN R Introduction

Exit times of diffusions with incompressible drift

MULTIPLE SOLUTIONS FOR CRITICAL ELLIPTIC PROBLEMS WITH FRACTIONAL LAPLACIAN

New exact multiplicity results with an application to a population model

Math The Laplacian. 1 Green s Identities, Fundamental Solution

1. Introduction This paper is devoted to the study of the regularity of stable solutions to the semilinear. u = 0 in R n (1.2)

On the shape of solutions to the Extended Fisher-Kolmogorov equation

Minimization problems on the Hardy-Sobolev inequality

Sobolev Spaces. Chapter 10

COMBINED EFFECTS FOR A STATIONARY PROBLEM WITH INDEFINITE NONLINEARITIES AND LACK OF COMPACTNESS

ON NONHOMOGENEOUS BIHARMONIC EQUATIONS INVOLVING CRITICAL SOBOLEV EXPONENT

Entropy-dissipation methods I: Fokker-Planck equations

Frequency functions, monotonicity formulas, and the thin obstacle problem

EIGENVALUE QUESTIONS ON SOME QUASILINEAR ELLIPTIC PROBLEMS. lim u(x) = 0, (1.2)

Week 6 Notes, Math 865, Tanveer

A CONVEX-CONCAVE ELLIPTIC PROBLEM WITH A PARAMETER ON THE BOUNDARY CONDITION

SYMMETRY RESULTS FOR PERTURBED PROBLEMS AND RELATED QUESTIONS. Massimo Grosi Filomena Pacella S. L. Yadava. 1. Introduction

Robustness for a Liouville type theorem in exterior domains

Fourier Transform & Sobolev Spaces

INFINITELY MANY POSITIVE SOLUTIONS OF NONLINEAR SCHRÖDINGER EQUATIONS WITH NON-SYMMETRIC POTENTIALS

On Chern-Simons-Schrödinger equations including a vortex point

On non negative solutions of some quasilinear elliptic inequalities

On some weighted fractional porous media equations

THE WAVE EQUATION. d = 1: D Alembert s formula We begin with the initial value problem in 1 space dimension { u = utt u xx = 0, in (0, ) R, (2)

Three equations with exponential nonlinearities

NONLINEAR ELLIPTIC EQUATIONS WITH MEASURES REVISITED

Math 46, Applied Math (Spring 2009): Final

Wiener Measure and Brownian Motion

ON SERRIN S OVERDETERMINED PROBLEM AND A CONJECTURE OF BERESTYCKI, CAFFARELLI AND NIRENBERG

p-laplacian problems with critical Sobolev exponents

Nonexistence of solutions for quasilinear elliptic equations with p-growth in the gradient

Nonlinear and Nonlocal Degenerate Diffusions on Bounded Domains

Fifth Abel Conference : Celebrating the Mathematical Impact of John F. Nash Jr. and Louis Nirenberg

On the structure of Hardy Sobolev Maz ya inequalities

Numerical methods for a fractional diffusion/anti-diffusion equation

PERTURBATION RESULTS OF CRITICAL ELLIPTIC EQUATIONS OF CAFFARELLI-KOHN-NIRENBERG TYPE

Inverse Scattering with Partial data on Asymptotically Hyperbolic Manifolds

SEMILINEAR ELLIPTIC EQUATIONS WITH DEPENDENCE ON THE GRADIENT

EXISTENCE OF SOLUTIONS FOR CROSS CRITICAL EXPONENTIAL N-LAPLACIAN SYSTEMS

TOPICS IN NONLINEAR ANALYSIS AND APPLICATIONS. Dipartimento di Matematica e Applicazioni Università di Milano Bicocca March 15-16, 2017

MATH 126 FINAL EXAM. Name:

Nonlinear Analysis. Global solution curves for boundary value problems, with linear part at resonance

ON THE FRACTIONAL CAUCHY PROBLEM ASSOCIATED WITH A FELLER SEMIGROUP

HARDY INEQUALITIES WITH BOUNDARY TERMS. x 2 dx u 2 dx. (1.2) u 2 = u 2 dx.

Nonlinear elliptic systems with exponential nonlinearities

Bielefeld Course on Nonlinear Waves - June 29, Department of Mathematics University of North Carolina, Chapel Hill. Solitons on Manifolds

An Operator Theoretical Approach to Nonlocal Differential Equations

Uniqueness of ground state solutions of non-local equations in R N

Applied Math Qualifying Exam 11 October Instructions: Work 2 out of 3 problems in each of the 3 parts for a total of 6 problems.

ODE solutions for the fractional Laplacian equations arising in co

On the Hardy constant of non-convex planar domains: the case of the quadrilateral

Appeared in Commun. Contemp. Math. 11 (1) (2009) ZERO ORDER PERTURBATIONS TO FULLY NONLINEAR EQUATIONS: COMPARISON, EXISTENCE AND UNIQUENESS

Comparison Results for Semilinear Elliptic Equations in Equimeasurable Domains

Symmetry and monotonicity of least energy solutions

Laplace s Equation. Chapter Mean Value Formulas

MULTIPLE SOLUTIONS FOR A KIRCHHOFF EQUATION WITH NONLINEARITY HAVING ARBITRARY GROWTH

Singularity formation in critical parabolic problems II

There are five problems. Solve four of the five problems. Each problem is worth 25 points. A sheet of convenient formulae is provided.

