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arXiv:2305.00728v1 [math.AP] 01 May 2023

Principal eigenvalues and eigenfunctions for fully nonlinear equations in punctured balls

Isabeau Birindelli Affiliation: Dipartimento di Matematica, Sapienza Università di Roma    Françoise Demengel Affiliation: Département de Mathématiques, CY Paris University    Fabiana Leoni Affiliation: Dipartimento di Matematica, Sapienza Università di Roma
Abstract

This paper is devoted to the proof of the existence of the principal eigenvalue and related eigenfunctions for fully nonlinear uniformly elliptic equations posed in a punctured ball, in presence of a singular potential. More precisely, we analyze existence, uniqueness and regularity of solutions (λ¯γ,uγ)(\bar{\lambda}_{\gamma},u_{\gamma}) of the equation

F(D2uγ)+λ¯γuγrγ=0inB(0,1){0},uγ=0onB(0,1)F(D^{2}u_{\gamma})+\bar{\lambda}_{\gamma}\frac{u_{\gamma}}{r^{\gamma}}=0\ {\rm in}\ B(0,1)\setminus\{0\},\ u_{\gamma}=0\ {\rm on}\ \partial B(0,1)

where uγ>0u_{\gamma}>0 in B(0,1)B(0,1), and γ>0\gamma>0. We prove existence of radial solutions which are continuous on B(0,1)¯\overline{B(0,1)} in the case γ<2\gamma<2, existence of unbounded solutions in the case γ=2\gamma=2 and a non existence result for γ>2\gamma>2. We also give the explicit value of λ¯2\bar{\lambda}_{2} in the case of Pucci’s operators, which generalizes the Hardy–Sobolev constant for the Laplacian.

1 Introduction

In this paper we will study radial eigenvalues and related positive radial eigenfunctions for the Dirichlet problem

F(D2u)+μrγu=0 in B(0,1)¯{0}F(D^{2}u)+\mu r^{-\gamma}u=0\,\mbox{ in }\ \overline{B(0,1)}\setminus\{0\}

when γ>0\gamma>0, and FF is a second order fully nonlinear uniformly elliptic operator. By radial eigenvalue and radial eigenfunction we mean respectfully a real value λγ\lambda_{\gamma} and a radial nontrivial function uγu_{\gamma} satisfying the equation

(1.1) {F(D2uγ)+λγrγuγ=0 in B(0,1)¯{0}uγ=0 on B(0,1).\left\{\begin{array}[]{lc}F(D^{2}u_{\gamma})+\lambda_{\gamma}r^{-\gamma}u_{\gamma}=0&\mbox{ in }\ \overline{B(0,1)}\setminus\{0\}\\ u_{\gamma}=0&\mbox{ on }\ \partial B(0,1).\end{array}\right.

In principle, eigenfunctions are required to satisfy the above eigenvalue problem in the viscosity sense, but, due to the radial symmetry, this is equivalent to consider classical solutions.

We will focus on constant sign eigenfunctions, in particular positive eigenfunctions, thus referring to the so called principal eigenvalues. If necessary, in order to emphasize the dependence of the eigenvalue on the operator FF, the potential f(r)f(r) appearing in the zero order term and the domain Ω\Omega in which the equation is considered, we will use the notation λ=λ(F,f(r),Ω)\lambda=\lambda(F,f(r),\Omega).

Interestingly, we will see that for problem (1.1), as in the case when FF is the Laplace operator, γ=2\gamma=2 is a critical value, in the sense that for γ<2\gamma<2 there exists smooth eigenfunctions, for γ>2\gamma>2 there are no eigenfunctions and, for γ=2\gamma=2, the eigenfunctions are unbounded.

Let us recall some known results when FF is the Laplacian. In the case γ=2\gamma=2, the equation is naturally linked to Hardy’s inequality. Indeed, if N>2N>2 and uH01(B(0,1))u\in H_{0}^{1}(B(0,1)) (respectively, uH1(N)u\in H^{1}(\mathbb{R}^{N})), then u(x)|x|\frac{u(x)}{|x|} belongs to L2(B(0,1))L^{2}(B(0,1)) (respectively u(x)|x|L2(N)\frac{u(x)}{|x|}\in L^{2}(\mathbb{R}^{N})), and there exists a positive constant cc such that

(|u(x)||x|)2c|u|2.\int\left(\frac{|u(x)|}{|x|}\right)^{2}\leq c\int|\nabla u|^{2}.

Furthermore, the best constant c=4(N2)2c=\frac{4}{(N-2)^{2}} is not achieved, in the sense that

(1.2) infuH01(B(0,1)),B(0,1)(|u(x)||x||)2=1B(0,1)|u|2=(N2)24\inf_{u\in H_{0}^{1}(B(0,1)),\int_{B(0,1)}\left(\frac{|u(x)|}{|x|}|\right)^{2}=1}\int_{B(0,1)}|\nabla u|^{2}=\frac{(N-2)^{2}}{4}

but there is no uH01u\in H_{0}^{1} which realizes the infimum. By obvious arguments, B(0,1)B(0,1) can be replaced by any bounded regular open set of N\mathbb{R}^{N} containing 00, and the optimal constant does not depend on the size of Ω\Omega. Note that the right hand side of (1.2) coincides with the variational characterization of the first (or principal) eigenvalue for the equation

Δu=λu|x|2.-\Delta u=\lambda\frac{u}{|x|^{2}}.

For further knowledge on the Hardy–Sobolev inequality and for the case of the pp-Laplacian, we refer to [16, 19, 21].

On the other hand, if the exponent γ\gamma of the potential is strictly less than 2, since H01(B(0,1))H_{0}^{1}(B(0,1)) is compactly embedded into the weighted space L2(B(0,1),1rγ)L^{2}(B(0,1),\frac{1}{r^{\gamma}}), then existence of minima in H01(B(0,1))H_{0}^{1}(B(0,1)) can be obtained by standard arguments of the direct method in calculus of variations. In that case, denoting

(1.3) λ¯γ=infuH01(B(0,1)),B(0,1)|u(x)|2|x|γ=1B(0,1)|u|2\bar{\lambda}_{\gamma}=\inf_{u\in H_{0}^{1}(B(0,1)),\int_{B(0,1)}\frac{|u(x)|^{2}}{|x|^{\gamma}}=1}\int_{B(0,1)}|\nabla u|^{2}

one sees that λ¯γ\bar{\lambda}_{\gamma} is also the first eigenvalue for the equation

Δu+λ¯γurγ=0,\Delta u+\bar{\lambda}_{\gamma}\frac{u}{r^{\gamma}}=0\,,

meaning that λ¯γ\bar{\lambda}_{\gamma} is such that there exists u>0u>0 in H01(B(0,1))H_{0}^{1}(B(0,1)) satisfying the equation.

Note that, by its definition, λ¯γ\bar{\lambda}_{\gamma} depends on the domain, since

λ¯γ(B(0,t))=1t2γλ¯γ(B(0,1)).\bar{\lambda}_{\gamma}(B(0,t))=\frac{1}{t^{2-\gamma}}\bar{\lambda}_{\gamma}(B(0,1)).

If γ>2\gamma>2 there is no embedding from H01(B(0,1))H_{0}^{1}(B(0,1)) into L2(B(0,1),1rγ)L^{2}(B(0,1),\frac{1}{r^{\gamma}}). Indeed, as an example, the function

u(r)=rN22+ϵ(logr)u(r)=r^{-\frac{N-2}{2}+\epsilon}(-\log r)

with 0<ϵ<γ220<\epsilon<\frac{\gamma-2}{2}, belongs to H01(B(0,1))H_{0}^{1}(B(0,1)) and satisfies

B(0,1)u(|x|)2|x|γ=+\int_{B(0,1)}\frac{u(|x|)^{2}}{|x|^{\gamma}}=+\infty

For results in the variational linear case we refer to the works of many authors, but in particular we wish to mention the works of Cirstea and collaborators [9, 11, 12, 10] .

Let us now focus on the case of concern of this paper i.e. when FF is a fully nonlinear uniformly elliptic operator, that is FF is a continuous function defined on the set 𝒮N\mathcal{S}_{N} of symmetric N×NN\times N matrices, and it satisfies, for positive constants Λλ>0\Lambda\geq\lambda>0,

(1.4) λtr(M)F(M+M)F(M)Λtr(M),\lambda\,\hbox{tr}(M^{\prime})\leq F(M+M^{\prime})-F(M)\leq\Lambda\,\hbox{tr}(M^{\prime})\,,

for all M,M𝒮NM,M^{\prime}\in\mathcal{S}_{N}, with MM^{\prime} positive semidefinite.

We suppose also that FF is rotationally invariant, that is

(1.5) F(OtMO)=F(M)F(O^{t}MO)=F(M)

for every orthogonal matrix OO and for all M𝒮NM\in\mathcal{S}_{N}, and that FF is positively homogeneous of degree 11, i.e.

(1.6) F(tM)=tF(M)F(tM)=tF(M)

for any M𝒮NM\in\mathcal{S}_{N} and for all t>0t>0. In this case we will see that, as in the regular case i.e. γ=0\gamma=0, the first eigenvalue for problem (1.1) can be defined on the model of [1], i.e. by the optimization formula

(1.7) λ¯γ=λ¯γ(F,rγ,B(0,1){0})=sup{μ:uC(B(0,1){0}),u>0 in B(0,1){0},F(D2u)+μurγ0},\begin{array}[]{rl}\bar{\lambda}_{\gamma}&=\bar{\lambda}_{\gamma}(F,r^{-\gamma},B(0,1)\setminus\{0\})\\[8.61108pt] &=\sup\{\mu\,:\ \exists\,u\in C(B(0,1)\setminus\{0\})\,,\ u>0\hbox{ in }B(0,1)\setminus\{0\},\ F(D^{2}u)+\mu\frac{u}{r^{\gamma}}\leq 0\}\,,\end{array}

where the differential inequality is understood in the viscosity sense.

The first easy observation is that, by considering constant super-solutions, one always has λ¯γ0\bar{\lambda}_{\gamma}\geq 0. One of the goals of the present paper is to show, in particular, that λ¯γ>0\bar{\lambda}_{\gamma}>0 for γ2\gamma\leq 2.

In case of smooth coefficients and regular domains, the principal eigenvalues and related eigenfunctions for fully nonlinear operators FF have been largely investigated. We refer to e.g. [18, 2, 3, 4, 20].

The Pucci’s extremal operators will play a crucial role and we will treat them in depth. We begin by recalling their definition: by decomposing each matrix M𝒮NM\in\mathcal{S}_{N} as M=M+MM=M^{+}-M^{-}, where M+M^{+} and MM^{-} are positive semidefinite matrices satisfying M+M=OM^{+}M^{-}=O, then Pucci’s sup operator can be defined as

λ,Λ+(M)=Λtr(M+)λtr(M),\mathcal{M}^{+}_{\lambda,\Lambda}(M)=\Lambda\hbox{tr}(M^{+})-\lambda\hbox{tr}(M^{-})\,,

as well as Pucci’s inf operator is given by

λ,Λ(M)=λtr(M+)Λtr(M)=λ,Λ+(M).\mathcal{M}^{-}_{\lambda,\Lambda}(M)=\lambda\hbox{tr}(M^{+})-\Lambda\hbox{tr}(M^{-})=-\mathcal{M}^{+}_{\lambda,\Lambda}(-M).

As it is well known, see [8], under assumptions (1.4) and (1.6), each operator FF satisfies

(1.8) λ,Λ(M)F(M)λ,Λ+(M),M𝒮N,\mathcal{M}^{-}_{\lambda,\Lambda}(M)\leq F(M)\leq\mathcal{M}^{+}_{\lambda,\Lambda}(M)\,,\qquad\forall\,M\in\mathcal{S}_{N}\,,

showing as Pucci’s operators act as explicit extremal operators in the whole class of uniformly elliptic operators having the same ellipticity constants. In the sequel, we will omit in the notation the dependence on the ellipticity constants, which are fixed once for all.

We further recall that for a C2C^{2} radial function u(x)=u(|x|)u(x)=u(|x|), one has

D2u(x)=u′′(r)xxr2+u(r)r(Ixxr2),D^{2}u(x)=u^{\prime\prime}(r)\frac{x\otimes x}{r^{2}}+\frac{u^{\prime}(r)}{r}\left(I-\frac{x\otimes x}{r^{2}}\right)\,,

and, as a consequence,

+(D2u)=Λ(N1)(u(r)r)+λ(N1)(u(r)r)+Λ(u′′(r))+λ(u′′(r)),{\cal M}^{+}(D^{2}u)=\Lambda(N-1)\left(\frac{u^{\prime}(r)}{r}\right)^{+}-\lambda(N-1)\left(\frac{u^{\prime}(r)}{r}\right)^{-}+\Lambda(u^{\prime\prime}(r))^{+}-\lambda(u^{\prime\prime}(r))^{-}\,,
(D2u)=λ(N1)(u(r)r)+Λ(N1)(u(r)r)+λ(u′′(r))+Λ(u′′(r)).{\cal M}^{-}(D^{2}u)=\lambda(N-1)\left(\frac{u^{\prime}(r)}{r}\right)^{+}-\Lambda(N-1)\left(\frac{u^{\prime}(r)}{r}\right)^{-}+\lambda(u^{\prime\prime}(r))^{+}-\Lambda(u^{\prime\prime}(r))^{-}\,.

Thus, the ODEs satisfied by radial solutions of Pucci’s extremal equations have coefficients depending on the dimension like parameters, associated with +\mathcal{M}^{+} and \mathcal{M}^{-} respectively, defined as

N~+=λΛ(N1)+1,N~=Λλ(N1)+1.\tilde{N}_{+}=\frac{\lambda}{\Lambda}(N-1)+1\,,\quad\tilde{N}_{-}=\frac{\Lambda}{\lambda}(N-1)+1\,.

Note that one has always

N~NN~+,\tilde{N}_{-}\geq N\geq\tilde{N}_{+}\,,

with equalities holding true if and only if Λ=λ\Lambda=\lambda. We will assume always that N~+>2\tilde{N}_{+}>2.

We can now state the main results of the paper. We will always assume that FF satisfies assumptions (1.4), (1.5) and (1.6). Let us start with the case γ<2\gamma<2.

Theorem 1.1.

Suppose that γ<2\gamma<2. Then:

  • (i)

    λ¯γ\bar{\lambda}_{\gamma} defined in (1.7 ) is positive and there exists a function uu, continuous in B(0,1)¯\overline{B(0,1)}, radial, strictly positive in B(0,1)B(0,1), such that

    {F(D2u)+λ¯γurγ=0 in B(0,1){0}u=0 on B(0,1).\left\{\begin{array}[]{cl}F(D^{2}u)+\bar{\lambda}_{\gamma}\frac{u}{r^{\gamma}}=0&\hbox{ in }\ B(0,1)\setminus\{0\}\\[4.30554pt] u=0&\hbox{ on }\ \partial B(0,1)\end{array}\right..

    Furthermore uu is C2(B(0,1){0})C^{2}(B(0,1)\setminus\{0\}) and it can be extended on B(0,1)B(0,1) as a Lipschitz continuous function if γ1\gamma\leq 1, as a function of class C1(B(0,1))C^{1}(B(0,1)) when γ<1\gamma<1, and as an Hölder continuous function with exponent 2γ2-\gamma if γ>1\gamma>1.