Estimations universelles pour les solutions d EDP elliptiques non linéaires

Nonlinear stabilization via a linear observability

Small energy regularity for a fractional Ginzburg-Landau system

Stable solitons of the cubic-quintic NLS with a delta-function potential

Hölder regularity estimation by Hart Smith and Curvelet transforms

Sharp energy estimates and 1D symmetry for nonlinear equations involving fractional Laplacians

Transcription:

Perturbations of singular solutions to Gelfand s problem Juan Dávila (Universidad de Chile) In celebration of the 60th birthday of Ireneo Peral February 2007 collaboration with Louis Dupaigne (Université de Amiens) Perturbations of singular solutions to Gelfand s problem p.1

The problem Let Ω R N be an open bounded set with smooth boundary, λ > 0. Perturbations of singular solutions to Gelfand s problem p.2

The problem Let Ω R N be an open bounded set with smooth boundary, λ > 0. Consider the equation u = λe u u = 0 in Ω on Ω Perturbations of singular solutions to Gelfand s problem p.2

The problem Let Ω R N be an open bounded set with smooth boundary, λ > 0. Consider the equation u = λe u u = 0 in Ω on Ω Some references: Gelfand (1963) Some problems in the theory of quasilinear equations. Section 15 due to Barenblatt. Liouville (1853) Sur l équation aux différences partielles d2 log λ dudv ± λ 2a = 0. 2 Perturbations of singular solutions to Gelfand s problem p.2

Chandrasekhar (1939, 1957) An introduction to the study of stellar structure. (N = 3) Frank-Kamenetskii (1955) Diffusion and heat exchange in chemical kinetics. Bebernes et Eberly (1989) Mathematical problems from combustion theory. (N = 2, 3) Perturbations of singular solutions to Gelfand s problem p.3

Basic properties Proposition. There is 0 < λ < + such that: if 0 λ < λ then there exists a classical solution, Perturbations of singular solutions to Gelfand s problem p.4

Basic properties Proposition. There is 0 < λ < + such that: if 0 λ < λ then there exists a classical solution, if λ = λ there exists a unique weak solution u Perturbations of singular solutions to Gelfand s problem p.4

Basic properties Proposition. There is 0 < λ < + such that: if 0 λ < λ then there exists a classical solution, if λ = λ there exists a unique weak solution u if λ > λ no solution exists (even in the weak sense). Perturbations of singular solutions to Gelfand s problem p.4

Basic properties Proposition. There is 0 < λ < + such that: if 0 λ < λ then there exists a classical solution, if λ = λ there exists a unique weak solution u if λ > λ no solution exists (even in the weak sense). Moreover, if 0 λ < λ there is a unique minimal solution u λ, which is smooth and characterized by λ e u λ ϕ 2 ϕ 2 ϕ C0 (Ω). Ω Ω Perturbations of singular solutions to Gelfand s problem p.4

Basic properties Definition: u L 1 (Ω) is a weak solution if dist(x, Ω)e u L 1 (Ω) and Ω u( ζ) = λ Ω eu ζ ζ C 2 (Ω), ζ Ω = 0. Perturbations of singular solutions to Gelfand s problem p.5

Basic properties Definition: u L 1 (Ω) is a weak solution if dist(x, Ω)e u L 1 (Ω) and Ω u( ζ) = λ Ω eu ζ ζ C 2 (Ω), ζ Ω = 0. Other properties: u = lim λ λ u λ and λ Ω e u ϕ 2 Ω ϕ 2 ϕ C 0 (Ω). Perturbations of singular solutions to Gelfand s problem p.5

The question We know that there exist λ such that if 0 λ < λ there is a classical solution, if λ = λ there is a unique weak solution u if λ > λ there is no solution. Perturbations of singular solutions to Gelfand s problem p.6

The question We know that there exist λ such that if 0 λ < λ there is a classical solution, if λ = λ there is a unique weak solution u if λ > λ there is no solution. Is u a classical solution? Perturbations of singular solutions to Gelfand s problem p.6

Bifurcation diagram for Ω = B 1 Joseph-Lundgren (72): Perturbations of singular solutions to Gelfand s problem p.7

Bifurcation diagram for Ω = B 1 Joseph-Lundgren (72): In particular Theorem. If Ω = B 1 and N 9 then u is classical, and if N 10 then u = 2 log x, λ = 2(N 2). Perturbations of singular solutions to Gelfand s problem p.7

General domains Theorem. (Crandall-Rabinowitz (75), Mignot-Puel (80)) If Ω is a smooth bounded domain in R N and N 9 then u is classical. Perturbations of singular solutions to Gelfand s problem p.8

Stability and Sobolev s inequalities Let u = u λ. Multiplying the equation by e 2ju 1 and integrating λ e u (e 2ju 1) = u e 2ju Ω Ω = 2j e 2ju u 2 = 2 (e ju ) 2. Ω j Ω Perturbations of singular solutions to Gelfand s problem p.9

Stability and Sobolev s inequalities Let u = u λ. Multiplying the equation by e 2ju 1 and integrating λ e u (e 2ju 1) = u e 2ju Ω Ω = 2j e 2ju u 2 = 2 (e ju ) 2. Ω j Ω From stability with ϕ = e ju 1 we have λ e u (e ju 1) 2 (e ju 1) 2. Ω Ω Perturbations of singular solutions to Gelfand s problem p.9

Hence 2 j Ω e u (e ju 1) 2 Ω e u (e 2ju 1) Perturbations of singular solutions to Gelfand s problem p.10

Hence 2 e u (e ju 1) 2 e u (e 2ju 1) j Ω Ω ( ) 2 j 1 e (2j+1)u lower order terms Ω Perturbations of singular solutions to Gelfand s problem p.10

Hence 2 e u (e ju 1) 2 e u (e 2ju 1) j Ω Ω ( ) 2 j 1 e (2j+1)u lower order terms Ω Conclusion: if j < 2, q = 2j + 1 then u L q C where C is independent of λ. Perturbations of singular solutions to Gelfand s problem p.10

Hence 2 e u (e ju 1) 2 e u (e 2ju 1) j Ω Ω ( ) 2 j 1 e (2j+1)u lower order terms Ω Conclusion: if j < 2, q = 2j + 1 then u L q C where C is independent of λ. By elliptic estimates and Sobolev s inequality u W 2,q L if q > N/2, which works if N 9. Perturbations of singular solutions to Gelfand s problem p.10

General nonlinearities Let g : [0, ) [0, ) be a C 2, positive, increasing function satisfying: lim s + g(u)/u = +. Consider u = λg(u) in Ω u = 0 on Ω Perturbations of singular solutions to Gelfand s problem p.11

General nonlinearities Let g : [0, ) [0, ) be a C 2, positive, increasing function satisfying: lim s + g(u)/u = +. Consider u = λg(u) in Ω u = 0 on Ω Cabré (06) If Ω R N is strictly convex and N 4 then u is classical. Cabré-Capella (06) If Ω = B 1 and N 9 then u is classical. Nedev (00) If Ω R N is any bounded domain and N 3 then u is classical. Perturbations of singular solutions to Gelfand s problem p.11

Other operators { p u = λg(u) in Ω u = 0 on Ω Perturbations of singular solutions to Gelfand s problem p.12

Other operators { p u = λg(u) in Ω u = 0 on Ω Clément-de Figueiredo-Mitidieri (96), Jacobsen and Schmitt (02) Considered the radial case with exponential and power nonlinearities. Perturbations of singular solutions to Gelfand s problem p.12

Other operators { p u = λg(u) in Ω u = 0 on Ω Clément-de Figueiredo-Mitidieri (96), Jacobsen and Schmitt (02) Considered the radial case with exponential and power nonlinearities. García-Azorero-Peral-Puel (94) In general domains, if g(u) = e u the extremal solution is bounded if N < p + 4p/(p 1) and this condition is optimal. Perturbations of singular solutions to Gelfand s problem p.12

Other operators { p u = λg(u) in Ω u = 0 on Ω Clément-de Figueiredo-Mitidieri (96), Jacobsen and Schmitt (02) Considered the radial case with exponential and power nonlinearities. García-Azorero-Peral-Puel (94) In general domains, if g(u) = e u the extremal solution is bounded if N < p + 4p/(p 1) and this condition is optimal. Cabré-Sanchón (06) Consider general domains and power type nonlinearities. Perturbations of singular solutions to Gelfand s problem p.12

The case Ω = B 1, N 10 Lemma. (Brezis-Vázquez (97)) If u H 1 0(Ω) is a solution u L (Ω) for some λ which is stable, then λ = λ and u = u. Perturbations of singular solutions to Gelfand s problem p.13

The case Ω = B 1, N 10 Lemma. (Brezis-Vázquez (97)) If u H 1 0(Ω) is a solution u L (Ω) for some λ which is stable, then λ = λ and u = u. Application to the case Ω = B 1. Note that u = 2 log x, λ = 2(N 2) is a singular solution. Perturbations of singular solutions to Gelfand s problem p.13

The case Ω = B 1, N 10 Lemma. (Brezis-Vázquez (97)) If u H 1 0(Ω) is a solution u L (Ω) for some λ which is stable, then λ = λ and u = u. Application to the case Ω = B 1. Note that u = 2 log x, λ = 2(N 2) is a singular solution. Let ϕ C 0 (B 1 ). Then ϕ 2 λ e u ϕ 2 = B 1 B 1 B 1 ϕ 2 λ B1 ϕ 2 x 2. Perturbations of singular solutions to Gelfand s problem p.13