  • (ii)

    λ¯γ\bar{\lambda}_{\gamma} is stable under various regular approximations :

    λ¯γ=limϵ0λ¯(F,1(r2+ϵ2)γ2,B(0,1)),\bar{\lambda}_{\gamma}=\lim_{\epsilon\rightarrow 0}\bar{\lambda}(F,\frac{1}{(r^{2}+\epsilon^{2})^{\frac{\gamma}{2}}},B(0,1))\,,\,
    λ¯γ=limδ0λ¯(F,1rγ,B(0,1)B(0,δ)¯).\bar{\lambda}_{\gamma}=\lim_{\delta\rightarrow 0}\bar{\lambda}(F,\frac{1}{r^{\gamma}},B(0,1)\setminus\overline{B(0,\delta)})\,.

Statement (i) of the above theorem shows in particular that λ¯γ\bar{\lambda}_{\gamma} is actually achieved on smooth radial eigenfunctions. Thus, if we define

(1.9) λ¯γ:=sup{μ:uC2(B(0,1){0}),u>0 in B(0,1){0},u radial,F(D2u)+μurγ0},\bar{\lambda}_{\gamma}^{\prime}:=\sup\{\mu\,:\ \exists\,u\in C^{2}(B(0,1)\setminus\{0\})\,,\ u>0\hbox{ in }B(0,1)\setminus\{0\},\ u\hbox{ radial},\ \ F(D^{2}u)+\mu\frac{u}{r^{\gamma}}\leq 0\}\,,

it then follows that

λ¯γ=λ¯γ.\bar{\lambda}_{\gamma}=\bar{\lambda}_{\gamma}^{\prime}.

Actually, we will work initially with the smooth eigenvalue λ¯γ\bar{\lambda}_{\gamma}^{\prime}, and we will finally prove that it coincides with λ¯γ\bar{\lambda}_{\gamma}. Note that, due to the lack of regularity of the coefficient function 1rγ\frac{1}{r^{\gamma}} we cannot employ directly the results of [14] which ensure that solutions of

F(D2u)+f(r)u=0F(D^{2}u)+f(r)u=0

in a radial domain are radial when ff is non increasing. Nonetheless, we will prove that the two eigenvalues coincide for any γ2\gamma\leq 2. However, due to the singularity at zero, we cannot prove that any eigenfunction is radial.

Theorem 1.1 will be proved after several steps and intermediate results. In particular, we will prove a comparison theorem for smooth, bounded, radial sub- and super-solutions in the punctured ball, without assuming any order condition at the origin. Furthermore, we will show that for μ<λ¯γ\mu<\bar{\lambda}_{\gamma} the problem

{F(D2u)+μurγ=f(r)rγ in B(0,1){0}u=0 on B(0,1)\left\{\begin{array}[]{cl}F(D^{2}u)+\mu ur^{-\gamma}=f(r)r^{-\gamma}&\hbox{ in }B(0,1)\setminus\{0\}\\ u=0&\hbox{ on }\partial B(0,1)\end{array}\right.

admits a unique radial solution uC2(B(0,1){0})C(B(0,1)¯)u\in C^{2}(B(0,1)\setminus\{0\})\cap C(\overline{B(0,1)}) for any radial and continuous datum fB(0,1)¯f\in\overline{B(0,1)} satisfying f0f\leq 0.

Next, for the case γ=2\gamma=2 we have the following result, which gives explicit expressions for the eigenvalues and the eigenfunctions in case of Pucci’s operators.

Theorem 1.2.

Assume that γ=2\gamma=2. Then:

  • (i)

    For the operator +\mathcal{M}^{+} one has

    λ¯2(+)=Λ(N~+2)24\bar{\lambda}_{2}(\mathcal{M}^{+})=\Lambda\frac{(\tilde{N}_{+}-2)^{2}}{4}

    and the function u(x)=rN~+22(lnr)u(x)=r^{-\frac{\tilde{N}_{+}-2}{2}}(-\ln r) is an explicit solution of

    {+(D2u)+λ¯2ur2=0 in B(0,1){0}u=0 on B(0,1)\left\{\begin{array}[]{cl}\mathcal{M}^{+}(D^{2}u)+\bar{\lambda}_{2}\frac{u}{r^{2}}=0&\hbox{ in }\ B(0,1)\setminus\{0\}\\[4.30554pt] u=0&\hbox{ on }\ \partial B(0,1)\end{array}\right.

    Analogously, for the operator \mathcal{M}^{-} one has

    λ¯2()=λ(N~2)24\bar{\lambda}_{2}(\mathcal{M}^{-})=\lambda\frac{(\tilde{N}_{-}-2)^{2}}{4}

    and the function u(x)=rN~22(lnr)u(x)=r^{-\frac{\tilde{N}_{-}-2}{2}}(-\ln r) is an explicit solution of

    {(D2u)+λ¯2ur2=0 in B(0,1){0}u=0 on B(0,1)\left\{\begin{array}[]{cl}\mathcal{M}^{-}(D^{2}u)+\bar{\lambda}_{2}\frac{u}{r^{2}}=0&\hbox{ in }\ B(0,1)\setminus\{0\}\\[4.30554pt] u=0&\hbox{ on }\ \partial B(0,1)\end{array}\right.
  • (ii)

    The eigenvalues λ¯2(±)\bar{\lambda}_{2}(\mathcal{M}^{\pm}) are stable under various regularization

    λ¯2(±)=limγ2λ¯γ(±)\bar{\lambda}_{2}(\mathcal{M}^{\pm})=\lim_{\gamma\rightarrow 2}\bar{\lambda}_{\gamma}(\mathcal{M}^{\pm})
    λ¯2(±)=limδ0λ¯(±,B(0,1)B(0,δ)¯)\bar{\lambda}_{2}(\mathcal{M}^{\pm})=\lim_{\delta\rightarrow 0}\bar{\lambda}(\mathcal{M}^{\pm},B(0,1)\setminus\overline{B(0,\delta)})
    λ¯2(±)=limϵ0λ¯(±,1(r2+ϵ2))\bar{\lambda}_{2}(\mathcal{M}^{\pm})=\lim_{\epsilon\rightarrow 0}\bar{\lambda}(\mathcal{M}^{\pm},\frac{1}{(r^{2}+\epsilon^{2})})
  • (iii)

    For any operator FF satisfying (1.4) and (1.6) one has

    Λ(N~+2)24λ¯2(F)λ(N~2)24.\Lambda\frac{(\tilde{N}_{+}-2)^{2}}{4}\leq\bar{\lambda}_{2}(F)\leq\lambda\frac{(\tilde{N}_{-}-2)^{2}}{4}\,.

We observe that we cannot prove the existence of eigenfunctions for a general operator FF, but we can merely provide the estimate on the eigenvalue given by statement (iii) above. Theorem 1.2 will be obtained by using a variational approach adapted to the fully nonlinear radial framework. Indeed, we will define variational eigenvalues associated with the operators ±\mathcal{M}^{\pm} in an analogous way as in (1.3), taking advantage of the radial symmetry of solutions. Then, the full statements of Theorem 1.2 will follow as consequences of the properties established for λ¯γ\bar{\lambda}_{\gamma} in the case γ<2\gamma<2 and the stability of the variational formulation as γ2\gamma\to 2.

Finally, for the case γ>2\gamma>2, the singularity of the coefficient is too strong and it prevents the existence of positive smooth super-solutions, as stated by the following non existence result.

Theorem 1.3.

If γ>2\gamma>2, then the eigenvalue λ¯γ\bar{\lambda}^{\prime}_{\gamma} defined by (1.9) satisfies λ¯γ=0\bar{\lambda}_{\gamma}^{\prime}=0.

Let us observe that, symmetrically, one could define the eigenvalue associated with negative eigenfunctions, by setting

λ¯γ=sup{μ:uC(B(0,1){0}),u<0 in B(0,1),F(D2u)+μurγ0}=0.\bar{\lambda}_{\gamma}^{-}=\sup\{\mu\,:\ \exists\,u\in C(B(0,1)\setminus\{0\})\,,\ u<0\hbox{ in }B(0,1),\ \ \ F(D^{2}u)+\mu\frac{u}{r^{\gamma}}\geq 0\}=0.

In this case, the results above can be extended to λ¯γ\bar{\lambda}_{\gamma}^{-} with obvious modifications.

Let us conclude this introduction by observing that, in case of semilinear or quasilinear equations, many existence, non existence and classification results have been obtained in presence of zero oder terms having Hardy’s potential perturbed with additional sub- or superlinear terms. In particular, we refer to [5, 6, 9, 22] for results related to Laplace operator, and to [16] for the pp-Laplace operator.

The case where, in all directions above, Δ\Delta or Δp\Delta_{p} is replaced by a non variational fully nonlinear operator will be the object of future works.

2 The case γ<2\gamma<2: proof of Theorem 1.1

Theorem 1.1 will be proved as a consequence of several classical steps: a comparison principle, existence and regularity results and a maximum principle ”below” the first eigenvalue.

2.1 Maximum principles, existence and regularity results

The first result of the present section is a crucial technical lemma.

Lemma 2.1.

Let fC(B(0,1){0})f\in C\left(B(0,1)\setminus\{0\}\right) be a radial, bounded and positive function and assume that uC2(B(0,1){0})u\in C^{2}\left(B(0,1)\setminus\{0\}\right) is a radial, bounded function satisfying

(2.1) +(D2u)frγ in B(0,1){0}.{\cal M}^{+}(D^{2}u)\geq fr^{-\gamma}\qquad\hbox{ in }B(0,1)\setminus\{0\}\,.

Then

  • (i)

    u0u^{\prime}\geq 0 in a right neighborhood of 00;

  • (ii)

    limr0u(r)rN~1=0\displaystyle\lim_{r\rightarrow 0}u^{\prime}(r)r^{{\tilde{N}}_{-}-1}=0 and in a right neighborhood of 00 one has

    u(r)inffΛ(N~γ)r1γ;u^{\prime}(r)\geq\frac{\inf f}{\Lambda({\tilde{N}}_{-}-\gamma)}r^{1-\gamma}\,;
  • (iii)

    if, furthermore, +(D2u)=frγ{\cal M}^{+}(D^{2}u)=fr^{-\gamma}, then, in a right neighborhood of 00, one has also

    u(r)supfλ(Nγ)r1γ.u^{\prime}(r)\leq\frac{\sup f}{\lambda(N-\gamma)}r^{1-\gamma}\,.

    In particular, there exists a constant c>0c>0 such that, for rr sufficiently small,

    |u(r)|cr1γ|u^{\prime}(r)|\leq cr^{1-\gamma}

    and then uu is locally Lipschitz continuous in B(0,1)B(0,1) if γ1\gamma\leq 1, it belongs to C1(B(0,1))C^{1}(B(0,1)) if γ<1\gamma<1, and it is locally Hölder continuous in B(0,1)B(0,1) with exponent 2γ2-\gamma if γ>1\gamma>1.

Proof.

Let us prove, by contradiction, that uu^{\prime} does not change sign in a right neighborhood of 0. If not, there exists a decreasing sequence {rn}\{r_{n}\} converging to 0, such that u(rn)=0u^{\prime}(r_{n})=0 for all nn, and u0u^{\prime}\leq 0 in ]r2n+1,r2n[]r_{2n+1},r_{2n}[, u0u^{\prime}\geq 0 in ]r2n+2,r2n+1[]r_{2n+2},r_{2n+1}[. Since u(r2n)=u(r2n+1)=0u^{\prime}(r_{2n})=u^{\prime}(r_{2n+1})=0, there exists some s2n]r2n+1,r2n[s_{2n}\in]r_{2n+1},r_{2n}[ such that u′′(s2n)=0u^{\prime\prime}(s_{2n})=0. This yields the contradiction

0λ(N1)u(s2n)s2n=+(D2u(s2n))f(s2n)s2nγ>0.0\geq\lambda(N-1)\frac{u^{\prime}(s_{2n})}{s_{2n}}=\mathcal{M}^{+}(D^{2}u(s_{2n}))\geq f(s_{2n})s_{2n}^{-\gamma}>0\,.

Next, arguing again by contradiction, if u(r)0u^{\prime}(r)\leq 0 for rr sufficiently small, then, by (2.1), one has u′′(r)>0u^{\prime\prime}(r)>0 and, in a right neighborhood of 00,

+(D2u)=Λu′′(r)+λ(N1)u(r)rf(r)rγ.\mathcal{M}^{+}(D^{2}u)=\Lambda u^{\prime\prime}(r)+\lambda(N-1)\frac{u^{\prime}(r)}{r}\geq f(r)r^{-\gamma}\,.

Hence,

(u(r)rN~+1)frN~+1γΛ>0(u^{\prime}(r)r^{{\tilde{N}}_{+}-1})^{\prime}\geq\frac{fr^{{\tilde{N}}_{+}-1-\gamma}}{\Lambda}>0

and, in particular, urN~+1u^{\prime}r^{{\tilde{N}}_{+}-1} is increasing in a right neighborhood of 00. Thus, limr0u(r)rN~+1\lim_{r\to 0}u^{\prime}(r)r^{{\tilde{N}}_{+}-1} exists and it is lesser than or equal to 0. If it was lesser than zero, then we would have, for some constant l>0l>0,

u(r)lr1N~+u^{\prime}(r)\leq-lr^{1-{\tilde{N}}_{+}}

in a right neighborhood of 00, yielding a contradiction to the boundedness of uu This shows that limr0u(r)rN~+1=0\lim_{r\to 0}u^{\prime}(r)r^{{\tilde{N}}_{+}-1}=0 and, by monotonicity, u(r)>0u^{\prime}(r)>0 in a right neighborhood of 00. The reached contradiction proves statement (i).

In order to prove (ii), let us observe that, for rr sufficiently small, by (2.1) we have either

u′′(r)+(N1)u(r)rf(r)rγΛu^{\prime\prime}(r)+(N-1)\frac{u^{\prime}(r)}{r}\geq\frac{f(r)r^{-\gamma}}{\Lambda}

if u′′(r)0u^{\prime\prime}(r)\geq 0, or

u′′(r)+(N~1)u(r)rf(r)rγλu^{\prime\prime}(r)+({\tilde{N}}_{-}-1)\frac{u^{\prime}(r)}{r}\geq\frac{f(r)r^{-\gamma}}{\lambda}

if u′′(r)0u^{\prime\prime}(r)\leq 0. Since u(r)0u^{\prime}(r)\geq 0 and N~N{\tilde{N}}_{-}\geq N, in both cases one has

u′′(r)+(N~1)u(r)rf(r)rγΛ,u^{\prime\prime}(r)+({\tilde{N}}_{-}-1)\frac{u^{\prime}(r)}{r}\geq\frac{f(r)r^{-\gamma}}{\Lambda}\,,

that is

(urN~1)f(r)rN~1γΛinffΛrN~1γ.(u^{\prime}r^{{\tilde{N}}_{-}-1})^{\prime}\geq\frac{f(r)r^{{\tilde{N}}_{-}-1-\gamma}}{\Lambda}\geq\frac{\inf f}{\Lambda}r^{{\tilde{N}}_{-}-1-\gamma}\,.