The case Ω = B 1, N 10 Lemma. (Brezis-Vázquez (97)) If u H 1 0(Ω) is a solution u L (Ω) for some λ which is stable, then λ = λ and u = u. Application to the case Ω = B 1. Note that u = 2 log x, λ = 2(N 2) is a singular solution. Let ϕ C 0 (B 1 ). Then ϕ 2 λ e u ϕ 2 = B 1 B 1 B 1 ϕ 2 λ B1 ϕ 2 x 2. Hardy s inequality: if N 3 (N 2) 2 RN ϕ 2 4 x ϕ 2 ϕ C 2 0 (R N ). R N Perturbations of singular solutions to Gelfand s problem p.13

The case Ω = B 1, N 10 By Hardy s inequality u = 2 log x is stable if 2(N 2) (N 2)2 4 N 10. Perturbations of singular solutions to Gelfand s problem p.14

More precise question If N 10 and Ω is a bounded smooth domain, is u singular? Perturbations of singular solutions to Gelfand s problem p.15

More precise question If N 10 and Ω is a bounded smooth domain, is u singular? Remark: if Ω = B 1 \ B 1/2 then u is always classical (any N). Perturbations of singular solutions to Gelfand s problem p.15

More precise question If N 10 and Ω is a bounded smooth domain, is u singular? Remark: if Ω = B 1 \ B 1/2 then u is always classical (any N). Suppose N 10 and Ω is a bounded smooth convex domain. Is u singular? Perturbations of singular solutions to Gelfand s problem p.15

Perturbations of a ball Let ψ C 2 (B; R N ) and Ω t = {x + tψ(x) : x B}. Perturbations of singular solutions to Gelfand s problem p.16

Perturbations of a ball Let ψ C 2 (B; R N ) and Ω t = {x + tψ(x) : x B}. Consider u = λe u u = 0 in Ω t on Ω t Perturbations of singular solutions to Gelfand s problem p.16

Perturbations of a ball Let ψ C 2 (B; R N ) and Ω t = {x + tψ(x) : x B}. Consider u = λe u u = 0 in Ω t on Ω t Theorem. (D.-Dupaigne) If N 4 there exists δ > 0 such that if t < δ then there is a singular solution λ(t), u(t) such that u(t) log 1 x ξ t 2 + λ(t) 2(N 2) 0 L as t 0, where ξ t B. Perturbations of singular solutions to Gelfand s problem p.16

Corollary. If N 11 and t is small then u is singular. Moreover there is ξ t B such that 1 u (t) log x ξ t 2 + λ (t) 2(N 2) 0 L as t 0. Perturbations of singular solutions to Gelfand s problem p.17

There is a singular solution (λ(t), u(t)) such that u(t) log 1 x ξ t 2 + λ(t) 2(N 2) 0 L Perturbations of singular solutions to Gelfand s problem p.18

There is a singular solution (λ(t), u(t)) such that u(t) log 1 x ξ t 2 + λ(t) 2(N 2) 0 L Since N 11 we have 2(N 2) < (N 2)2 4. Then for small t λ(t)e u(t) 2 log 1 x ξ t L (N 2) 2 4. Perturbations of singular solutions to Gelfand s problem p.18

There is a singular solution (λ(t), u(t)) such that u(t) log 1 x ξ t 2 + λ(t) 2(N 2) 0 L Since N 11 we have 2(N 2) < (N 2)2 4. Then for small t λ(t)e 1 u(t) 2 log x ξ t L (N 2) 2 4. For ϕ C0 (Ω t ), by Hardy s inequality: λ(t) Ωt e u(t) ϕ 2 (N 2)2 4 RN ϕ 2 x 2 R N ϕ 2. Perturbations of singular solutions to Gelfand s problem p.18

There is a singular solution (λ(t), u(t)) such that u(t) log 1 x ξ t 2 + λ(t) 2(N 2) 0 L Since N 11 we have 2(N 2) < (N 2)2 4. Then for small t λ(t)e 1 u(t) 2 log x ξ t L (N 2) 2 4. For ϕ C0 (Ω t ), by Hardy s inequality: λ(t) Ωt e u(t) ϕ 2 (N 2)2 4 RN ϕ 2 x 2 R N ϕ 2. By the lemma of Brezis-Vázquez we conclude u (t) = u(t), λ (t) = λ(t). Perturbations of singular solutions to Gelfand s problem p.18

Consider u = λ(1 + u) p in Ω t u = 0 on Ω t where Ω t is a C 2 perturbation of the ball, p > 1. Perturbations of singular solutions to Gelfand s problem p.19

Consider u = λ(1 + u) p in Ω t u = 0 on Ω t where Ω t is a C 2 perturbation of the ball, p > 1. Theorem. If N 11 and p > 6 + 4 p 1 + 4 p p 1 then for t small the extremal solution is singular. Perturbations of singular solutions to Gelfand s problem p.19

Consider u = λ(1 + u) p in Ω t u = 0 on Ω t where Ω t is a C 2 perturbation of the ball, p > 1. Theorem. If N 11 and p > 6 + 4 p 1 + 4 p p 1 then for t small the extremal solution is singular. It is known that for any domain, if N 10, or N 11 and p < 6 + 4 p 1 + 4 p p 1 then u is classical. Perturbations of singular solutions to Gelfand s problem p.19

Linearization The proof is by linearization around the singular solution 2 log x, λ = 2(N 2). Perturbations of singular solutions to Gelfand s problem p.20

Linearization The proof is by linearization around the singular solution 2 log x, λ = 2(N 2). We change variables y = x + tψ(x), x B 1 and define Then v(x) = u(x + tψ(x)). y u = x v + L t v where L t is a small second order operator. Perturbations of singular solutions to Gelfand s problem p.20

Linearization We look for a solution of the form v(x) = log where c = 2(N 2). 1 x ξ 2 + φ, λ = c + µ, Perturbations of singular solutions to Gelfand s problem p.21

Linearization We look for a solution of the form v(x) = log where c = 2(N 2). Then we need to solve φ L t φ 1 x ξ 2 + φ, λ = c + µ, c x ξ 2φ = c 1 φ) + x ξ 2(eφ ( 1 ) + L t log x ξ 2 φ = log 1 x ξ 2 on B. µ x ξ 2eφ in B Perturbations of singular solutions to Gelfand s problem p.21

A simple case Ω t is an ellipsoid, v(x) = u(x, (1 t)x N ), x = (x, x N ), and then ξ = 0. Perturbations of singular solutions to Gelfand s problem p.22

A simple case Ω t is an ellipsoid, v(x) = u(x, (1 t)x N ), x = (x, x N ), and then ξ = 0. Then the equation becomes φ t 2 2 φ x 2 N + µ φ = 0 + t 2 2 u 0 x 2eφ x 2 N on B. where u 0 (x) = 2 log x. c c x 2φ = 1 φ) x 2(eφ in B Perturbations of singular solutions to Gelfand s problem p.22

Comments Consider the linear operator c x ξ 2 Perturbations of singular solutions to Gelfand s problem p.23

Comments Consider the linear operator c x ξ 2 If N 9 the operator is not coercive in H 1 0. Perturbations of singular solutions to Gelfand s problem p.23

Comments Consider the linear operator c x ξ 2 If N 9 the operator is not coercive in H 1 0. If c (N 2)2 4, which holds if N 10, this operator is coercive. Perturbations of singular solutions to Gelfand s problem p.23

Comments Consider the linear operator c x ξ 2 If N 9 the operator is not coercive in H 1 0. If c (N 2)2 4, which holds if N 10, this operator is coercive. Typically solutions are singular at ξ, with a behavior x ξ α for some α > 0. Perturbations of singular solutions to Gelfand s problem p.23

Comments Consider the linear operator c x ξ 2 If N 9 the operator is not coercive in H 1 0. If c (N 2)2 4, which holds if N 10, this operator is coercive. Typically solutions are singular at ξ, with a behavior x ξ α for some α > 0. This functional setting is not useful since the nonlinear term that appears in the right hand side, c namely x ξ (e φ 1 φ), is too strong. 2 Perturbations of singular solutions to Gelfand s problem p.23

Right inverse for the linear operator Lemma. Let N 4, h,g be such that x ξ 2 h, x ξ 2 g L (B), h > 0, w smooth Perturbations of singular solutions to Gelfand s problem p.24

Right inverse for the linear operator Lemma. Let N 4, h,g be such that x ξ 2 h, x ξ 2 g L (B), h > 0, w smooth Consider φ c x ξ 2φ = g + µ 0h + φ = w where V i,ξ are explicit. on B N i=1 µ i V i,ξ in B Perturbations of singular solutions to Gelfand s problem p.24

Right inverse for the linear operator Lemma. Let N 4, h,g be such that x ξ 2 h, x ξ 2 g L (B), h > 0, w smooth Consider φ c x ξ 2φ = g + µ 0h + φ = w on B N i=1 µ i V i,ξ in B where V i,ξ are explicit. If ξ is small enough there is a solution φ, µ 0,..., µ N such that φ L + µ i C h x ξ 2 g L Perturbations of singular solutions to Gelfand s problem p.24

Right inverse for the linear operator The same result is true for the linear operator φ c x ξ 2φ L tφ if ξ and t are small enough. Perturbations of singular solutions to Gelfand s problem p.25

The nonlinear problem Using the linear lemma and the fixed point theorem we obtain φ, µ 0,..., µ N such that Perturbations of singular solutions to Gelfand s problem p.26

The nonlinear problem Using the linear lemma and the fixed point theorem we obtain φ, µ 0,..., µ N such that c φ L t φ x ξ 2φ = c 1 φ) x ξ 2(eφ where u ξ = log 1 x ξ 2 + µ 0 1 x ξ 2eφ + L t u ξ + φ = u ξ B N i=1 µ i V i,ξ Perturbations of singular solutions to Gelfand s problem p.26