Arguing as above, we deduce that urN~1u^{\prime}r^{{\tilde{N}}_{-}-1} is increasing in a right neighborhood of 00, hence it has a nonnegative limit as r0r\to 0, and such a limit must be 00, since uu is bounded. Moreover, by integrating the above inequality, we obtain

u(r)inffΛ(N~γ)r1γ.u^{\prime}(r)\geq\frac{\inf f}{\Lambda({\tilde{N}}_{-}-\gamma)}r^{1-\gamma}\,.

Let us finally prove (iii). Assuming that +(D2u)=f(r)rγ\mathcal{M}^{+}(D^{2}u)=f(r)r^{-\gamma} and using statement (i), it follows that, for every r>0r>0 sufficiently small, one has either

u′′(r)+(N1)u(r)r=f(r)rγΛu^{\prime\prime}(r)+(N-1)\frac{u^{\prime}(r)}{r}=\frac{f(r)r^{-\gamma}}{\Lambda}

or

u′′(r)+(N~1)u(r)r=f(r)rγλ.u^{\prime\prime}(r)+({\tilde{N}}_{-}-1)\frac{u^{\prime}(r)}{r}=\frac{f(r)r^{-\gamma}}{\lambda}\,.

In both cases, we deduce

u′′(r)+(N1)u(r)rf(r)rγλ,u^{\prime\prime}(r)+(N-1)\frac{u^{\prime}(r)}{r}\leq\frac{f(r)r^{-\gamma}}{\lambda}\,,

which yields

(u(r)rN1)f(r)λrN1γsupfλrN1γ.(u^{\prime}(r)r^{N-1})^{\prime}\leq\frac{f(r)}{\lambda}r^{N-1-\gamma}\leq\frac{\sup f}{\lambda}r^{N-1-\gamma}\,.

Hence, u(r)rN1supfλ(Nγ)rNγu^{\prime}(r)r^{N-1}-\frac{\sup f}{\lambda(N-\gamma)}r^{N-\gamma} is non increasing in a right neighborhood of 00 and it has a limit as r0r\to 0. This implies that u(r)rN1u^{\prime}(r)r^{N-1} has a limit as r0r\to 0 as well, and such a limit is zero by the boundedness of uu. By integrating the last inequality, we finally deduce

u(r)supfλ(Nγ)r1γ.u^{\prime}(r)\leq\frac{\sup f}{\lambda(N-\gamma)}r^{1-\gamma}\,.

The regularity of uu at zero is then a consequence of the estimate |u(r)|cr1γ|u^{\prime}(r)|\leq cr^{1-\gamma}. Elsewhere, it follows from the assumption uC2(B(0,1){0})u\in C^{2}(B(0,1)\setminus\{0\}).

Remark 2.2.

By using the change of variable v=uv=-u, one gets that if fC(B(0,1){0})f\in C\left(B(0,1)\setminus\{0\}\right) is a radial, bounded and positive function and uC2(B(0,1){0})u\in C^{2}\left(B(0,1)\setminus\{0\}\right) is a bounded radial function satisfying

(D2u)frγ in B(0,1){0},{\cal M}^{-}(D^{2}u)\leq-fr^{-\gamma}\quad\hbox{ in }B(0,1)\setminus\{0\}\,,

then, for rr sufficiently small, u(r)0u^{\prime}(r)\leq 0, limr0u(r)rN~1=0\lim_{r\to 0}u^{\prime}(r)r^{{\tilde{N}_{-}-1}}=0 and

u(r)inffΛ(N~γ)r1γ.u^{\prime}(r)\leq-\frac{\inf f}{\Lambda({\tilde{N}}_{-}-\gamma)}r^{1-\gamma}\,.

Moreover, if (D2u)=frγ in B(0,1){0}{\cal M}^{-}(D^{2}u)=-fr^{-\gamma}\quad\hbox{ in }B(0,1)\setminus\{0\}, then |u(r)|cr1γ|u^{\prime}(r)|\leq cr^{1-\gamma} for a positive constant cc. Hence uu is locally Lipschitz continuous in B(0,1)B(0,1) for γ1\gamma\leq 1, it belongs to C1(B(0,1))C^{1}(B(0,1)) if γ<1\gamma<1, and it is locally Hölder continuous in B(0,1)B(0,1) with exponent 2γ2-\gamma for γ>1\gamma>1.

Obviously, since +{\cal M}^{-}\leq{\cal M}^{+}, one gets an analogous conclusion when

+(D2u)frγ.{\cal M}^{+}(D^{2}u)\leq-fr^{-\gamma}.

We can now prove a comparison principle for general radial fully nonlinear singular equations of the form

F(D2u)βurγ=f(r)rγ in B(0,1){0}F(D^{2}u)-\beta ur^{-\gamma}=f(r)r^{-\gamma}\quad\hbox{ in }B(0,1)\setminus\{0\}

when no boundary condition at the origin is assumed.

Theorem 2.3.

Let f,gC(B(0,1))f,g\in C\left(B(0,1)\right) be radial functions and assume that u,vC(B(0,1)¯)C2(B(0,1){0})u,v\in C\left(\overline{B(0,1)}\right)\cap C^{2}(B(0,1)\setminus\{0\}) are radial functions satisfying in B(0,1){0}B(0,1)\setminus\{0\}

F(D2u)βu(r)rγf(r)rγF(D2v)βv(r)rγg(r)rγ\begin{array}[]{c}F(D^{2}u)-\beta u(r)r^{-\gamma}\geq f(r)r^{-\gamma}\\[8.61108pt] F(D^{2}v)-\beta v(r)r^{-\gamma}\leq g(r)r^{-\gamma}\end{array}

with β0\beta\geq 0 and fgf\geq g in B(0,1)B(0,1). Then, uvu\leq v on B(0,1)\partial B(0,1) implies uvu\leq v in B(0,1)¯\overline{B(0,1)}.

Proof.

Let us first consider the case in which either β>0\beta>0 or f>gf>g in B(0,1)B(0,1). We suppose by contradiction that

maxB(0,1)¯(uv)>0.\max_{\overline{B(0,1)}}(u-v)>0\,.

If the maximum is achieved at 0, then (uv)(0)>0(u-v)(0)>0 and, by the assumptions on ff, gg and β\beta, there exist δ>0\delta>0 and a neighborhood on the right of 00 on which

(β(u(r)v(r))+f(r)g(r))rγδrγ>0(\beta(u(r)-v(r))+f(r)-g(r))r^{-\gamma}\geq\delta r^{-\gamma}>0

By the uniform ellipticity of FF, we then obtain for rr sufficiently small

+(D2(uv))δrγ{\cal M}^{+}(D^{2}(u-v))\geq\delta r^{-\gamma}

Using Lemma 2.1 for uvu-v, one gets that for some positive constant cc, (uv)cδr1γ(u-v)^{\prime}\geq c\delta r^{1-\gamma}, which contradicts the fact that uvu-v attains its maximum at 00. Hence, there exists 0<r¯<10<\bar{r}<1 such that u(r¯)v(r¯)=max(uv)u(\bar{r})-v(\bar{r})=\max(u-v). Then, (D2uD2v)(r¯)0(D^{2}u-D^{2}v)(\bar{r})\leq 0 and, by ellipticity, we get the contradiction

(f(r¯)+βu(r¯))rγF(D2u(r¯))F(D2v(r¯))(g(r¯)+βv(r¯))rγ.(f(\bar{r})+\beta u(\bar{r}))r^{-\gamma}\leq F(D^{2}u(\bar{r}))\leq F(D^{2}v(\bar{r}))\leq(g(\bar{r})+\beta v(\bar{r}))r^{-\gamma}\,.

For the case β=0\beta=0 and fgf\geq g, let us introduce the radial function

w(r)=1rτw(r)=1-r^{\tau}

with 0<τ2γ0<\tau\leq 2-\gamma. A direct computation shows that

+(D2w)τΛ(|τ1|(N~+1))rτ2.\mathcal{M}^{+}(D^{2}w)\leq\tau\Lambda(|\tau-1|-(\tilde{N}_{+}-1))r^{\tau-2}\,.

We observe that |τ1|<1<N~+1|\tau-1|<1<\tilde{N}_{+}-1, so that

+(D2w)Crγ in B(0,1){0}\mathcal{M}^{+}(D^{2}w)\leq-Cr^{-\gamma}\qquad\hbox{ in }B(0,1)\setminus\{0\}

with C=τΛ(N~+1|τ1|)>0C=\tau\Lambda(\tilde{N}_{+}-1-|\tau-1|)>0. Thus, for any ϵ>0\epsilon>0, we have

F(D2(uϵw))F(D2u)ϵ+(D2w)(f+ϵC)rγ.F(D^{2}(u-\epsilon w))\geq F(D^{2}u)-\epsilon\,\mathcal{M}^{+}(D^{2}w)\geq(f+\epsilon\,C)r^{-\gamma}\,.

Since f+ϵC>gf+\epsilon\,C>g and uϵw=uvu-\epsilon w=u\leq v on B(0,1)\partial B(0,1), the previous argument proves that

uϵwv in B(0,1)¯u-\epsilon w\leq v\qquad\hbox{ in }\overline{B(0,1)}

and the conclusion follows by letting ϵ0\epsilon\to 0.

Remark 2.4.

The auxiliary function introduced in the proof of Theorem 2.3 shows that there exist a radial function wC2(B(0,1){0})w\in C^{2}(B(0,1)\setminus\{0\}), strictly positive in B(0,1){0}B(0,1)\setminus\{0\}, such that

F(D2w)cwrγ in B(0,1){0}F(D^{2}w)\leq-cwr^{-\gamma}\qquad\hbox{ in }B(0,1)\setminus\{0\}

for a constant c>0c>0. This proves that λ¯γ(F)λ¯γ(F)c>0\bar{\lambda}_{\gamma}(F)\geq\bar{\lambda}_{\gamma}^{\prime}(F)\geq c>0.

Next, we have the following existence, uniqueness and regularity result.

Theorem 2.5.

Let fC(B(0,1))f\in C(B(0,1)) be a radial, bounded function. For β0\beta\geq 0 and bb\in\mathbb{R} there exists a unique bounded radial function uC(B(0,1)¯{0})C2(B(0,1){0})u\in C(\overline{B(0,1)}\setminus\{0\})\cap C^{2}(B(0,1)\setminus\{0\}) satisfying

(2.2) {F(D2u)βurγ=rγf(r) in B(0,1){0}u=b on B(0,1)\left\{\begin{array}[]{cc}F(D^{2}u)-\beta{ur^{-\gamma}}=r^{-\gamma}f(r)&\hbox{ in }\ B(0,1)\setminus\{0\}\\ u=b&\hbox{ on }\ \partial B(0,1)\end{array}\right.

Moreover, uu can be extended up to B(0,1)¯\overline{B(0,1)}, and one has: uC1(B(0,1)¯)u\in C^{1}(\overline{B(0,1)}) if γ<1\gamma<1, uu is Lipschitz continuous in B(0,1)¯\overline{B(0,1)} if γ1\gamma\leq 1, uu is Hölder continuous in B(0,1)¯\overline{B(0,1)} with exponent 2γ2-\gamma if γ>1\gamma>1.

Proof.

For every nn\in{\mathbb{N}} let us introduce the regularized Dirichlet boundary value problem

(2.3) {F(D2un)βun(r2+1/n)γ/2=(r2+1/n)γ/2f(r) in B(0,1)un=b on B(0,1)\left\{\begin{array}[]{cl}F(D^{2}u_{n})-\beta{u_{n}(r^{2}+1/n)^{-\gamma/2}}=(r^{2}+1/n)^{-\gamma/2}f(r)&\hbox{ in }\ B(0,1)\\ u_{n}=b&\hbox{ on }\ \partial B(0,1)\end{array}\right.

which, by standard viscosity solutions theory, see [13], has a unique solution unC(B(0,1)¯)u_{n}\in C(\overline{B(0,1)}). By the symmetry results of [14], it follows that unu_{n} is radial, hence, as a solution of the associated ODE, unu_{n} belongs to C2(B(0,1))C^{2}(B(0,1)).

For 0<τ2γ0<\tau\leq 2-\gamma, let us consider the radial function

w(r)=L(1rτ)+b,w(r)=L(1-r^{\tau})+b\,,

where L>0L>0 is a constant to be suitably chosen. The same computation used in the proof of Theorem 2.3 yields

+(D2w)LCrγLC(r2+1/n)γ/2,\mathcal{M}^{+}(D^{2}w)\leq-L\,Cr^{-\gamma}\leq-L\,C(r^{2}+1/n)^{-\gamma/2}\,,

and then, by uniform ellipticity, it follows that

F(D2w)βwrγ(LC+βb)(r2+1/n)γ/2f(r)(r2+1/n)γ/2F(D^{2}w)-\beta wr^{-\gamma}\leq(-L\,C+\beta b^{-})(r^{2}+1/n)^{-\gamma/2}\leq f(r)(r^{2}+1/n)^{-\gamma/2}

as soon as CC is chosen large enough. Analogously, for some convenient positive constant LL, the function L(1rτ)+b-L(1-r^{\tau})+b is a radial sub-solution of problem (2.3).

The standard comparison principle then implies that the sequence {un}\{u_{n}\} is uniformly bounded in C(B(0,1)¯)C(\overline{B(0,1)}). Hence, it is locally uniformly bounded in C2(B(0,1){0})C^{2}(B(0,1)\setminus\{0\}) and, up to a subsequence, it is converging locally uniformly in B(0,1)¯{0}\overline{B(0,1)}\setminus\{0\} to a radial solution uu of problem (2.2), which is a globally bounded function belonging to C2(B(0,1){0})C^{2}(B(0,1)\setminus\{0\}).

Let us now show that the constructed bounded radial solution uu is actually continuous in the whole ball B(0,1)¯\overline{B(0,1)}. Indeed, the same approximation argument used in order to prove the existence of uu can be applied, in particular, in order to show the existence of a radial bounded solution w¯\bar{w} of the Dirichlet problem

{+(D2w¯)=(f+B+1)rγ in B(0,1){0}w¯=u on B(0,1)\left\{\begin{array}[]{cl}{\cal M}^{+}(D^{2}\bar{w})=-(\|f\|_{\infty}+B+1)r^{-\gamma}&\quad\hbox{ in }B(0,1)\setminus\{0\}\\ \bar{w}=u&\quad\hbox{ on }\partial B(0,1)\end{array}\right.

where B>0B>0 is a constant such that β|u|B\beta|u|\leq B in B(0,1)B(0,1). Lemma 2.1 and Remark 2.2 applied to w¯\bar{w} yield that

|w¯|cr1γ|\bar{w}^{\prime}|\leq cr^{1-\gamma}

for some c>0c>0. As a consequence, we have

+(D2(uw¯))F(D2(uw¯))F(D2u)+(D2w¯)rγ in B(0,1){0}{\cal M}^{+}(D^{2}(u-\bar{w}))\geq F(D^{2}(u-\bar{w}))\geq F(D^{2}u)-\mathcal{M}^{+}(D^{2}\bar{w})\geq r^{-\gamma}\qquad\hbox{ in }B(0,1)\setminus\{0\}

and then, by Lemma 2.1 (i), in a right neighborhood of zero one has (uw¯)(r)0.(u-\bar{w})^{\prime}(r)\geq 0\,. Hence,

u(r)cr1γu^{\prime}(r)\geq-cr^{1-\gamma}

for rr small enough. Analogously, we have

(D2(u+w¯))F(D2(u+w¯))F(D2u)++(D2w¯)rγ in B(0,1){0}{\cal M}^{-}(D^{2}(u+\bar{w}))\leq F(D^{2}(u+\bar{w}))\leq F(D^{2}u)+\mathcal{M}^{+}(D^{2}\bar{w})\leq-r^{-\gamma}\qquad\hbox{ in }B(0,1)\setminus\{0\}

which implies, by Remark 2.2,

u(r)w¯cr1γu^{\prime}(r)\leq-{\bar{w}}^{\prime}\leq cr^{1-\gamma}

for rr small enough. Arguing as in the proof of Lemma 2.1, from the estimate |u(r)|cr1γ|u^{\prime}(r)|\leq cr^{1-\gamma} for rr sufficiently small, we deduce that uu is Lipschitz continuous in B(0,1)¯\overline{B(0,1)} if γ1\gamma\leq 1, it belongs to C1(B(0,1)¯)C^{1}(\overline{B(0,1)}) if γ<1\gamma<1, and it is Hölder continuous in B(0,1)¯\overline{B(0,1)} with exponent 2γ2-\gamma if γ>1\gamma>1.