Reduction We have to show that there is a choice of ξ such that µ 1,..., µ N = 0. Perturbations of singular solutions to Gelfand s problem p.27

Reduction We have to show that there is a choice of ξ such that µ 1,..., µ N = 0. Multiplying the equation by suitable test functions and integrating we reach a system of equations of the form F (ξ, t) = 0 Perturbations of singular solutions to Gelfand s problem p.27

Reduction We have to show that there is a choice of ξ such that µ 1,..., µ N = 0. Multiplying the equation by suitable test functions and integrating we reach a system of equations of the form F (ξ, t) = 0 This can be solved by the implicit function theorem. Perturbations of singular solutions to Gelfand s problem p.27

The linear lemma We consider only the operator c x 2. Perturbations of singular solutions to Gelfand s problem p.28

The linear lemma We consider only the operator c x 2. Let N 3, g C (B \ {0}) be a radial function such that x 2 g L (B). Then the equation φ c x 2φ = g in B φ = 0 on B has a solution in L (B) if and only if B gw 0 = 0 Perturbations of singular solutions to Gelfand s problem p.28

The linear lemma We consider only the operator c x 2. Let N 3, g C (B \ {0}) be a radial function such that x 2 g L (B). Then the equation φ c x 2φ = g in B φ = 0 on B has a solution in L (B) if and only if B gw 0 = 0 where W 0 = r α+ r α and α ± = N 2 (N 2) 2 ± 2 4 c. Perturbations of singular solutions to Gelfand s problem p.28

The linear lemma We consider only the operator c x 2. Let N 3, g C (B \ {0}) be a radial function such that x 2 g L (B). Then the equation φ c x 2φ = g in B φ = 0 on B has a solution in L (B) if and only if B gw 0 = 0 where W 0 = r α+ r α and α ± = N 2 (N 2) 2 ± 2 4 c. Moreover φ L C x 2 g L and this solution is unique. Perturbations of singular solutions to Gelfand s problem p.28

Idea of the proof: the condition is necessary W 0 = r α+ r α is in the kernel of the linear operator W 0 c x 2W 0 = 0 in B W 0 = 0 on B Perturbations of singular solutions to Gelfand s problem p.29

Idea of the proof: the condition is necessary W 0 = r α+ r α is in the kernel of the linear operator W 0 c x 2W 0 = 0 in B W 0 = 0 on B If φ is bounded one may justify the integration by parts ) ) gw 0 = ( φ c x 2φ W 0 = φ ( W 0 c x 2W 0 = 0 Perturbations of singular solutions to Gelfand s problem p.29

Idea of the proof: the condition is sufficient Construction of a solution: we seek φ(r) that solves φ c x 2 φ = g: φ + N 1 r φ + c r2φ = g Perturbations of singular solutions to Gelfand s problem p.30

Idea of the proof: the condition is sufficient Construction of a solution: we seek φ(r) that solves φ c x 2 φ = g: φ + N 1 r φ + c r2φ = g Then φ(r) = 1 α α + r 0 s((s/r)α (s/r) α+ )g(s) ds Perturbations of singular solutions to Gelfand s problem p.30

Idea of the proof: the condition is sufficient Construction of a solution: we seek φ(r) that solves φ c x 2 φ = g: φ + N 1 r φ + c r2φ = g Then φ(r) = 1 r α α + 0 (s/r) s((s/r)α α+ )g(s) ds φ(r) = r2 S N 1 B W 0(x)g(rx) dx Since g(x) C/ x 2 we have φ L. Since B W 0g = 0 we have φ(1) = 0. Perturbations of singular solutions to Gelfand s problem p.30

Non radial case We decompose φ in a Fourier series φ(x) = k φ k(r)ϕ k (θ) where r > 0, θ S N 1, and ϕ k are the eigenfunctions of on the sphere S N 1 : S N 1ϕ k = λ k ϕ k. Perturbations of singular solutions to Gelfand s problem p.31

Non radial case We decompose φ in a Fourier series φ(x) = k φ k(r)ϕ k (θ) where r > 0, θ S N 1, and ϕ k are the eigenfunctions of on the sphere S N 1 : S N 1ϕ k = λ k ϕ k. Then φ c x 2 φ = g in B is equivalent to φ k N 1 φ k c λ k φ r r 2 k = g k Perturbations of singular solutions to Gelfand s problem p.31

Non radial case We decompose φ in a Fourier series φ(x) = k φ k(r)ϕ k (θ) where r > 0, θ S N 1, and ϕ k are the eigenfunctions of on the sphere S N 1 : S N 1ϕ k = λ k ϕ k. Then φ c x 2 φ = g in B is equivalent to φ k N 1 φ k c λ k φ r r 2 k = g k If c λ k 0 the equation has a bounded solution without requiring orthogonality conditions. If c λ k > 0 orthogonality conditions are required (with respect to elements in the kernel ). Perturbations of singular solutions to Gelfand s problem p.31

c = 2(N 2) λ 0 = 0 λ 1 =... = λ N = N 1 λ k 2N, k N + 1 and N 4 yields Numbers... Perturbations of singular solutions to Gelfand s problem p.32

c = 2(N 2) λ 0 = 0 λ 1 =... = λ N = N 1 λ k 2N, k N + 1 and N 4 yields Numbers... c λ k > 0 for k = 0,..., N c λ k 0 for k N + 1 So N + 1 conditions are required to have a bounded solution. Perturbations of singular solutions to Gelfand s problem p.32

Related work Caffarelli-Hardt-Simon (84) Construction of singular minimal surfaces which are not cones (by perturbation of minimal cones). Perturbations of singular solutions to Gelfand s problem p.33

Related work Caffarelli-Hardt-Simon (84) Construction of singular minimal surfaces which are not cones (by perturbation of minimal cones). Pacard (92,93) Existence of singular solutions to u = e u and u p (without boundary conditions) Perturbations of singular solutions to Gelfand s problem p.33

Related work Caffarelli-Hardt-Simon (84) Construction of singular minimal surfaces which are not cones (by perturbation of minimal cones). Pacard (92,93) Existence of singular solutions to u = e u and u p (without boundary conditions) Mazzeo-Pacard (96) construct solutions to u = u p with singularities on points ( N N 2 < p < N+2 k N 2 ) or manifolds ( k 2 < p < k+2 k 2, k is de codimension). Perturbations of singular solutions to Gelfand s problem p.33

Related work Caffarelli-Hardt-Simon (84) Construction of singular minimal surfaces which are not cones (by perturbation of minimal cones). Pacard (92,93) Existence of singular solutions to u = e u and u p (without boundary conditions) Mazzeo-Pacard (96) construct solutions to u = u p with singularities on points ( N N 2 < p < N+2 k N 2 ) or manifolds ( k 2 < p < k+2 k 2, k is de codimension). Rebai (96,99) u = e u in a ball in dimension 3, also multiple singularities N 10 (without boundary condition) Perturbations of singular solutions to Gelfand s problem p.33

A variant Consider u = λe u in B u = ψ on B where ψ is a smooth function. Perturbations of singular solutions to Gelfand s problem p.34

Consider A variant u = λe u u = ψ in B on B where ψ is a smooth function. Theorem. (D.-Dupaigne) If N 4 and ψ is small enough (in C 2,α ) then there exists ξ B and a singular solution λ, u such that u log 1 x ξ 2 L (B). Perturbations of singular solutions to Gelfand s problem p.34

Consider A variant u = λe u u = ψ in B on B where ψ is a smooth function. Theorem. (D.-Dupaigne) If N 4 and ψ is small enough (in C 2,α ) then there exists ξ B and a singular solution λ, u such that u log 1 x ξ 2 L (B). Note that ξ depends on ψ. Perturbations of singular solutions to Gelfand s problem p.34

The case N = 3 Consider u = λe u in B u = ψ on B where ψ is a smooth function. Perturbations of singular solutions to Gelfand s problem p.35

The case N = 3 Consider u = λe u u = ψ where ψ is a smooth function. in B on B Theorem. (Matano, Rebai (99)) If N = 3 there is δ > 0 such that for any ψ C 2,α < δ and any ξ < δ there is a singular solution λ, u such that u log 1 x ξ 2 L (B). Perturbations of singular solutions to Gelfand s problem p.35

Isolated singularities in dimension 3 The function u(r, θ) = log(1/r 2 )+log(2/λ)+2ω(θ) r > 0, θ S 2 is a singular solution in R 3 if and only if S 2ω + e 2ω 1 = 0 in S 2. Smooth solutions form a 3 dimensional manifold. Perturbations of singular solutions to Gelfand s problem p.36

Isolated singularities in dimension 3 The function u(r, θ) = log(1/r 2 )+log(2/λ)+2ω(θ) r > 0, θ S 2 is a singular solution in R 3 if and only if S 2ω + e 2ω 1 = 0 in S 2. Smooth solutions form a 3 dimensional manifold. Bidaut-Veron Veron (91) describe all possible behaviors of smooth solutions to u = λe u in B 1 \ {0} (with an isolated singularity) in dimension 3, such that e u C x 2. Perturbations of singular solutions to Gelfand s problem p.36

Isolated singularities in N = 3 In dimension 3, if e u C x 2. Perturbations of singular solutions to Gelfand s problem p.37

Isolated singularities in N = 3 In dimension 3, if e u C x 2. then either 0 is a removable singularity, Perturbations of singular solutions to Gelfand s problem p.37

Isolated singularities in N = 3 In dimension 3, if e u C x 2. then either 0 is a removable singularity, or lim x 0 (u(x) γ x 1 ) exists for some γ < 0 and u = λe u + 4πγδ 0, Perturbations of singular solutions to Gelfand s problem p.37