Let us observe that the argument above shows that any bounded radial solution of problem (2.2) is continuous in B(0,1)¯\overline{B(0,1)}. This, jointly with Theorem 2.3, implies that problem (2.2) has a unique radial bounded solution.

The argument used in the above proof yields also the following compactness result, which we state separately for the sake of clarity.

Theorem 2.6.

Let {un}n\{u_{n}\}_{n} be a uniformly bounded sequence of radial functions belonging to C2(B(0,1){0})C^{2}(B(0,1)\setminus\{0\}) and satisfying

F(D2un)=fnrγ in B(0,1){0},F(D^{2}u_{n})={f_{n}r^{-\gamma}}\qquad\hbox{ in }B(0,1)\setminus\{0\}\,,

where {fn}n\{f_{n}\}_{n} are radial, bounded and continuous on B(0,1){0}B(0,1)\setminus\{0\}. If {fn}\{f_{n}\} is uniformly bounded, then {un}n\{u_{n}\}_{n} are equicontinuous, thus uniformly converging in B(0,1)¯\overline{B(0,1)} up to a subsequence. If {fn}\{f_{n}\} is uniformly converging to fC(B(0,1)¯)f\in C(\overline{B(0,1)}), then, up to a subsequence, {un}n\{u_{n}\}_{n} is uniformly converging to a radial solution uC2(B(0,1){0})C(B(0,1)¯)u\in C^{2}(B(0,1)\setminus\{0\})\cap C(\overline{B(0,1)}) of

F(D2u)=rγf in B(0,1){0}.F(D^{2}u)={r^{-\gamma}f}\qquad\hbox{ in }B(0,1)\setminus\{0\}\,.

In the next results, we prove several properties of the “smooth” eigenvalue

λ¯γ:=sup{μ:uC2(B(0,1){0}),u>0 in B(0,1){0},u radial,F(D2u)+μurγ0}.\bar{\lambda}_{\gamma}^{\prime}\,:=\sup\{\mu\,:\ \exists\,u\in C^{2}(B(0,1)\setminus\{0\})\,,\ u>0\hbox{ in }B(0,1)\setminus\{0\},\ u\hbox{ radial},\ \ F(D^{2}u)+\mu\frac{u}{r^{\gamma}}\leq 0\}\,.

In Subsection 2.3 we will prove in facts that λ¯γ=λ¯γ\bar{\lambda}_{\gamma}^{\prime}=\bar{\lambda}_{\gamma}.

Let us start by proving the validity of the maximum principle below the value λ¯γ\bar{\lambda}_{\gamma}^{\prime}.

Theorem 2.7.

Let μ<λ¯γ\mu<\bar{\lambda}_{\gamma}^{\prime} and suppose that uC(B(0,1)¯)C2(B(0,1){0})u\in C(\overline{B(0,1)})\cap C^{2}(B(0,1)\setminus\{0\}) is a radial function satisfying

F(D2u)+μurγ0 in B(0,1){0}.F(D^{2}u)+\mu ur^{-\gamma}\geq 0\qquad\hbox{ in }\ B(0,1)\setminus\{0\}\,.

If u(1)0u(1)\leq 0, then u0u\leq 0 in B(0,1)¯\overline{B(0,1)}.

Proof.

If μ<0\mu<0, we just apply Theorem 2.3 with vgf0v\equiv g\equiv f\equiv 0. So, we can assume without loss of generality that μ0\mu\geq 0.

For μ]μ,λ¯γ[\mu^{\prime}\in]\mu,\bar{\lambda}_{\gamma}^{\prime}[, let vC2(B(0,1){0})v\in C^{2}(B(0,1)\setminus\{0\}) be a radial function satisfying

F(D2v)+μvrγ0,v>0 in B(0,1){0}.F(D^{2}v)+\mu^{\prime}vr^{-\gamma}\leq 0\,,\quad v>0\qquad\hbox{ in }B(0,1)\setminus\{0\}\,.

We can assume without loss of generality that v>0v>0 on B(0,1)\partial B(0,1), e.g. by performing a dilation in rr (this may change a little μ\mu^{\prime} but we can still suppose by continuity that μ]μ,λ¯γ[\mu^{\prime}\in]\mu,\bar{\lambda}_{\gamma}^{\prime}[). Arguing as in the proof of Lemma 2.1, since (D2v)+μvrγ0{\cal M}^{-}(D^{2}v)+\mu^{\prime}vr^{-\gamma}\leq 0, we easily obtain that v(r)v^{\prime}(r) has constant sign near zero. Assuming by contradiction that v(r)0v^{\prime}(r)\geq 0 in a neighborhood of zero, then vv is bounded in B(0,1){0}B(0,1)\setminus\{0\}. Hence, Remark 2.2 applies and yields v(r)0v^{\prime}(r)\leq 0 for rr small enough: a contradiction. This shows that v(r)0v^{\prime}(r)\leq 0 in a neighborhood of 00.

Then, there are two possible cases: either limr0v(r)=+\lim_{r\to 0}v(r)=+\infty or vv can be extended as a continuous function on B(0,1)¯\overline{B(0,1)}. In the first case, by applying the standard comparison principle, it is easy to prove that for all ϵ>0\epsilon>0 one has uϵvu\leq\epsilon v in B(0,1)¯{0}\overline{B(0,1)}\setminus\{0\}. In this case, letting ϵ0\epsilon\to 0, we get the conclusion. On the other hand, if vv is bounded and continuous on B(0,1)¯\overline{B(0,1)}, we can argue by contradiction. Let us assume that uu is positive somewhere in B(0,1)B(0,1), so that uv\frac{u}{v} has a positive maximum on B(0,1)¯\overline{B(0,1)}, achieved at some point inside B(0,1)B(0,1). Up to a multiplicative constant for vv, we can suppose that

maxB(0,1)¯uv=1,\max_{\overline{B(0,1)}}\frac{u}{v}=1\,,

so that u(r)v(r)u(r)\leq v(r). If the maximum is achieved at 00, then one has u(0)=v(0)>0.u(0)=v(0)>0\,. By continuity, for rr small enough one has

+(D2(uv))F(D2u)F(D2v)12(μv(0)μu(0))rγ.{\cal M}^{+}(D^{2}(u-v))\geq F(D^{2}u)-F(D^{2}v)\geq\frac{1}{2}(\mu^{\prime}v(0)-\mu u(0))r^{-\gamma}\,.

Since μv(0)μu(0)=(μμ)v(0)>0\mu^{\prime}v(0)-\mu u(0)=(\mu^{\prime}-\mu)v(0)>0, we can use Lemma 2.1 (ii) and we get that (uv)(r)>0(u-v)^{\prime}(r)>0 in a right neighborhood of 00. This is a contradiction to uvu-v has a maximum point at zero.

Hence, we have that 1=maxuv>u(0)v(0)1=\max\frac{u}{v}>\frac{u(0)}{v(0)}. Let us select η<1\eta<1 such that η>max{μμ,u(0)v(0)}\eta>\max\{\frac{\mu}{\mu^{\prime}},\frac{u(0)}{v(0)}\}. Then, the function uηvu-\eta v has a positive maximum achieved at some point 0<r¯<10<\bar{r}<1.

Since D2u(r¯)ηD2v(r¯)D^{2}u(\bar{r})\leq\eta D^{2}v(\bar{r}), by ellipticity and using (1.6), we get

μv(r¯)r¯γμu(r¯)r¯γF(D2u(r¯))F(ηD2v(r¯))μηv(r¯)r¯γ,-\mu v(\bar{r}){\bar{r}}^{-\gamma}\leq-\mu u(\bar{r}){\bar{r}}^{-\gamma}\leq F(D^{2}u(\bar{r}))\leq F(\eta D^{2}v(\bar{r}))\leq-\mu^{\prime}\eta\,v(\bar{r}){\bar{r}}^{-\gamma}\,,

which gives the contradiction μμη\mu\geq\mu^{\prime}\eta.

The next result provides the existence, uniqueness and regularity of solutions below the eigenvalue λ¯γ\bar{\lambda}_{\gamma}^{\prime}.

Theorem 2.8.

Let ff be a radial and continuous function in B(0,1)¯\overline{B(0,1)} satisfying f0f\leq 0, with ff not identically zero. Then, for every μ<λ¯γ\mu<\bar{\lambda}_{\gamma}^{\prime} there exists a unique, bounded, radial function uC2(B(0,1){0})u\in C^{2}(B(0,1)\setminus\{0\}) satisfying

{F(D2u)+μurγ=f(r)rγ in B(0,1){0}u=0 on B(0,1)\left\{\begin{array}[]{cl}F(D^{2}u)+\mu ur^{-\gamma}=f(r)r^{-\gamma}&\hbox{ in }B(0,1)\setminus\{0\}\\ u=0&\hbox{ on }\partial B(0,1)\end{array}\right.

Moreover, uu can be extended as a strictly positive continuous function in B(0,1)B(0,1), Lipschitz continuous in B(0,1)¯\overline{B(0,1)} if γ1\gamma\leq 1, (2γ)(2-\gamma)-Hölder continuous in B(0,1)¯\overline{B(0,1)} if γ>1\gamma>1.

Proof.

As in the proof of Theorem 2.7, we can assume without loss of generality that μ>0\mu>0, otherwise the conclusion just follows from Theorem 2.5. The uniqueness of uu follows from Theorem 2.7.

As far as existence is concerned, let us recursively define a sequence {un}n0\{u_{n}\}_{n\geq 0} as follows: we set

u00,u_{0}\equiv 0\,,

and then, by using Theorem 2.5, we define un+1C2(B(0,1){0})C(B(0,1)¯)u_{n+1}\in C^{2}(B(0,1)\setminus\{0\})\cap C(\overline{B(0,1)}) as the unique bounded radial solution of

{F(D2un+1)=(fμun)rγ in B(0,1){0}un+1=0 on B(0,1)\left\{\begin{array}[]{cc}F(D^{2}u_{n+1})=(f-\mu u_{n})r^{-\gamma}&\hbox{ in }B(0,1)\setminus\{0\}\\ u_{n+1}=0&\hbox{ on }\partial B(0,1)\end{array}\right.

By Theorem 2.3, we have that un+10u_{n+1}\geq 0, hence it is strictly positive in B(0,1){0}B(0,1)\setminus\{0\} by the standard strong maximum principle, since ff is not identically zero. In particular, unu_{n} is not identically zero for all n1n\geq 1. By applying the comparison principle in Theorem 2.3 again, we deduce also that un+1unu_{n+1}\geq u_{n}. Let us prove that {un}n\{u_{n}\}_{n} is uniformly bounded. If not, by setting vn=un1unv_{n}={\|u_{n}\|_{\infty}}^{-1}u_{n} and kn=un+11un1k_{n}=\|u_{n+1}\|_{\infty}^{-1}\|u_{n}\|_{\infty}\leq 1, one gets that vn+1v_{n+1} satisfies

{F(D2vn+1)=(f(r)un+1μknvn(r))rγ in B(0,1){0}vn+1=0 on B(0,1)\left\{\begin{array}[]{cc}F(D^{2}v_{n+1})=\left(\frac{f(r)}{\|u_{n+1}\|_{\infty}}-\mu k_{n}v_{n}(r)\right)r^{-\gamma}&\hbox{ in }B(0,1)\setminus\{0\}\\ v_{n+1}=0&\hbox{ on }\partial B(0,1)\end{array}\right.

Since {vn}n\{v_{n}\}_{n} is uniformly bounded, by applying Theorem 2.6, we can extract a subsequence still denoted by {vn}n\{v_{n}\}_{n} uniformly converging to a function v0v\geq 0 satisfying

{F(D2v)+μkvrγ=0 in B(0,1){0}v=0 on B(0,1)\left\{\begin{array}[]{cc}F(D^{2}v)+\mu kvr^{-\gamma}=0&\hbox{ in }B(0,1)\setminus\{0\}\\ v=0&\hbox{ on }\partial B(0,1)\end{array}\right.

where k1k\leq 1 is the limit of some converging subsequence of {kn}n\{k_{n}\}_{n}. Since vv is a radial solution, one has that vC2(B(0,1){0})v\in C^{2}(B(0,1)\setminus\{0\}) and, since μkμ<λ¯γ\mu k\leq\mu<\bar{\lambda}_{\gamma}^{\prime}, Theorem 2.7 yields v0v\leq 0. Hence, we get v0v\equiv 0, a contradiction with v=1\|v\|_{\infty}=1.

We have obtained that {un}n\{u_{n}\}_{n} is bounded, and using once more Theorem 2.6, we deduce that {un}\{u_{n}\} uniformly converges to some uu, which satisfies the desired equation. By the strong maximum principle, we get that u>0u>0 in B(0,1){0}B(0,1)\setminus\{0\}. Moreover, by Remark 2.2, we have that u(r)0u^{\prime}(r)\leq 0 for r>0r>0 small enough, which implies u(0)>0u(0)>0. Finally, the global regularity of uu follows from Theorem 2.5.

We can now prove that the smooth eigenvalue λ¯γ\bar{\lambda}_{\gamma}^{\prime} is actually achieved on smooth eigenfunctions.

Theorem 2.9.

There exists uC(B(0,1)¯)C2(B(0,1){0})u\in C(\overline{B(0,1)})\cap C^{2}(B(0,1)\setminus\{0\}), radial, strictly positive in B(0,1)B(0,1) and satisfying

{F(D2u)+λ¯γurγ=0 in B(0,1){0}u=0 on B(0,1)\left\{\begin{array}[]{cl}F(D^{2}u)+\bar{\lambda}_{\gamma}^{\prime}ur^{-\gamma}=0&\hbox{ in }B(0,1)\setminus\{0\}\\ u=0&\hbox{ on }\partial B(0,1)\end{array}\right.

Furthermore, in B(0,1)¯\overline{B(0,1)}, uu is Lipschitz continuous when γ1\gamma\leq 1 and Hölder continuous with exponent 2γ2-\gamma if γ>1\gamma>1.

Proof.

We consider a sequence {λn}\{\lambda_{n}\}, with λnλ¯γ\lambda_{n}\rightarrow\bar{\lambda}_{\gamma}^{\prime} and λn<λ¯γ\lambda_{n}<\bar{\lambda}_{\gamma}^{\prime} and, for all nn, the solution unC(B(0,1)¯)C2(B(0,1){0})u_{n}\in C(\overline{B(0,1)})\cap C^{2}(B(0,1)\setminus\{0\}) provided by Theorem 2.8 of

F(D2un)+λnunrγ=rγ,un(1)=0.F(D^{2}u_{n})+\lambda_{n}u_{n}r^{-\gamma}={-r^{-\gamma}},\quad u_{n}(1)=0\ .

We claim that the positive sequence {un}n\{\|u_{n}\|_{\infty}\}_{n} is unbounded. Indeed, arguing by contradiction, if {un}n\{u_{n}\}_{n} is uniformly bounded, then, by using Theorem 2.6 and considering a subsequence if necessary, we obtain that there exists a solution uC(B(0,1)¯)C2(B(0,1){0})u\in C(\overline{B(0,1)})\cap C^{2}(B(0,1)\setminus\{0\}), u0u\geq 0, of

F(D2u)+λ¯γurγ=rγ,u(1)=0.F(D^{2}u)+\bar{\lambda}_{\gamma}^{\prime}ur^{-\gamma}={-r^{-\gamma}},\quad u(1)=0\,.

Then, arguing as in the proof of Theorem 2.8, we deduce that uu is strictly positive in B(0,1)B(0,1), and by taking 0<ϵ<1u0<\epsilon<\frac{1}{\|u\|_{\infty}}, we see that uu satisfies

F(D2u)+(λ¯γ+ϵ)urγ0,F(D^{2}u)+(\bar{\lambda}_{\gamma}^{\prime}+\epsilon)ur^{-\gamma}\leq 0,

a contradiction to the definition of λ¯γ\bar{\lambda}_{\gamma}^{\prime}. It then follows that the sequence {un}n\{u_{n}\}_{n} is not uniformly bounded. Normalizing and considering a subsequence, letting nn\to\infty yields the existence of uC(B(0,1)¯)C2(B(0,1){0})u\in C(\overline{B(0,1)})\cap C^{2}(B(0,1)\setminus\{0\}) satisfying

F(D2u)+λ¯γurγ=0,inB(0,1){0},u(1)=0.F(D^{2}u)+\bar{\lambda}_{\gamma}^{\prime}ur^{-\gamma}=0,\ {\rm in}\ B(0,1)\setminus\{0\}\ ,u(1)=0\ .

Finally, the strict positivity of uu in B(0,1)B(0,1) and its global regularity in B(0,1)¯\overline{B(0,1)} follow by arguing as in the proof of Theorem 2.8.

The uniqueness, up to positive multiplicative constants, of the solution given by Theorem 2.9 is provided by the last result of the present section.

Proposition 2.10.

The eigenvalue λ¯γ\bar{\lambda}_{\gamma}^{\prime} is simple.

Proof.

From Theorem 2.9, there exists a bounded eigenfunction vv. Let uu be another eigenfunction.

We define η:=sup{t>0,tv<u}\eta\,:=\sup\{t>0,tv<u\}, or, equivalently, 1η=supB(0,1){0}vu\frac{1}{\eta}=\sup_{B(0,1)\setminus\{0\}}\frac{v}{u}, which is well defined by Hopf Lemma applied to uu and vv on B(0,1)\partial B(0,1). Then, the function uηvu-\eta v is nonnegative in B(0,1)¯{0}\overline{B(0,1)}\setminus\{0\} and it satisfies

(D2(uηv))0 in B(0,1){0}.{\cal M}^{-}(D^{2}(u-\eta v))\leq 0\qquad\hbox{ in }B(0,1)\setminus\{0\}\,.

If, by contradiction, uηv>0u-\eta v>0 at some point in B(0,1){0}B(0,1)\setminus\{0\}, then, by the strong maximum principle, uηv>0u-\eta v>0 in the whole of B(0,1){0}B(0,1)\setminus\{0\}.

We now distinguish the cases u(0)u(0) finite or infinite.

- In the case u(0)=+u(0)=+\infty, one necessarily has

1η=limr1vu=v(1)u(1)\frac{1}{\eta}=\lim_{r\rightarrow 1}\frac{v}{u}=\frac{v^{\prime}(1)}{u^{\prime}(1)}

but this contradicts Hopf’s Lemma.

- If u(0)<u(0)<\infty, we have either 1η=limr1vu=v(1)u(1)\frac{1}{\eta}=\lim_{r\rightarrow 1}\frac{v}{u}=\frac{v^{\prime}(1)}{u^{\prime}(1)} or 1η=v(0)u(0)\frac{1}{\eta}=\frac{v(0)}{u(0)}. Here, the contradiction follows either from Hopf’s Lemma or from Remark 2.2, which gives (uηv)(r)0(u-\eta v)^{\prime}(r)\leq 0 for r>0r>0 sufficiently small, so that uηvu-\eta v cannot have a strict minimum point at zero.

Thus, we have obtained that all the eigenfunctions are bounded and multiple of each others.

2.2 The eigenvalue inherited from some equation on +\mathbb{R}^{+}

We suppose in this section that FF is one of Pucci’s operators. We consider only the case F=+F=\mathcal{M}^{+}, the changes to bring for F=F=\mathcal{M}^{-} being obvious.

We present below an alternative proof of the existence of radial eigenfunctions related to the eigenvalue λ¯γ\bar{\lambda}_{\gamma}. Here, the idea is to show the existence of global solutions defined in (0,+)(0,+\infty) of the ODE associated with radial solutions of the equation

+(D2u)=urγ in N{0}.{\cal M}^{+}(D^{2}u)=-\frac{u}{r^{\gamma}}\,\qquad\hbox{ in }\mathbb{R}^{N}\setminus\{0\}\,.

We recall that uC2(N{0})u\in C^{2}(\mathbb{R}^{N}\setminus\{0\}) is a radial solution of the above equation if and only if u=u(r)u=u(r) is a C2((,,,))C^{2}((0,+\infty)) solution of the second order ODE

(2.4) u′′=M+((N1)rK+(u)urγ) in (0,+),u^{\prime\prime}=M_{+}\left(-\frac{(N-1)}{r}K_{+}(u^{\prime})-\frac{u}{r^{\gamma}}\right)\qquad\hbox{ in }(0,+\infty)\,,

where

K+(s)={Λs if s0λs if s<0,M+(s)={1Λs if s01λs if s<0.K_{+}(s)=\left\{\begin{array}[]{ll}\Lambda\,s&\hbox{ if }s\geq 0\\ \lambda\,s&\hbox{ if }s<0\end{array}\right.\,,\qquad M_{+}(s)=\left\{\begin{array}[]{ll}\frac{1}{\Lambda}\,s&\hbox{ if }s\geq 0\\[4.30554pt] \frac{1}{\lambda}\,s&\hbox{ if }s<0\end{array}\right.\,.
Theorem 2.11.

There exists a global solution 𝑂𝑃𝐸𝑁uC2(0,+))u\in C^{2}(0,+\infty)) of equation (2.4), which extends as a continuous function on [0,+)[0,+\infty) satisfying u(0)=1u(0)=1. Moreover, there exists r¯>0\bar{r}>0 such that u(r¯)=0u(\bar{r})=0 and u(r)>0u(r)>0 for 0r<r¯0\leq r<\bar{r}.

Proof.

We begin by proving the local existence of uu near zero. We distinguish the cases γ<1\gamma<1 and γ1\gamma\geq 1.

1st1^{\hbox{st}} case : γ<1\gamma<1

For fixed r0>0r_{0}>0 to be conveniently chosen, let us define the function set

Vr0={uC([0,r0]):|u(r)1|12,u(0)=1}.V_{r_{0}}=\{u\in C([0,r_{0}])\,:\ |u(r)-1|\leq\frac{1}{2},u(0)=1\}.

For uVr0u\in V_{r_{0}}, let us define

T(u)(r):=10r1λsN10su(t)tN1γ𝑑t𝑑s.T(u)(r)\,:=1-\int_{0}^{r}\frac{1}{\lambda s^{N-1}}\int_{0}^{s}u(t)t^{N-1-\gamma}dtds.

We fix r0r_{0} such that r02γλ(Nγ)(2γ)3r_{0}^{2-\gamma}\leq\frac{\lambda(N-\gamma)(2-\gamma)}{3}. Then, it is easy to verify that TT maps Vr0V_{r_{0}} into itself and it is a contraction mapping on it. Let us denote by uVr0u\in V_{r_{0}} its fixed point.

It then follows that uu satisfies

u(r)=1λrN10ru(t)tN1γdtu^{\prime}(r)=-\frac{1}{\lambda r^{N-1}}\int_{0}^{r}u(t)t^{N-1-\gamma}dt

as well as

u′′=uλrγ(N1)ur.u^{\prime\prime}=-\frac{u}{\lambda r^{\gamma}}-(N-1)\frac{u^{\prime}}{r}\,.

Thus, we clearly have u0u^{\prime}\leq 0 and, if we prove that u′′0u^{\prime\prime}\leq 0 as well, then uu is a solution of (2.4) in (0,r0)(0,r_{0}). We observe that u0u^{\prime}\leq 0 implies u1u\leq 1 and, consequently,

u(r)1λrN10rtN1γdt=r1γλ(Nγ).u^{\prime}(r)\geq-\frac{1}{\lambda r^{N-1}}\int_{0}^{r}t^{N-1-\gamma}dt=-\frac{r^{1-\gamma}}{\lambda(N-\gamma)}\,.

Hence

(2.5) u(r)1r2γλ(2γ)(Nγ),u(r)\geq 1-\frac{r^{2-\gamma}}{\lambda(2-\gamma)(N-\gamma)}\,,

which in turn implies

u(r)\displaystyle u^{\prime}(r) \displaystyle\leq 1λrN10r(1t2γλ(2γ)(Nγ))tN1γdt\displaystyle-\frac{1}{\lambda r^{N-1}}\int_{0}^{r}(1-\frac{t^{2-\gamma}}{\lambda(2-\gamma)(N-\gamma)})t^{N-1-\gamma}dt
=\displaystyle= r1γλ(Nγ)+r32γλ2(2γ)(Nγ)(N+22γ)\displaystyle-\frac{r^{1-\gamma}}{\lambda(N-\gamma)}+\frac{r^{3-2\gamma}}{\lambda^{2}(2-\gamma)(N-\gamma)(N+2-2\gamma)}
\displaystyle\leq r1γ2λ(Nγ)\displaystyle-\frac{r^{1-\gamma}}{2\lambda(N-\gamma)}

by the choice of r0r_{0}. Thus, we have proved that

(2.6) r1γλ(Nγ)u(r)r1γ2λ(Nγ)-\frac{r^{1-\gamma}}{\lambda(N-\gamma)}\leq u^{\prime}(r)\leq-\frac{r^{1-\gamma}}{2\lambda(N-\gamma)}

From estimates (2.5) and (2.6), we further deduce

u′′\displaystyle u^{\prime\prime} =\displaystyle= uλrγ(N1)ur\displaystyle-\frac{u}{\lambda r^{\gamma}}-(N-1)\frac{u^{\prime}}{r}
\displaystyle\leq (1r2γλ(2γ)(Nγ))rγλ+(N1)rγλ(Nγ)\displaystyle-\left(1-\frac{r^{2-\gamma}}{\lambda(2-\gamma)(N-\gamma)}\right)\frac{r^{-\gamma}}{\lambda}+(N-1)\frac{r^{-\gamma}}{\lambda(N-\gamma)}
=\displaystyle= (1γ)rγλ(Nγ)+r22γλ2(2γ)(Nγ)\displaystyle-\frac{(1-\gamma)r^{-\gamma}}{\lambda(N-\gamma)}+\frac{r^{2-2\gamma}}{\lambda^{2}(2-\gamma)(N-\gamma)}
\displaystyle\leq (1γ)rγ2λ(Nγ)\displaystyle-\frac{(1-\gamma)r^{-\gamma}}{2\lambda(N-\gamma)}

if we fix r0r_{0} by setting r02γ=λ(1γ)(2γ)3r_{0}^{2-\gamma}=\frac{\lambda(1-\gamma)(2-\gamma)}{3}. By this choice for r0r_{0}, we obtain that uu satisfies equation (2.4) in (0,r0](0,r_{0}] and, moreover, that uC1([0,r0])u\in C^{1}([0,r_{0}]).

2nd2^{\hbox{nd}} case : γ1\gamma\geq 1

In this case, the solution uu is expected to be locally convex near zero. Thus, for vVr0v\in V_{r_{0}}, we define the map

T(v)(r)=10r1ΛsN~+10su(t)tN~+1γ𝑑t𝑑sT(v)(r)=1-\int_{0}^{r}\frac{1}{\Lambda s^{\tilde{N}_{+}-1}}\int_{0}^{s}u(t)t^{{\tilde{N}_{+}-1}-\gamma}dt\,ds

As in the previous case, it is easy to check that if r02γΛ(N~+γ)(2γ)3r_{0}^{2-\gamma}\leq\frac{\Lambda(\tilde{N}_{+}-\gamma)(2-\gamma)}{3}, then TT is a contraction mapping on Vr0V_{r_{0}}. Let uVr0u\in V_{r_{0}} be its fixed point. We then have

u(r)=1ΛrN~+10ru(t)tN~+1γdtu^{\prime}(r)=-\frac{1}{\Lambda r^{\tilde{N}_{+}-1}}\int_{0}^{r}u(t)t^{\tilde{N}_{+}-1-\gamma}dt

and

u′′=(N~+1)ruuΛrγ.u^{\prime\prime}=-\frac{(\tilde{N}_{+}-1)}{r}u^{\prime}-\frac{u}{\Lambda r^{\gamma}}\,.

Thus, in order to prove that uu satisfies (2.4) in (0,r0](0,r_{0}], it is enough to show that u′′0u^{\prime\prime}\geq 0.

By using a bootstrap argument analogous to the one used in the first case, we deduce

r1γΛ(N~+γ)ur1γΛ(N~+γ)+r32γΛ2(N~+γ)(2γ)(N~++22γ)-\frac{r^{1-\gamma}}{\Lambda(\tilde{N}_{+}-\gamma)}\leq u^{\prime}\leq-\frac{r^{1-\gamma}}{\Lambda(\tilde{N}_{+}-\gamma)}+\frac{r^{3-2\gamma}}{\Lambda^{2}(\tilde{N}_{+}-\gamma)(2-\gamma)(\tilde{N}_{+}+2-2\gamma)}

as well as

1r2γΛ(N~+γ)(2γ)u1r2γΛ(N~+γ)(2γ)+r42γ2Λ2(N~+γ)(2γ)2(N~++22γ).1-\frac{r^{2-\gamma}}{\Lambda(\tilde{N}_{+}-\gamma)(2-\gamma)}\leq u\leq 1-\frac{r^{2-\gamma}}{\Lambda(\tilde{N}_{+}-\gamma)(2-\gamma)}+\frac{r^{4-2\gamma}}{2\Lambda^{2}(\tilde{N}_{+}-\gamma)(2-\gamma)^{2}(\tilde{N}_{+}+2-2\gamma)}\,.