Isolated singularities in N = 3 In dimension 3, if e u C x 2. then either 0 is a removable singularity, or lim x 0 (u(x) γ x 1 ) exists for some γ < 0 and u = λe u + 4πγδ 0, or there exists ω solution to S 2ω + e 2ω 1 = 0 in S 2 such that lim r + u(rθ) log(1/r2 ) = ω(θ), θ S 2. Perturbations of singular solutions to Gelfand s problem p.37

Is u singular for all Ω convex? Let ε > 0, x = (y, z) R N, y R N 1, z RN 2. Perturbations of singular solutions to Gelfand s problem p.38

Is u singular for all Ω convex? Let ε > 0, x = (y, z) R N, y R N 1, z RN 2. Ω ε = {(y, εz) : (y, z) B 1 R N }. ε R N 2 R N 1 Perturbations of singular solutions to Gelfand s problem p.38

Is u singular for all Ω convex? Let ε > 0, x = (y, z) R N, y R N 1, z RN 2. Ω ε = {(y, εz) : (y, z) B 1 R N }. ε R N 2 R N 1 Theorem. (Dancer (93)) Suppose N 2 9. If ε is small then u ε is classical. Note that N = N 1 + N 2 may be larger than 10. Perturbations of singular solutions to Gelfand s problem p.38

Is u singular for all Ω convex? Let ε > 0, x = (y, z) R N, y R N 1, z RN 2. Ω ε = {(y, εz) : (y, z) B 1 R N }. ε R N 2 R N 1 Theorem. (Dancer (93)) Suppose N 2 9. If ε is small then u ε is classical. Note that N = N 1 + N 2 may be larger than 10. The result is still true if Ω is a smooth bounded strictly convex. Perturbations of singular solutions to Gelfand s problem p.38

What happens if N 2 10? Consider a torus Ω ε in R N with cross-section a ball of radius ε > 0 in R N 2, N = N 1 + N 2, N 1 1. Perturbations of singular solutions to Gelfand s problem p.39

What happens if N 2 10? Consider a torus Ω ε in R N with cross-section a ball of radius ε > 0 in R N 2, N = N 1 + N 2, N 1 1. If N 2 11 then for ε small the extremal solution is singular. Perturbations of singular solutions to Gelfand s problem p.39

Singularities at infinity Consider u + u p = 0, u > 0 in Ω = R N \ D, u = 0 on D, lim u(x) = 0 x + where p > N+2 N 2 and D is a smooth bounded open set such that Ω is connected. Perturbations of singular solutions to Gelfand s problem p.40

Singularities at infinity Consider u + u p = 0, u > 0 in Ω = R N \ D, u = 0 on D, lim u(x) = 0 x + where p > N+2 N 2 and D is a smooth bounded open set such that Ω is connected. Theorem. (D.-del Pino-Musso-Wei) If N 3 and p > N+2 N 2 then there are infinitely many solutions, that have slow decay u(x) x 2 p 1 as x +. Perturbations of singular solutions to Gelfand s problem p.40

If λ > λ there is no solution. Perturbations of singular solutions to Gelfand s problem p.41

If λ > λ there is no solution. If λ = λ there is a unique solution. Perturbations of singular solutions to Gelfand s problem p.41

If λ > λ there is no solution. If λ = λ there is a unique solution. Suppose λ < λ and let u λ be the minimal solution. Then u (u u λ ) = λ e u (u u λ ) Ω Ω u λ (u u λ ) = λ e u λ (u u λ ) Ω Ω Perturbations of singular solutions to Gelfand s problem p.41

If λ > λ there is no solution. If λ = λ there is a unique solution. Suppose λ < λ and let u λ be the minimal solution. Then u (u u λ ) = λ e u (u u λ ) Ω Ω u λ (u u λ ) = λ e u λ (u u λ ) Ω Ω Hence Ω (u u λ ) 2 = λ Ω (e u e u λ )(u u λ ). Perturbations of singular solutions to Gelfand s problem p.41

We have Ω (u u λ) 2 = λ Ω (eu e u λ )(u u λ) Perturbations of singular solutions to Gelfand s problem p.42

We have Ω (u u λ) 2 = λ Ω (eu e u λ )(u u λ) Since u is stable Ω (u u λ) 2 λ Ω eu (u u λ ) 2 Perturbations of singular solutions to Gelfand s problem p.42

We have Ω (u u λ) 2 = λ Ω (eu e u λ )(u u λ) Since u is stable Ω (u u λ) 2 λ Ω eu (u u λ ) 2 It follows that (e u + e u (u λ u) e u λ )(u u λ ) 0. Ω Perturbations of singular solutions to Gelfand s problem p.42

We have Ω (u u λ) 2 = λ Ω (eu e u λ )(u u λ) Since u is stable Ω (u u λ) 2 λ Ω eu (u u λ ) 2 It follows that (e u + e u (u λ u) e u λ )(u u λ ) 0. Ω By convexity the integrand is non-positive. This implies u = u λ but u L while u λ is classical. Perturbations of singular solutions to Gelfand s problem p.42