We then have

u′′(r)\displaystyle u^{\prime\prime}(r) =\displaystyle= uΛrγ(N~+1)ru\displaystyle-\frac{u}{\Lambda r^{\gamma}}-\frac{(\tilde{N}_{+}-1)}{r}u^{\prime}
\displaystyle\geq γ1Λ(N~+γ)rγ+32γΛ2(N~+γ)(2γ)(N~++22γ)r22γ\displaystyle\frac{\gamma-1}{\Lambda(\tilde{N}_{+}-\gamma)}r^{-\gamma}+\frac{3-2\gamma}{\Lambda^{2}(\tilde{N}_{+}-\gamma)(2-\gamma)(\tilde{N}_{+}+2-2\gamma)}r^{2-2\gamma}
r43γ2Λ3(N~+γ)(2γ)2(N~++22γ)\displaystyle-\frac{r^{4-3\gamma}}{2\Lambda^{3}(\tilde{N}_{+}-\gamma)(2-\gamma)^{2}(\tilde{N}_{+}+2-2\gamma)}

By choosing r0r_{0} such that

r02γΛ(32γ)(2γ)r_{0}^{2-\gamma}\leq\Lambda(3-2\gamma)(2-\gamma)

we obtain in any case that u′′0u^{\prime\prime}\geq 0 in (0,r0](0,r_{0}].

Thus, there exists a local solution uu of equation (2.4) in (0,r0](0,r_{0}], which is positive and satisfies the initial condition u(0)=1u(0)=1. By observing the Lipschitz continuity of the functions K+K_{+} and M+M_{+} and using Cauchy–Lipschitz Theorem, we can extend the solution uu as a global solution in (0,+)(0,+\infty).

It remains to prove that there exists a first point r¯\bar{r} such that u(r¯)=0u(\bar{r})=0 and u(r)>0u(r)>0 for 0r<r¯0\leq r<\bar{r}.

We argue by contradiction, and we assume that u(r)>0u(r)>0 for all r0r\geq 0. Since uu^{\prime} is initially negative, if there exists a first point r1>0r_{1}>0 such that u(r1)=0u^{\prime}(r_{1})=0, then u′′(r1)0u^{\prime\prime}(r_{1})\geq 0. On the other hand, from equation (2.4), we deduce u′′(r1)<0u^{\prime\prime}(r_{1})<0 since u(r1)>0u(r_{1})>0. Hence, one has u(r)<0u^{\prime}(r)<0 for all r>0r>0. From (2.4), it then follows that, independently of the sign of u′′u^{\prime\prime}, one has

u′′+N1ruurγΛ.u^{\prime\prime}+\frac{N-1}{r}u^{\prime}\leq-\frac{ur^{-\gamma}}{\Lambda}\,.

Inspired by [7] and [15], let us introduce the function

y(r)=u(r)u(r)rN1,y(r)=\frac{u^{\prime}(r)}{u(r)}r^{N-1}\,,

which is, then, negative and it satisfies

yrN1γΛy2rN1.y^{\prime}\leq-\frac{r^{N-1-\gamma}}{\Lambda}-\frac{y^{2}}{r^{N-1}}\,.

By integrating between some r1>0r_{1}>0 and rr , we obtain

y(r)+k(r)c1rNγ,y(r)+k(r)\leq-c_{1}r^{N-\gamma}\,,

for some c1>0c_{1}>0 and k(r)=r1ry2(t)tN1𝑑tk(r)=\int_{r_{1}}^{r}\frac{y^{2}(t)}{t^{N-1}}\,dt. This yields in particular y(r)c1rNγy(r)\leq-c_{1}r^{N-\gamma} and therefore, for rr sufficiently large,

(2.7) k(r)c2rN+2(1γ).k(r)\geq c_{2}r^{N+2(1-\gamma)}\,.

On the other hand, we also have

k(r)y(r),k(r)\leq-y(r)\,,

that is

k(r)k(r)rN1k(r)\leq\sqrt{k^{\prime}(r)r^{N-1}}\,

which yields, after integration on (r,+)(r,+\infty),

(2.8) k(r)(N2)rN2.k(r)\leq(N-2)r^{N-2}\,.

Being N+2(1γ)>N2N+2(1-\gamma)>N-2, estimates (2.7) and (2.8) give a contradiction, showing that the constructed solution uu cannot be globally positive in [0,+)[0,+\infty).

As an immediate consequence of the above result and Theorem 2.7, we deduce the following

Corollary 2.12.

Let r¯\bar{r} be defined as in Theorem 2.11. Then λ¯γ(B(0,1){0})=r¯γ2\bar{\lambda}_{\gamma}^{\prime}(B(0,1)\setminus\{0\})=\bar{r}^{\gamma-2}.

Remark 2.13.

Let us observe that, as in the case of equations with continuous coefficients, one could prove the existence of a numerable set of radial eigenvalues, by proving the oscillatory behavior of the solution uu constructed in Theorem 2.11, see [7] and [15].

2.3 The stability of the principal eigenvalue and related eigenfunctions

The results of the present section give, as a corollary, the proof of Theorem 1.1.

Let us start by proving the stability with respect to the ϵ\epsilon-regularization of the singular potential. We recall that rϵ=(r2+ϵ2)12r_{\epsilon}=(r^{2}+\epsilon^{2})^{\frac{1}{2}} and λ¯γϵ=λ¯(F,1rϵγ,B(0,1))\bar{\lambda}_{\gamma}^{\epsilon}=\bar{\lambda}(F,\frac{1}{r_{\epsilon}^{\gamma}},B(0,1)).

Theorem 2.14.

One has

λ¯γ=limϵ0λ¯γϵ.\bar{\lambda}_{\gamma}^{\prime}=\lim_{\epsilon\rightarrow 0}\bar{\lambda}_{\gamma}^{\epsilon}\,.

Furthermore, if {uϵ}\{u_{\epsilon}\} is the sequence of the eigenfunctions associated with the eigenvalue λ¯γϵ\bar{\lambda}_{\gamma}^{\epsilon} and satisfying uϵ(0)=1u_{\epsilon}(0)=1, then, one can extract from {uϵ}\{u_{\epsilon}\} a subsequence uniformly converging on B(0,1)¯\overline{B(0,1)} to the eigenfunction associated with λ¯γ\bar{\lambda}_{\gamma}^{\prime} which takes the value 11 at zero.

Proof.

Let {uϵ}\{u_{\epsilon}\} be the sequence as in the statement. Then, each uϵu_{\epsilon} is a smooth positive function in B(0,1)B(0,1) satisfying in particular

F(D2uϵ)+λ¯γϵuϵrγ0 in B(0,1){0},F(D^{2}u_{\epsilon})+\bar{\lambda}_{\gamma}^{\epsilon}\frac{u_{\epsilon}}{r^{\gamma}}\geq 0\quad\hbox{ in }B(0,1)\setminus\{0\}\,,

so that, by Theorem 2.7, one has λ¯γϵλ¯γ\bar{\lambda}_{\gamma}^{\epsilon}\geq\bar{\lambda}_{\gamma}^{\prime}. Moreover, the sequence {λ¯γϵ}\{\bar{\lambda}_{\gamma}^{\epsilon}\} is monotone increasing with respect to ϵ\epsilon. Thus, we deduce

μ:=limϵ0λ¯γϵλ¯γ.\mu\,:=\lim_{\epsilon\to 0}\bar{\lambda}_{\gamma}^{\epsilon}\geq\bar{\lambda}_{\gamma}^{\prime}\,.

On the other hand, by the monotonicity properties of radially symmetric solutions of elliptic equations, we know that uϵ(r)0u_{\epsilon}^{\prime}(r)\leq 0 for r[0,1]r\in[0,1]. Since

+(D2uϵ)F(D2uϵ){\cal M}^{+}(D^{2}u_{\epsilon})\geq F(D^{2}u_{\epsilon})

we deduce that, independently of the sign of uϵ′′(r)u_{\epsilon}^{\prime\prime}(r), one has

uϵ′′+(N~+1)uϵrλ¯γϵλuϵrϵγ.u_{\epsilon}^{\prime\prime}+(\tilde{N}_{+}-1)\frac{u_{\epsilon}^{\prime}}{r}\geq-\frac{\bar{\lambda}_{\gamma}^{\epsilon}}{\lambda}u_{\epsilon}r_{\epsilon}^{-\gamma}\,.

This implies

(uϵrN~+1)λ¯γϵλuϵrN~+1rϵγλ¯γϵλrN~+1γ,(u_{\epsilon}^{\prime}r^{\tilde{N}_{+}-1})^{\prime}\geq-\frac{\bar{\lambda}_{\gamma}^{\epsilon}}{\lambda}u_{\epsilon}\frac{r^{\tilde{N}_{+}-1}}{r_{\epsilon}^{\gamma}}\geq-\frac{\bar{\lambda}_{\gamma}^{\epsilon}}{\lambda}r^{\tilde{N}_{+}-1-\gamma}\,,

and therefore, by integrating,

0uϵ(r)λ¯γϵλ(N~+γ)r1γ.0\geq u_{\epsilon}^{\prime}(r)\geq-\frac{\bar{\lambda}_{\gamma}^{\epsilon}}{\lambda(\tilde{N}_{+}-\gamma)}r^{1-\gamma}\,.

Hence, on B(0,1)¯\overline{B(0,1)}, the functions uϵu_{\epsilon} are uniformly Lipschitz continuous if γ1\gamma\leq 1, and uniformly (2γ)(2-\gamma)-Hölder continuous if γ>1\gamma>1. In both cases, up to a subsequence, {uϵ}\{u_{\epsilon}\} is uniformly converging to a continuous radial function uC(B(0,1)¯)u\in C(\overline{B(0,1)}) which satisfies u(0)=1u(0)=1 and

F(D2u)+μurγ=0.F(D^{2}u)+\mu\frac{u}{r^{\gamma}}=0.

Hence, uu is C2(B(0,1){0})C^{2}(B(0,1)\setminus\{0\}) and, by the standard strong maximum principle, uu is strictly positive in B(0,1)B(0,1). This yields, by definition, μλ¯γ\mu\leq\bar{\lambda}_{\gamma}^{\prime}. Hence, μ=λ¯γ\mu=\bar{\lambda}_{\gamma}^{\prime} and the conclusion follows from Proposition 2.10.

As a consequence of the previous theorem, we finally obtain the following

Corollary 2.15.

One has

λ¯γ=limδ0λ¯γ(B(0,1)B(0,δ)¯)=λ¯γ.\bar{\lambda}_{\gamma}=\lim_{\delta\to 0}\bar{\lambda}_{\gamma}\left(B(0,1)\setminus\overline{B(0,\delta)}\right)=\bar{\lambda}_{\gamma}^{\prime}\,.
Proof.

We observe that the function δλ¯γ(B(0,1)B(0,δ))\delta\mapsto\bar{\lambda}_{\gamma}\left(B(0,1)\setminus B(0,\delta)\right) is monotone increasing. Moreover, by their own definition, we have that

λ¯γλ¯γλ¯γ(B(0,1)B(0,δ)) for all δ0.\bar{\lambda}_{\gamma}^{\prime}\leq\bar{\lambda}_{\gamma}\leq\bar{\lambda}_{\gamma}\left(B(0,1)\setminus B(0,\delta)\right)\,\quad\hbox{ for all }\delta\geq 0\,.

On the other hand, by Theorem 2.14, for any η>0\eta>0 there exists ϵ0>0\epsilon_{0}>0 such that

λ¯γϵ0λ¯γ+η2.\bar{\lambda}_{\gamma}^{\epsilon_{0}}\leq\bar{\lambda}_{\gamma}^{\prime}+\frac{\eta}{2}\,.

Furthermore, by using the continuity of the principal eigenvalue with respect to the domain for equations with regular coefficients, there exists δ0>0\delta_{0}>0 such that

OPENλ¯γϵ0(B(0,1))B(0,δ0))λ¯γϵ0+η2λ¯γ+η.\bar{\lambda}_{\gamma}^{\epsilon_{0}}(B(0,1))\setminus B(0,\delta_{0}))\leq\bar{\lambda}_{\gamma}^{\epsilon_{0}}+\frac{\eta}{2}\leq\bar{\lambda}_{\gamma}^{\prime}+\eta\,.

Now, since OPENϵλ¯γϵ(B(0,1))B(0,δ0))\epsilon\mapsto\bar{\lambda}^{\epsilon}_{\gamma}\left(B(0,1))\setminus B(0,\delta_{0})\right) decreases when ϵ\epsilon decreases to zero, one gets

OPENλ¯γ(B(0,1)B(0,δ0))λ¯γϵ0(B(0,1))B(0,δ0))λ¯γ+η,\bar{\lambda}_{\gamma}\left(B(0,1)\setminus B(0,\delta_{0})\right)\leq\bar{\lambda}_{\gamma}^{\epsilon_{0}}\left(B(0,1))\setminus B(0,\delta_{0})\right)\leq\bar{\lambda}_{\gamma}^{\prime}+\eta\,,

which gives the conclusion.

3 The case γ=2\gamma=2 : Proof of Theorem 1.2.

The aim of this section is to give the proof of Theorem 1.2.

Let us start by recalling that, in the semilinear case, the eigenvalue related to Laplace operator with an inverse quadratic potential can be defined by a variational approach, i.e. by considering the minimum problem

λ¯2(Δ):=infB(0,1)u2|x|2𝑑x=1uH01(B(0,1))B(0,1)|u|2𝑑x.\bar{\lambda}_{2}(\Delta)\,:\,=\inf_{\stackrel{{\scriptstyle u\in H_{0}^{1}(B(0,1))}}{{\int_{B(0,1)}\frac{u^{2}}{|x|^{2}}dx=1}}}\int_{B(0,1)}|\nabla u|^{2}dx.

In this case, one has

λ¯2(Δ)=(N22)2.\bar{\lambda}_{2}(\Delta)=\left(\frac{N-2}{2}\right)^{2}\,.

Indeed, on the one hand, by Hardy inequality, every function uH01(B(0,1)CLOSEu\in H^{1}_{0}(B(0,1) satisfies

B(0,1)u2|x|2𝑑x(2N2)2B(0,1)|u|2𝑑x\int_{B(0,1)}\frac{u^{2}}{|x|^{2}}dx\leq\left(\frac{2}{N-2}\right)^{2}\int_{B(0,1)}|\nabla u|^{2}dx

and then

λ¯2(Δ)(N22)2.\bar{\lambda}_{2}(\Delta)\geq\left(\frac{N-2}{2}\right)^{2}\,.

On the other hand, for every ϵ>0\epsilon>0, the function uϵ(r)=rN22+ϵ(logr)u_{\epsilon}(r)=r^{-\frac{N-2}{2}+\epsilon}(-\log r) belongs to H01(B(0,1))H_{0}^{1}(B(0,1)) and satisfies

B(0,1)|uϵ|2=[(N22)2+ϵ2]B(0,1)|uϵ|2|x|2𝑑x,\int_{B(0,1)}|\nabla u_{\epsilon}|^{2}=\left[\left(\frac{N-2}{2}\right)^{2}+\epsilon^{2}\right]\int_{B(0,1)}\frac{|u_{\epsilon}|^{2}}{|x|^{2}}dx\,,

so that

λ¯2(Δ)(N22)2+ϵ2,ϵ>0.\bar{\lambda}_{2}(\Delta)\leq\left(\frac{N-2}{2}\right)^{2}+\epsilon^{2}\,,\qquad\forall\,\epsilon>0\,.

As it is well known, the infimum defining λ¯2(Δ)\bar{\lambda}_{2}(\Delta) is not achieved, that is the Dirichlet problem

{Δu=λ¯2(Δ)ur2 in B(0,1)u=0 on B(0,1)\left\{\begin{array}[]{cl}-\Delta u=\bar{\lambda}_{2}(\Delta)\frac{u}{r^{2}}&\hbox{ in }B(0,1)\\[8.61108pt] u=0&\hbox{ on }\partial B(0,1)\end{array}\right.

has not finite energy solutions uH01(B(0,1))u\in H^{1}_{0}(B(0,1)).

A kind of variational approach is possible also in the fully nonlinear framework for the case of Pucci’s operators. From now on, we consider the operator +\mathcal{M}^{+}, being obvious the changes to be made for the operator \mathcal{M}^{-}.

Let us introduce the space of functions

𝒱={uC2([0,1]):u(0)=0,supp(u) compact in [0,1)},\mathcal{V}=\left\{u\in C^{2}([0,1])\,:u^{\prime}(0)=0\,,\ {\rm supp}(u)\hbox{ compact in }[0,1)\right\}\,,

endowed with the norm

u=(01|u|2rN~+1𝑑r)1/2,\|u\|=\left(\int_{0}^{1}|u^{\prime}|^{2}r^{\tilde{N}_{+}-1}dr\right)^{1/2}\,,

and let us denote by 01\mathcal{H}^{1}_{0} the closure of 𝒱\mathcal{V}. Then, for all γ2\gamma\leq 2, we can consider the minimum problem

λ¯γ,var:=inf01u2rN~+1γ𝑑r=1u0101|u|2rN~+1𝑑r.\bar{\lambda}_{\gamma,var}\,:\,=\inf_{\stackrel{{\scriptstyle u\in\mathcal{H}_{0}^{1}}}{{\int_{0}^{1}u^{2}r^{\tilde{N}_{+}-1-\gamma}dr=1}}}\int_{0}^{1}|u^{\prime}|^{2}r^{\tilde{N}_{+}-1}dr\,.

In the next results, we will relate the two values λ¯γ(+)\bar{\lambda}_{\gamma}(\mathcal{M}^{+}) and λ¯γ,var\bar{\lambda}_{\gamma,var}, and we will study their asymptotic behavior as γ2\gamma\to 2.

Theorem 3.1.

One has

λ¯2,var=(N~+22)2.\bar{\lambda}_{2,var}=\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}\,.
Proof.

For any ϵ>0\epsilon>0, let uϵ(r)=rN~+22+ϵ(logr)u_{\epsilon}(r)=r^{-\frac{\tilde{N}_{+}-2}{2}+\epsilon}(-\log r). Then, it is easy to check that uϵ01u_{\epsilon}\in\mathcal{H}_{0}^{1} and a direct computation shows that

01|uϵ|2rN~+1𝑑r=[(N~+22)2+ϵ2]01uϵ2rN~+3𝑑r,\int_{0}^{1}|u_{\epsilon}^{\prime}|^{2}r^{\tilde{N}_{+}-1}dr=\left[\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}+\epsilon^{2}\right]\int_{0}^{1}u_{\epsilon}^{2}r^{\tilde{N}_{+}-3}dr\,,

hence

λ¯2,var(N~+22)2+ϵ2,ϵ>0.\bar{\lambda}_{2,var}\leq\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}+\epsilon^{2}\,,\qquad\forall\,\epsilon>0\,.

On the other hand, we observe that the function u=rN~+22(logr)u=r^{-\frac{\tilde{N}_{+}-2}{2}}(-\log r) satisfies, for r>0r>0 ,

u′′+(N~+1)ur=(N~+22)2ur2.u^{\prime\prime}+(\tilde{N}_{+}-1)\frac{u^{\prime}}{r}=-\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}ur^{-2}.

Let us multiply the above equation by v2urN~+1\frac{v^{2}}{u}r^{\tilde{N}_{+}-1}, where v𝒱v\in\mathcal{V} is arbitrarily fixed. Since N~+>2\tilde{N}_{+}>2, we have that urN~+1u\frac{u^{\prime}r^{\tilde{N}_{+}-1}}{u} tends to zero as r0r\to 0. As a consequence, integrating by parts, we get

(N~+22)201v2rN~+3dr=01(uuvv)2rN~+1dr01(v)2rN~+1dr,-\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}\int_{0}^{1}v^{2}r^{\tilde{N}_{+}-3}dr=\int_{0}^{1}\left(\frac{u^{\prime}}{u}v-v^{\prime}\right)^{2}r^{\tilde{N}_{+}-1}dr-\int_{0}^{1}(v^{\prime})^{2}r^{\tilde{N}_{+}-1}dr\,,

which yields, by the arbitrariness of v𝒱v\in\mathcal{V},

λ¯2,var(N~+22)2.\bar{\lambda}_{2,var}\geq\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}\,.

In order to establish the relationship between λ¯γ,var\bar{\lambda}_{\gamma,var} and λ¯γ\bar{\lambda}_{\gamma} we need to investigate on the monotonicity and convexity properties of the functions uu realizing the infimum in the definition of λ¯γ,var\bar{\lambda}_{\gamma,var}.

Proposition 3.2.

Let 1<γ<21<\gamma<2 and assume that uγ01u_{\gamma}\in\mathcal{H}^{1}_{0}, with uγ0u_{\gamma}\geq 0, realizes the infimum defining λ¯γ,var\bar{\lambda}_{\gamma,var}. Then, uγC2((0,1])u_{\gamma}\in C^{2}((0,1]) is bounded, uγ0u_{\gamma}^{\prime}\leq 0 and uγ′′0u_{\gamma}^{\prime\prime}\geq 0 in (0,1)(0,1).

Proof.

Since uγu_{\gamma} is a minimum, for any v01v\in\mathcal{H}^{1}_{0} one has

01uγvrN~+1=λ¯γ,var01uγvrN~+1γ.\int_{0}^{1}u_{\gamma}^{\prime}v^{\prime}r^{\tilde{N}_{+}-1}=\bar{\lambda}_{\gamma,var}\int_{0}^{1}u_{\gamma}vr^{\tilde{N}_{+}-1-\gamma}.

In particular, uγu_{\gamma} satisfies in the distributional sense

(3.1) (uγrN~+1)=λ¯γ,varuγrN~+1γ-(u^{\prime}_{\gamma}r^{\tilde{N}_{+}-1})^{\prime}=\bar{\lambda}_{\gamma,var}u_{\gamma}r^{\tilde{N}_{+}-1-\gamma}

By regularity theory, this implies that uγu_{\gamma} belongs to C2((0,1])C^{2}((0,1]), it is strictly positive in (0,1)(0,1) and it satisfies uγ(1)=0u_{\gamma}(1)=0. Let us prove that uγu_{\gamma} is bounded and that it can be extended as a continuous function on [0,1][0,1]. Indeed, by multiplying equation (3.1) by a smooth function vC2([0,1])v\in C^{2}([0,1]), having compact support in [0,1)[0,1) and satisfying v(0)0v(0)\neq 0, and integrating on [ϵ,1][\epsilon,1] for ϵ>0\epsilon>0, one has

λ¯γ,varϵ1uγ(r)rN~+1γv(r)𝑑r=ϵ1uγ(r)rN~+1v(r)𝑑r+uγ(ϵ)ϵN~+1v(ϵ).\bar{\lambda}_{\gamma,var}\int_{\epsilon}^{1}u_{\gamma}(r)r^{\tilde{N}_{+}-1-\gamma}v(r)\,dr=\int_{\epsilon}^{1}u^{\prime}_{\gamma}(r)r^{\tilde{N}_{+}-1}v^{\prime}(r)\,dr+u^{\prime}_{\gamma}(\epsilon)\epsilon^{\tilde{N}_{+}-1}v(\epsilon)\,.

Letting ϵ\epsilon go to zero, we deduce limϵ0uγ(ϵ)ϵN~+1=0\lim_{\epsilon\rightarrow 0}u_{\gamma}^{\prime}(\epsilon)\epsilon^{\tilde{N}_{+}-1}=0. It then follows, again from (3.1), that uγ(r)0u^{\prime}_{\gamma}(r)\leq 0 and that there exists some positive constant c0c_{0} such that

uγ(r)c0r1N~+ for r(0,1].u^{\prime}_{\gamma}(r)\geq-c_{0}\,r^{1-\tilde{N}_{+}}\qquad\hbox{ for }r\in(0,1]\,.

This implies that

uγ(r)=r1uγ(s)dsc0r1s1N~+dsd0r2N~+u_{\gamma}(r)=-\int_{r}^{1}u^{\prime}_{\gamma}(s)\,ds\leq c_{0}\int_{r}^{1}s^{1-\tilde{N}_{+}}ds\leq d_{0}r^{2-\tilde{N}_{+}}

with d0=c0N~+2>0d_{0}=\frac{c_{0}}{\tilde{N}_{+}-2}>0, which, in turn, yields

uγ(r)rN~+1=λ¯γ,var0ruγ(s)sN~+1γdsλ¯γ,vard00rs1γds=c1r2γ.u^{\prime}_{\gamma}(r)r^{\tilde{N}_{+}-1}=-\bar{\lambda}_{\gamma,var}\int_{0}^{r}u_{\gamma}(s)s^{\tilde{N}_{+}-1-\gamma}ds\geq-\bar{\lambda}_{\gamma,var}\,d_{0}\int_{0}^{r}s^{1-\gamma}ds=-c_{1}r^{2-\gamma}\,.

Thus, we have

uγ(r)c1r1N~++2γu^{\prime}_{\gamma}(r)\geq-c_{1}\,r^{1-\tilde{N}_{+}+2-\gamma}

and, then,

uγ(r)d1r2N~++2γ.u_{\gamma}(r)\leq d_{1}r^{2-\tilde{N}_{+}+2-\gamma}\,.

Iterating the above inequalities, we obtain that for all integers j0j\geq 0 such that 2N~++j(2γ)<02-\tilde{N}_{+}+j(2-\gamma)<0, there exist positive constants cjc_{j} and djd_{j} satisfying

(3.2) uγ(r)cjr1N~++j(2γ),uγ(r)djr2N~++j(2γ).u^{\prime}_{\gamma}(r)\geq-c_{j}\,r^{1-\tilde{N}_{+}+j(2-\gamma)}\,,\quad u_{\gamma}(r)\leq d_{j}r^{2-\tilde{N}_{+}+j(2-\gamma)}\,.

Now, if there exists jj\in{\mathbb{N}} such that 2N~++j(2γ)=02-\tilde{N}_{+}+j(2-\gamma)=0, i.e. if N~+22γ\frac{\tilde{N}_{+}-2}{2-\gamma}\in{\mathbb{N}}, then, by integrating the estimates obtained at the (j1)(j-1)-th step, we obtain

uγ(r)cjr1,uγ(r)dj(lnr).u^{\prime}_{\gamma}(r)\geq-c_{j}\,r^{-1}\,,\quad u_{\gamma}(r)\leq d_{j}\,(-\ln r)\,.

Integrating once more, we finally deduce

uγ(r)cj+1(lnr)r1γuγ(r)dj+1=cj+1(2γ)2.u^{\prime}_{\gamma}(r)\geq-c_{j+1}(-\ln r)r^{1-\gamma}\Longrightarrow u_{\gamma}(r)\leq d_{j+1}=\frac{c_{j+1}}{(2-\gamma)^{2}}\,.

On the other hand, if N~+22γ\frac{\tilde{N}_{+}-2}{2-\gamma} is not integer, by integrating estimates (3.2) for j=[N~+22γ]j=\left[\frac{\tilde{N}_{+}-2}{2-\gamma}\right], we obtain

uγ(r)cj+1r1N~++(j+1)(2γ)uγ(r)dj+1=cj+12N~++(j+1)(2γ).u^{\prime}_{\gamma}(r)\geq-c_{j+1}r^{1-\tilde{N}_{+}+(j+1)(2-\gamma)}\Longrightarrow u_{\gamma}(r)\leq d_{j+1}=\frac{c_{j+1}}{2-\tilde{N}_{+}+(j+1)(2-\gamma)}\,.

This shows that, in any case, uγu_{\gamma} is bounded.

Let us finally prove that uγ′′0u_{\gamma}^{\prime\prime}\geq 0. We introduce the function

yγ(r):=(N~+1)uγ(r)+λ¯γ,varr1γuγ(r),y_{\gamma}(r)\,:=(\tilde{N}_{+}-1)u_{\gamma}^{\prime}(r)+{\bar{\lambda}_{\gamma,var}}r^{1-\gamma}u_{\gamma}(r)\,,

which verifies yγ=ruγ′′y_{\gamma}=-ru^{\prime\prime}_{\gamma}. Hence, we need to prove that yγ(r)0y_{\gamma}(r)\leq 0 for r(0,1]r\in(0,1]. An easy computation shows that

yγ(r)+(N~+1)yγ(r)r=λ¯γ,var(uγ(r)r1γ+(1γ)uγ(r)rγ)0,y_{\gamma}^{\prime}(r)+(\tilde{N}_{+}-1)\frac{y_{\gamma}(r)}{r}={\bar{\lambda}_{\gamma,var}}\left(u^{\prime}_{\gamma}(r)r^{1-\gamma}+(1-\gamma)u_{\gamma}(r)r^{-\gamma}\right)\leq 0\,,

so that

(yγ(r)rN~+1)0.(y_{\gamma}(r)r^{\tilde{N}_{+}-1})^{\prime}\leq 0\,.

Since uγu_{\gamma} is bounded and c0r1γuγ(r)0-c_{0}r^{1-\gamma}\leq u^{\prime}_{\gamma}(r)\leq 0, we deduce that yγ(r)rN~+10y_{\gamma}(r)r^{\tilde{N}_{+}-1}\rightarrow 0 as r0r\to 0. Hence, yγ(r)0y_{\gamma}(r)\leq 0 for r>0r>0.

Corollary 3.3.

Let γ]1,2[\gamma\in]1,2[. Then

λ¯γ(+)=Λλ¯γ,var.\bar{\lambda}_{\gamma}(\mathcal{M}^{+})=\Lambda\,\bar{\lambda}_{\gamma,var}\,.
Proof.

It is not difficult to prove that the infimum defining λ¯γ,var\bar{\lambda}_{\gamma,var} is achieved for 1<γ<21<\gamma<2. Thus, there exists vγ01v_{\gamma}\in\mathcal{H}^{1}_{0}, which can be assumed to be positive in [0,1)[0,1), and which satisfies in (0,1)(0,1)

Λvγ′′+λN1rvγ=Λλ¯γ,varvγrγ.\Lambda v_{\gamma}^{\prime\prime}+\lambda\frac{N-1}{r}v_{\gamma}^{\prime}=-\Lambda\,\bar{\lambda}_{\gamma,var}v_{\gamma}r^{-\gamma}.

By Proposition 3.2, we have that vγv_{\gamma} is bounded, vγ0v_{\gamma}^{\prime}\leq 0 and vγ′′0v_{\gamma}^{\prime\prime}\geq 0, so that vγv_{\gamma} satisfies

+(D2vγ)+Λλ¯γ,varvγrγ=0 in B(0,1){0}.{\cal M}^{+}(D^{2}v_{\gamma})+\Lambda\,\bar{\lambda}_{\gamma,var}v_{\gamma}r^{-\gamma}=0\quad\hbox{ in }B(0,1)\setminus\{0\}\,.

By definition, it then follows that λ¯γ(+)=λ¯γ(+)Λλ¯γ,var\bar{\lambda}_{\gamma}(\mathcal{M}^{+})=\bar{\lambda}_{\gamma}^{\prime}(\mathcal{M}^{+})\geq\Lambda\,\bar{\lambda}_{\gamma,var}. Furthermore, analyzing the boundary condition, we get, by regularity, that vγ(1)=0v_{\gamma}(1)=0 in the classical sense. If, by contradiction, Λλ¯γ,var<λ¯γ(+)\Lambda\,\bar{\lambda}_{\gamma,var}<\bar{\lambda}_{\gamma}^{\prime}(\mathcal{M}^{+}), then Theorem 2.7 would give vγ0v_{\gamma}\leq 0 in B(0,1)B(0,1), a contradiction.

Corollary 3.4.

One has

limγ2λ¯γ(+)=Λ(N~+22)2.\lim_{\gamma\rightarrow 2}\bar{\lambda}_{\gamma}(\mathcal{M}^{+})=\Lambda\,\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}\,.
Proof.

By Theorem 3.1 and Corollary 3.3, it is sufficient to prove that λ¯γ,varλ¯2,var\bar{\lambda}_{\gamma,var}\rightarrow\bar{\lambda}_{2,var} as γ2\gamma\to 2.

We first observe that, by their own definition, λ¯2,varλ¯γ,var\bar{\lambda}_{2,var}\leq\bar{\lambda}_{\gamma,var}.

On the other hand, for any ϵ>0\epsilon>0 there exists v01v\in\mathcal{H}^{1}_{0} such that

01|v|2rN~+1𝑑r(λ¯2,var+ϵ)01|v|2rN~+3𝑑r.\int_{0}^{1}|v^{\prime}|^{2}r^{\tilde{N}_{+}-1}dr\leq(\bar{\lambda}_{2,var}+\epsilon)\int_{0}^{1}|v|^{2}r^{\tilde{N}_{+}-3}dr\,.

Moreover, there exists γ0\gamma_{0} sufficiently close to 22 in order that, for γγ0\gamma\geq\gamma_{0} ,

01|v|2rN~+1γ𝑑r(1ϵ)01|v|2rN~+3𝑑r.\int_{0}^{1}|v|^{2}r^{\tilde{N}_{+}-1-\gamma}dr\geq(1-\epsilon)\int_{0}^{1}|v|^{2}r^{\tilde{N}_{+}-3}dr\,.

Thus, one has

01|v|2rN~+1𝑑r(λ¯2,var+ϵ)(1ϵ)101|v|2rN~+1γ𝑑r\int_{0}^{1}|v^{\prime}|^{2}r^{\tilde{N}_{+}-1}dr\leq(\bar{\lambda}_{2,var}+\epsilon)(1-\epsilon)^{-1}\int_{0}^{1}|v|^{2}r^{\tilde{N}_{+}-1-\gamma}dr

which yields

λ¯γ,var(λ¯2,var+ϵ)(1ϵ)1.\bar{\lambda}_{\gamma,var}\leq(\bar{\lambda}_{2,var}+\epsilon)(1-\epsilon)^{-1}\,.

We are now ready to prove statement (i) of Theorem 1.2.

Theorem 3.5.

One has

λ¯2(+)=Λ(N~+22)2\bar{\lambda}_{2}(\mathcal{M}^{+})=\Lambda\,\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}

and the function u(r)=rN~+22(lnr)u(r)=r^{-\frac{\tilde{N}_{+}-2}{2}}(-\ln r) is an explicit solution of

{+(D2u)+λ¯γurγ=0 in B(0,1){0}u=0 on B(0,1)\left\{\begin{array}[]{cl}\mathcal{M}^{+}(D^{2}u)+\bar{\lambda}_{\gamma}\frac{u}{r^{\gamma}}=0&\hbox{ in }\ B(0,1)\setminus\{0\}\\[4.30554pt] u=0&\hbox{ on }\ \partial B(0,1)\end{array}\right.
Proof.

For any positive constants c1c_{1} and c2c_{2}, let us consider the function

(3.3) u(r)=rN~+22(c1(lnr)+c2).u(r)=r^{-\frac{\tilde{N}_{+}-2}{2}}(c_{1}(-\ln r)+c_{2}).

An easy computation, analogous to the one made in the proof of Theorem 3.1, leads to

+(D2u)+Λ(N~+22)2ur2=0 in B(0,1){0}.\mathcal{M}^{+}(D^{2}u)+\Lambda\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}\frac{u}{r^{2}}=0\quad\hbox{ in }B(0,1)\setminus\{0\}\,.

This gives, by definition, that

λ¯2(+)Λ(N~+22)2.\bar{\lambda}_{2}(\mathcal{M}^{+})\geq\Lambda\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}\,.

On the other hand, by observing that λ¯γλ¯2\bar{\lambda}_{\gamma}\geq\bar{\lambda}_{2} for all γ2\gamma\leq 2 and by using Corollary 3.4, we also have

λ¯2(+)limγ2λ¯γ(+)=Λ(N~+22)2.\bar{\lambda}_{2}(\mathcal{M}^{+})\leq\ \lim_{\gamma\to 2}\bar{\lambda}_{\gamma}(\mathcal{M}^{+})=\Lambda\left(\frac{\tilde{N}_{+}-2}{2}\right)^{2}\,.

As a consequence of Corollary 3.4 and Theorem 3.5, we immediately deduce the first stability property of λ¯2(+)\bar{\lambda}_{2}(\mathcal{M}^{+}) stated in Theorem 1.2-(ii). The other ones are given by by the following result.

Corollary 3.6.

For the operators F=±F=\mathcal{M}^{\pm}, one has

limδ0λ¯2(B(0,1)B(0,δ)¯)=λ¯2=limϵ0λ¯2ϵ.\lim_{\delta\rightarrow 0}\bar{\lambda}_{2}(B(0,1)\setminus\overline{B(0,\delta)})=\bar{\lambda}_{2}=\lim_{\epsilon\to 0}\bar{\lambda}^{\epsilon}_{2}\,.
Proof.

We observe that

λ¯2(B(0,1)B(0,δ)¯)λ¯2\bar{\lambda}_{2}(B(0,1)\setminus\overline{B(0,\delta)})\geq\bar{\lambda}_{2}

and that λ¯2(B(0,1)B(0,δ)¯)\bar{\lambda}_{2}(B(0,1)\setminus\overline{B(0,\delta)}) is decreasing with respect to δ\delta. Hence,

limδ0λ¯2(B(0,1)OPENB(0,δ))¯λ¯2CLOSE.\lim_{\delta\rightarrow 0}\bar{\lambda}_{2}(B(0,1)\setminus\overline{B(0,\delta))}\geq\bar{\lambda}_{2}.

In order to prove the reverse inequality, we can use Theorem 3.5 jointly with Corollary 3.4, as well as Corollary 2.15. Indeed, for any η>0\eta>0 let γ0<2\gamma_{0}<2 such that, for all γ0γ<2\gamma_{0}\leq\gamma<2, one has

λ¯2λ¯γη.\bar{\lambda}_{2}\geq\bar{\lambda}_{\gamma}-\eta\,.

Moreover, let δ0=δ(γ,η)\delta_{0}=\delta(\gamma,\eta) be such that, for any δ<δ0\delta<\delta_{0},

λ¯γ(B(0,1)B(0,δ)¯)λ¯γ+η.\bar{\lambda}_{\gamma}(B(0,1)\setminus\overline{B(0,\delta)})\leq\bar{\lambda}_{\gamma}+\eta\,.

It then follows

λ¯2λ¯γ(B(0,1)B(0,δ)¯)2ηλ¯2(B(0,1)B(0,δ)¯)2η.\bar{\lambda}_{2}\geq\bar{\lambda}_{\gamma}(B(0,1)\setminus\overline{B(0,\delta)})-2\eta\geq\bar{\lambda}_{2}(B(0,1)\setminus\overline{B(0,\delta)})-2\eta\,.

The assertion concerning limλ¯2ϵ\lim\bar{\lambda}^{\epsilon}_{2} can be proved in the same way by using Theorem 2.14.

In order to complete the proof of Theorem 1.2, it is enough to observe that statement (iii) immediately follows from statement (i), the definition of λ¯2(F)\bar{\lambda}_{2}(F) and the ellipticity inequalities (1.8).

4 The case γ>2\gamma>2 : Proof of Theorem 1.3

This section is completely devoted to the proof of Theorem 1.3. Let us assume, by contradiction, that for γ>2\gamma>2 there exists uC2(B(0,1){0})u\in C^{2}(B(0,1)\setminus\{0\}) positive and radial, satisfying

(D2u)μurγ in B(0,1){0},{\cal M}^{-}(D^{2}u)\leq-\mu ur^{-\gamma}\quad\hbox{ in }B(0,1)\setminus\{0\}\,,

for some μ>0\mu>0.

Then, arguing as in the proof of Lemma 2.1, it follows that u(r)u^{\prime}(r) has constant sign in a right neighborhood of zero. If u(r)0u^{\prime}(r)\geq 0 for rr small, then, by the equation, u′′(r)0u^{\prime\prime}(r)\leq 0 and then we would have

(urN~+1)μurN~+1γΛ.(u^{\prime}r^{\tilde{N}_{+}-1})^{\prime}\leq-\frac{\mu ur^{\tilde{N}_{+}-1-\gamma}}{\Lambda}\,.

This implies that urN~+1u^{\prime}r^{\tilde{N}_{+}-1} has a nonnegative limit for r0r\to 0, and if this limit is strictly positive, we get that uu becomes large negative as r0r\to 0, a contradiction. Then the limit is zero, and then from the inequality above we get u(r)rN~1<0u^{\prime}(r)r^{\tilde{N}-1}<0, a contradiction again. Therefore, we have u(r)0u^{\prime}(r)\leq 0 for r>0r>0 sufficiently small. Then, we observe that, whatever is the sign of u′′u^{\prime\prime}, one has

u′′+(N~1)urμΛurγ.u^{\prime\prime}+(\tilde{N}_{-}-1)\frac{u^{\prime}}{r}\leq-\frac{\mu}{\Lambda}u\,r^{-\gamma}\,.

Thus,

(4.1) (urN~1)μΛurN~1γ<0,(u^{\prime}r^{{\tilde{N}_{-}-1}})^{\prime}\leq-\frac{\mu}{\Lambda}u\,r^{\tilde{N}_{-}-1-\gamma}<0\,,

and then u(r)rN~1u^{\prime}(r)r^{{\tilde{N}_{-}-1}} has a non positive limit as r0r\to 0. If the limit is strictly negative, then u(r)rN~1c<0u^{\prime}(r)r^{{\tilde{N}_{-}-1}}\leq-c<0 in a neighborhood of zero. Then, we get

u(r)c1r2N~u(r)\geq c_{1}r^{2-{\tilde{N}_{-}}}

for rr small and a positive c1c_{1}. Hence, by integrating (4.1) between rr and s>rs>r sufficiently small, we deduce

u(s)sN~1+u(r)rN~1c2rst1γ𝑑t=c2s2γr2γ2γ-u^{\prime}(s)s^{{\tilde{N}_{-}-1}}+u^{\prime}(r)r^{{\tilde{N}_{-}-1}}\geq c_{2}\int_{r}^{s}t^{1-\gamma}dt=c_{2}\frac{s^{2-\gamma}-r^{2-\gamma}}{2-\gamma}

and, since γ>2\gamma>2, this yields u(r)>0u^{\prime}(r)>0 for rr small enough: a contradiction.

Thus, one has limr0urN~1=0\lim_{r\to 0}u^{\prime}r^{{\tilde{N}_{-}-1}}=0 and, by (4.1), u(r)<0u^{\prime}(r)<0 for r>0r>0.

Next, by an inductive argument analogous to the one used in the proof of Proposition 3.2, we prove that for all integer j0j\geq 0 such that N~2+j(2γ)>0{\tilde{N}_{-}-2}+j(2-\gamma)>0 and for rr sufficiently small, one has, for some cj>0c_{j}>0,

(4.2) u(r)cjrj(2γ).u(r)\geq c_{j}r^{j(2-\gamma)}.

Indeed, (4.2) holds true for j=0j=0, since u<0u^{\prime}<0 and uu is positive. Let us suppose that (4.2) is true for jj and that N~2+(j+1)(2γ)>0{\tilde{N}_{-}-2}+(j+1)(2-\gamma)>0. Then, by (4.1),

u(r)rN~1μΛcj0rsN~1+j(2γ)γ𝑑s=μΛcjN~2+(j+1)(2γ)rN~2+(j+1)(2γ),-u^{\prime}(r)r^{\tilde{N}_{-}-1}\geq\frac{\mu}{\Lambda}c_{j}\int_{0}^{r}s^{\tilde{N}_{-}-1+j(2-\gamma)-\gamma}ds=\frac{\mu}{\Lambda}\frac{c_{j}}{\tilde{N}_{-}-2+(j+1)(2-\gamma)}r^{{\tilde{N}_{-}-2}+(j+1)(2-\gamma)}\,,

which, by integration, yields (4.2) for j+1j+1.

Now, let us assume that N~2γ2\frac{\tilde{N}_{-}-2}{\gamma-2} is not integer. Then, using estimate (4.2) with j=[N~2γ2]j=\left[\frac{\tilde{N}_{-}-2}{\gamma-2}\right] jointly with (4.1), we deduce for r0>r>0r_{0}>r>0

u(r0)r0N~1+u(r)rN~1μcjΛ(N~2+(j+1)(2γ))(sN~2+(j+1)(2γ)|rr0CLOSE.-u^{\prime}(r_{0})r_{0}^{{\tilde{N}_{-}-1}}+u^{\prime}(r)r^{{\tilde{N}_{-}-1}}\geq\frac{\mu\,c_{j}}{\Lambda\,\left(\tilde{N}_{-}-2+(j+1)(2-\gamma)\right)}\left(s^{\tilde{N}_{-}-2+(j+1)(2-\gamma)}\right|_{r}^{r_{0}}\,.

Since N~2+(j+1)(2γ)<0\tilde{N}_{-}-2+(j+1)(2-\gamma)<0, this yields the contradiction

limr0u(r)rN~1=+.\lim_{r\to 0}u^{\prime}(r)r^{{\tilde{N}_{-}-1}}=+\infty\,.

On the other hand, if N~2γ2=j+1\frac{\tilde{N}_{-}-2}{\gamma-2}=j+1 is integer, then N~2+j(2γ)=γ2>0\tilde{N}_{-}-2+j(2-\gamma)=\gamma-2>0, and from (4.2) it follows that

u(r)cjrγN~,u(r)\geq c_{j}r^{\gamma-\tilde{N}_{-}}\,,

hence

u(r)rN~1γcjr1.u(r)r^{\tilde{N}_{-}-1-\gamma}\geq c_{j}r^{-1}\,.

From (4.1) we then deduce, for 0<r<r00<r<r_{0},

u(r0)r0N~1+u(r)rN~1μcjΛ(lnr0lnr)-u^{\prime}(r_{0})r_{0}^{\tilde{N}_{-}-1}+u^{\prime}(r)r^{\tilde{N}_{-}-1}\geq\frac{\mu\,c_{j}}{\Lambda}\left(\ln r_{0}-\ln r\right)

and we reach, also in this case, the contradiction

limr0u(r)rN~1=+.\lim_{r\to 0}u^{\prime}(r)r^{{\tilde{N}_{-}-1}}=+\infty\,.

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